ID = CDS/P/2MASS/H hips_doi = 10.26093/cds/aladin/2thy-66 creator_did = ivo://CDS/P/2MASS/H hips_initial_ra = 266.40499479 hips_initial_dec = -28.936173970 hips_initial_fov = 58.63230142835039 hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_skyval_method = SKYVAL hips_skyval_value = -0.5 100.0 -3146.3114318847656 13218.762664794922 hips_overlay = mean hips_hierarchy = median hips_creator = Oberto A. (CDS) hips_copyright = CNRS/Unistra hips_version = 1.4 hips_release_date = 2021-02-23T18:05Z hips_frame = equatorial hips_order = 9 hips_order_min = 0 hips_tile_width = 512 hips_tile_format = jpeg fits dataproduct_type = image hips_pixel_cut = -0.5 100 moc_access_url = http://alasky.u-strasbg.fr/2MASS/H/Moc.fits hips_status = public master clonableOnce obs_title = 2MASS H (1.66um) obs_collection = The Two Micron All Sky Survey - H band (2MASS H) obs_description = 2MASS has uniformly scanned the entire sky in three near-infrared bands to detect and characterize point sources brighter than about 1 mJy in each band, with signal-to-noise ratio (SNR) greater than 10, using a pixel size of 2.0". This has achieved an 80,000-fold improvement in sensitivity relative to earlier surveys. 2MASS used two highly-automated 1.3-m telescopes, one at Mt. Hopkins, AZ, and one at CTIO, Chile. Each telescope was equipped with a three-channel camera, each channel consisting of a 256x256 array of HgCdTe detectors, capable of observing the sky simultaneously at J (1.25 microns), H (1.65 microns), and Ks (2.17 microns). The University of Massachusetts (UMass) was responsible for the overall management of the project, and for developing the infrared cameras and on-site computing systems at both facilities. The Infrared Processing and Analysis Center (IPAC) is responsible for all data processing through the Production Pipeline, and construction and distribution of the data products. Funding is provided primarily by NASA and the NSF obs_copyright_url = http://www.ipac.caltech.edu/2mass/ obs_ack = University of Massachusetts & IPAC/Caltech bib_reference = 2006AJ....131.1163S bib_reference_url = http://simbad.u-strasbg.fr/simbad/sim-ref?bibcode=2006AJ....131.1163S obs_copyright = University of Massachusetts & IPAC/Caltech t_min = 50600 t_max = 51941 obs_regime = Infrared em_min = 1.525E-6 em_max = 1.798E-6 hips_data_range = -3146 13219 prov_progenitor = IPAC/NASA client_category = Image/Infrared/2MASS hips_builder = Aladin/HipsGen v11.023 hips_pixel_scale = 2.236E-4 s_pixel_scale = 2.777E-4 moc_sky_fraction = 1 hips_estsize = 4631264878 hipsgen_date = 2020-05-29T23:00Z hipsgen_params = in=2MASSh out=Hips-H creator_did=ivo://CDS-test/P/2MASS/H -f "hips_pixel_cut=-0.5 100 log" skyval=SKYVAL "fitskeys=ORDATE SCANNO SCANDIR" maxthread=64 hips_frame=equatorial TILES PNG DETAILS hips_creation_date = 2013-05-06T20:36Z hips_service_url = https://alasky.cds.unistra.fr/2MASS/H hips_progenitor_url = https://alasky.cds.unistra.fr/2MASS/H/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/2MASS/H hips_status_1 = public mirror clonableOnce hips_service_url_2 = https://irsa.ipac.caltech.edu/data/hips/CDS/2MASS/H hips_status_2 = public mirror unclonable hips_tile_format_2 = jpeg moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 9 obs_initial_ra = 266.40499479 obs_initial_dec = -28.936173970 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288569682 ID = CDS/P/2MASS/J hips_doi = 10.26093/cds/aladin/3ntd-6fa creator_did = ivo://CDS/P/2MASS/J hips_initial_ra = 266.40499479 hips_initial_dec = -28.936173970 hips_initial_fov = 58.63230142835039 hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_skyval_method = SKYVAL hips_skyval_value = -0.5 100.0 -357.66149139404297 1421.6846084594727 hips_overlay = mean hips_hierarchy = median hips_hierarchy = mean hips_creator = Oberto A. (CDS) hips_copyright = CNRS/Unistra obs_title = 2MASS J (1.23um) hips_builder = Aladin/HipsGen v11.023 hips_builder = Aladin/HipsGen v11.023 hips_version = 1.4 hips_creation_date = 2014-02-11T11:28Z hips_release_date = 2021-02-24T06:06Z hips_frame = equatorial hips_order = 9 hips_order_min = 0 hips_tile_width = 512 dataproduct_type = image moc_access_url = http://alasky.u-strasbg.fr/2MASS/J/Moc.fits hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_cut = -0.5 40 hips_data_range = -357.7 1422 obs_collection = The Two Micron All Sky Survey - J band (2MASS J) obs_description = 2MASS has uniformly scanned the entire sky in three near-infrared bands to detect and characterize point sources brighter than about 1 mJy in each band, with signal-to-noise ratio (SNR) greater than 10, using a pixel size of 2.0". This has achieved an 80,000-fold improvement in sensitivity relative to earlier surveys. 2MASS used two highly-automated 1.3-m telescopes, one at Mt. Hopkins, AZ, and one at CTIO, Chile. Each telescope was equipped with a three-channel camera, each channel consisting of a 256x256 array of HgCdTe detectors, capable of observing the sky simultaneously at J (1.25 microns), H (1.65 microns), and Ks (2.17 microns). The University of Massachusetts (UMass) was responsible for the overall management of the project, and for developing the infrared cameras and on-site computing systems at both facilities. The Infrared Processing and Analysis Center (IPAC) is responsible for all data processing through the Production Pipeline, and construction and distribution of the data products. Funding is provided primarily by NASA and the NSF obs_copyright_url = http://www.ipac.caltech.edu/2mass/ obs_ack = University of Massachusetts & IPAC/Caltech bib_reference = 2006AJ....131.1163S bib_reference_url = http://simbad.u-strasbg.fr/simbad/sim-ref?bibcode=2006AJ....131.1163S obs_copyright = University of Massachusetts & IPAC/Caltech t_min = 50600 t_max = 51941 obs_regime = Infrared em_min = 1.147E-6 em_max = 1.323E-6 prov_progenitor = IPAC/NASA client_category = Image/Infrared/2MASS hips_pixel_scale = 2.236E-4 s_pixel_scale = 2.777E-4 moc_sky_fraction = 1 hips_estsize = 4593684487 hipsgen_date = 2020-06-16T12:47Z hipsgen_date = 2020-06-22T09:53Z hipsgen_params = in=2MASSj out=Hips-J creator_did=ivo://CDS-test/P/2MASS/J -f "hips_pixel_cut=-0.5 40 log" fading=true skyval=SKYVAL maxthread=64 hips_frame=equatorial JPEG hips_service_url = https://alasky.cds.unistra.fr/2MASS/J hips_progenitor_url = https://alasky.cds.unistra.fr/2MASS/J/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/2MASS/J hips_status_1 = public mirror clonableOnce hips_service_url_2 = https://irsa.ipac.caltech.edu/data/hips/CDS/2MASS/J hips_status_2 = public mirror unclonable hips_tile_format_2 = jpeg moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 9 obs_initial_ra = 266.40499479 obs_initial_dec = -28.936173970 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288568394 ID = CDS/P/2MASS/K hips_doi = 10.26093/cds/aladin/2ea3-abw creator_did = ivo://CDS/P/2MASS/K hips_initial_ra = 266.40499479 hips_initial_dec = -28.936173970 hips_initial_fov = 58.63230142835039 hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_skyval_method = SKYVAL hips_skyval_value = -0.5 100.0 -2660.7283935546875 9046.068969726562 hips_overlay = mean hips_hierarchy = median hips_hierarchy = mean hips_creator = Oberto A. (CDS) hips_copyright = CNRS/Unistra hips_version = 1.4 hips_release_date = 2021-02-23T01:29Z hips_frame = equatorial hips_order = 9 hips_order_min = 0 hips_tile_width = 512 dataproduct_type = image moc_access_url = http://alasky.u-strasbg.fr/2MASS/K/Moc.fits hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_cut = -0.5 40 hips_data_range = -2661 9046 obs_title = 2MASS K (2.16um) obs_collection = The Two Micron All Sky Survey - K band (2MASS K) obs_description = 2MASS has uniformly scanned the entire sky in three near-infrared bands to detect and characterize point sources brighter than about 1 mJy in each band, with signal-to-noise ratio (SNR) greater than 10, using a pixel size of 2.0". This has achieved an 80,000-fold improvement in sensitivity relative to earlier surveys. 2MASS used two highly-automated 1.3-m telescopes, one at Mt. Hopkins, AZ, and one at CTIO, Chile. Each telescope was equipped with a three-channel camera, each channel consisting of a 256x256 array of HgCdTe detectors, capable of observing the sky simultaneously at J (1.25 microns), H (1.65 microns), and Ks (2.17 microns). The University of Massachusetts (UMass) was responsible for the overall management of the project, and for developing the infrared cameras and on-site computing systems at both facilities. The Infrared Processing and Analysis Center (IPAC) is responsible for all data processing through the Production Pipeline, and construction and distribution of the data products. Funding is provided primarily by NASA and the NSF obs_copyright_url = http://www.ipac.caltech.edu/2mass/ obs_ack = University of Massachusetts & IPAC/Caltech bib_reference = 2006AJ....131.1163S bib_reference_url = http://simbad.u-strasbg.fr/simbad/sim-ref?bibcode=2006AJ....131.1163S obs_copyright = University of Massachusetts & IPAC/Caltech t_min = 50600 t_max = 51941 obs_regime = Infrared em_min = 2.015E-6 em_max = 2.303E-6 prov_progenitor = IPAC/NASA client_category = Image/Infrared/2MASS hips_builder = Aladin/HipsGen v11.023 hips_pixel_scale = 2.236E-4 s_pixel_scale = 2.777E-4 moc_sky_fraction = 1 hips_estsize = 4706425658 hips_creation_date = 2013-01-14T09:45Z hipsgen_date = 2020-08-04T10:56Z hipsgen_params = cache=CACHE-TODEL-K cacheRemoveOnExit=true in=2MASSk out=Hips-K3 creator_did=ivo://CDS-test/P/2MASS/K "hips_pixel_cut=-0.5 40 log" maxthread=64 -f hips_frame=equatorial skyval=SKYVAL JPEG hips_service_url = https://alasky.cds.unistra.fr/2MASS/K hips_progenitor_url = https://alasky.cds.unistra.fr/2MASS/K/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/2MASS/K hips_status_1 = public mirror clonableOnce hips_service_url_2 = https://irsa.ipac.caltech.edu/data/hips/CDS/2MASS/K hips_status_2 = public mirror unclonable hips_tile_format_2 = jpeg moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 9 obs_initial_ra = 266.40499479 obs_initial_dec = -28.936173970 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288570974 ID = CDS/P/2MASS/color hips_doi = 10.26093/cds/aladin/bzc8-nw creator_did = ivo://CDS/P/2MASS/color hips_initial_fov = 58.63230142835039 hips_initial_ra = 266.40499479 hips_initial_dec = -28.936173970 obs_collection = The Two Micron All Sky Survey - J-H-K bands (2MASS color) obs_title = 2MASS color J (1.23um), H (1.66um), K (2.16um) obs_description = 2MASS has uniformly scanned the entire sky in three near-infrared bands to detect and characterize point sources brighter than about 1 mJy in each band, with signal-to-noise ratio (SNR) greater than 10, using a pixel size of 2.0". This has achieved an 80,000-fold improvement in sensitivity relative to earlier surveys. 2MASS used two highly-automated 1.3-m telescopes, one at Mt. Hopkins, AZ, and one at CTIO, Chile. Each telescope was equipped with a three-channel camera, each channel consisting of a 256x256 array of HgCdTe detectors, capable of observing the sky simultaneously at J (1.25 microns), H (1.65 microns), and Ks (2.17 microns). The University of Massachusetts (UMass) was responsible for the overall management of the project, and for developing the infrared cameras and on-site computing systems at both facilities. The Infrared Processing and Analysis Center (IPAC) is responsible for all data processing through the Production Pipeline, and construction and distribution of the data products. Funding is provided primarily by NASA and the NSF obs_copyright_url = http://www.ipac.caltech.edu/2mass/ hips_creator = Oberto A., Boch T. (CDS) client_application = AladinLite client_application = AladinDesktop client_sort_key = 04-001-00 prov_progenitor = IPAC/NASA client_category = Image/Infrared/2MASS t_min = 50600 t_max = 51941 obs_regime = Infrared em_min = 1.147E-6 em_max = 2.303E-6 hips_builder = Custom ad-hoc Python script. Following cuts have been used: --> K-band (red): -0.493522647023201, 69, sqrt stretch --> H-band (green): -0.5254, 69, sqrt stretch --> J-band (blue) -0.456, 50, sqrt stretch. Moreover, in order to reduce the green noise, green pixels with values greater than the mean between red and blue values have been replaced with the mean value. hips_version = 1.4 hips_release_date = 2024-10-09T07:12Z hips_frame = equatorial hips_order = 9 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = University of Massachusetts & IPAC/Caltech bib_reference = 2006AJ....131.1163S bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2006AJ....131.1163S obs_copyright = University of Massachusetts & IPAC/Caltech hips_pixel_scale = 2.236E-4 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 75160788 hips_creation_date = 2012-02-24T12:43Z hips_tile_format = jpeg hips_hierarchy = mean dataproduct_subtype = color hips_service_url = https://alasky.cds.unistra.fr/2MASS/Color hips_service_url_1 = https://alaskybis.cds.unistra.fr/2MASS/Color hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 9 obs_initial_ra = 266.40499479 obs_initial_dec = -28.936173970 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1728979927807 ID = CDS/P/2MASS6X/H hips_doi = 10.26093/cds/aladin/t36n-rv creator_did = ivo://CDS/P/2MASS6X/H obs_collection = 2MASS6X H obs_title = 2MASS6X H (1.66um) obs_description = During the final months of 2MASS observatory operations, a campaign of targeted "long exposure" observations was carried out during times when no previously unscanned parts of the sky were available for the main survey. These observations used the same freeze-frame scanning technique employed for the survey, but with READ2-READ1 exposures six times longer than was used for normal survey observations (hence they are referred to as "6x" observations). The 2MASS 6x measurements were intended to probe ~1 magnitude deeper than the main survey in unconfused regions. Approximately 590 deg2 of sky distributed in 30 targeted regions were scanned at least once using the long exposures. Most of this area is concentrated in two large, comprehensive surveys of the Large and Small Magellanic Clouds, 383 deg2 and 127 deg2, respectively. Twenty-eight additional smaller fields were mapped in the 6x mode from both observatories, covering targets that include the Pleiades open cluster, galactic star formation complexes, M31, nearby galaxy clusters and the Lockman Hole. obs_copyright_url = http://www.ipac.caltech.edu/2mass/releases/allsky/doc/seca3_1.html prov_progenitor = IPAC/NASA client_category = Image/Infrared/2MASS/2MASS6X client_sort_key = 04-001-99-02 hips_creation_date = 2012-04-23T07:52Z hips_release_date = 2019-05-05T04:54Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Boch T. (CDS) hips_version = 1.4 hips_order = 9 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png jpeg fits dataproduct_type = image hips_pixel_cut = -5.716 152.2 hips_data_range = -54.3 3356 moc_access_url = http://alasky.unistra.fr/2MASS6X/2MASS6X_H/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = University of Massachusetts & IPAC/Caltech bib_reference = 2006AJ....131.1163S bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2006AJ....131.1163S obs_copyright = University of Massachusetts & IPAC/Caltech t_min = 51488 t_max = 51955 obs_regime = Infrared em_min = 1.525E-6 em_max = 1.798E-6 hips_hierarchy = mean hips_pixel_scale = 2.236E-4 hips_pixel_bitpix = -32 hipsgen_date = 2017-03-28T09:34Z hipsgen_params = out=2MASS6X_H "pixelCut=-5.716 152.2" UPDATE hips_initial_fov = 6.0 hips_initial_ra = 80.4118332 hips_initial_dec = -69.6132765 hips_order_min = 0 moc_sky_fraction = 0.01316 hips_estsize = 4612474682 hipsgen_date_1 = 2019-05-05T04:54Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/2MASS6X/2MASS6X_H UPDATE hips_service_url = https://alasky.cds.unistra.fr/2MASS6X/2MASS6X_H hips_service_url_1 = https://alaskybis.cds.unistra.fr/2MASS6X/2MASS6X_H hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 9 obs_initial_ra = 80.4118332 obs_initial_dec = -69.6132765 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288413030 ID = CDS/P/2MASS6X/J hips_doi = 10.26093/cds/aladin/3d3t-dhq creator_did = ivo://CDS/P/2MASS6X/J obs_collection = 2MASS6X J obs_title = 2MASS6X J (1.23um) obs_description = During the final months of 2MASS observatory operations, a campaign of targeted "long exposure" observations was carried out during times when no previously unscanned parts of the sky were available for the main survey. These observations used the same freeze-frame scanning technique employed for the survey, but with READ2-READ1 exposures six times longer than was used for normal survey observations (hence they are referred to as "6x" observations). The 2MASS 6x measurements were intended to probe ~1 magnitude deeper than the main survey in unconfused regions. Approximately 590 deg2 of sky distributed in 30 targeted regions were scanned at least once using the long exposures. Most of this area is concentrated in two large, comprehensive surveys of the Large and Small Magellanic Clouds, 383 deg2 and 127 deg2, respectively. Twenty-eight additional smaller fields were mapped in the 6x mode from both observatories, covering targets that include the Pleiades open cluster, galactic star formation complexes, M31, nearby galaxy clusters and the Lockman Hole. obs_copyright_url = http://www.ipac.caltech.edu/2mass/releases/allsky/doc/seca3_1.html prov_progenitor = IPAC/NASA client_category = Image/Infrared/2MASS/2MASS6X client_sort_key = 04-001-99-01 hips_release_date = 2019-05-05T04:57Z hips_creator = Boch T. (CDS) hips_version = 1.4 hips_order = 9 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = jpeg fits dataproduct_type = image hips_pixel_cut = -1.335 40.18 hips_data_range = -2.00 4285 moc_access_url = http://alasky.unistra.fr/2MASS6X/2MASS6X_J/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = University of Massachusetts & IPAC/Caltech bib_reference = 2006AJ....131.1163S bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2006AJ....131.1163S obs_copyright = University of Massachusetts & IPAC/Caltech t_min = 51488 t_max = 51955 obs_regime = Infrared em_min = 1.147E-6 em_max = 1.323E-6 hips_builder = Aladin/HipsGen v10.123 hips_creation_date = 2012-04-17T08:31Z hips_hierarchy = mean hips_pixel_scale = 2.236E-4 hips_pixel_bitpix = -32 hipsgen_date = 2017-03-28T09:41Z hipsgen_params = out=2MASS6X_J "pixelCut=-1.335 40.18" UPDATE hips_initial_fov = 6.0 hips_initial_ra = 80.4118332 hips_initial_dec = -69.6132765 hips_order_min = 0 moc_sky_fraction = 0.01316 hips_estsize = 4556104097 hipsgen_date_1 = 2019-05-05T04:57Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/2MASS6X/2MASS6X_J UPDATE hips_service_url = https://alasky.cds.unistra.fr/2MASS6X/2MASS6X_J hips_service_url_1 = https://alaskybis.cds.unistra.fr/2MASS6X/2MASS6X_J hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 9 obs_initial_ra = 80.4118332 obs_initial_dec = -69.6132765 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288413098 ID = CDS/P/2MASS6X/K hips_doi = 10.26093/cds/aladin/2pkm-1n1 creator_did = ivo://CDS/P/2MASS6X/K obs_collection = 2MASS6X K obs_title = 2MASS6X K (2.16um) obs_description = During the final months of 2MASS observatory operations, a campaign of targeted "long exposure" observations was carried out during times when no previously unscanned parts of the sky were available for the main survey. These observations used the same freeze-frame scanning technique employed for the survey, but with READ2-READ1 exposures six times longer than was used for normal survey observations (hence they are referred to as "6x" observations). The 2MASS 6x measurements were intended to probe ~1 magnitude deeper than the main survey in unconfused regions. Approximately 590 deg2 of sky distributed in 30 targeted regions were scanned at least once using the long exposures. Most of this area is concentrated in two large, comprehensive surveys of the Large and Small Magellanic Clouds, 383 deg2 and 127 deg2, respectively. Twenty-eight additional smaller fields were mapped in the 6x mode from both observatories, covering targets that include the Pleiades open cluster, galactic star formation complexes, M31, nearby galaxy clusters and the Lockman Hole. obs_copyright_url = http://www.ipac.caltech.edu/2mass/releases/allsky/doc/seca3_1.html prov_progenitor = IPAC/NASA client_category = Image/Infrared/2MASS/2MASS6X client_sort_key = 04-001-99-03 hips_release_date = 2019-05-05T04:58Z hips_creator = CDS hips_version = 1.4 hips_order = 9 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = jpeg fits dataproduct_type = image hips_pixel_cut = -9.683 70.12 hips_data_range = -4 6821 moc_access_url = http://alasky.unistra.fr/2MASS6X/2MASS6X_K/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = University of Massachusetts & IPAC/Caltech bib_reference = 2006AJ....131.1163S bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2006AJ....131.1163S obs_copyright = University of Massachusetts & IPAC/Caltech t_min = 51488 t_max = 51955 obs_regime = Infrared em_min = 2.015E-6 em_max = 2.303E-6 hips_builder = Aladin/HipsGen v10.123 hips_creation_date = 2012-04-23T15:03Z hips_hierarchy = mean hips_pixel_scale = 2.236E-4 hips_pixel_bitpix = -32 hipsgen_date = 2017-03-28T09:43Z hipsgen_params = out=2MASS6X_K "pixelCut=-9.683 70.12" UPDATE hips_order_min = 0 hips_initial_fov = 6.0 hips_initial_ra = 80.4118332 hips_initial_dec = -69.6132765 moc_sky_fraction = 0.01316 hips_estsize = 4556104097 hipsgen_date_1 = 2019-05-05T04:58Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/2MASS6X/2MASS6X_K UPDATE hips_service_url = https://alasky.cds.unistra.fr/2MASS6X/2MASS6X_K hips_service_url_1 = https://alaskybis.cds.unistra.fr/2MASS6X/2MASS6X_K hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 9 obs_initial_ra = 80.4118332 obs_initial_dec = -69.6132765 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288413158 ID = CDS/P/2MASS6X/color hips_doi = 10.26093/cds/aladin/398e-2je creator_did = ivo://CDS/P/2MASS6X/color obs_title = 2MASS6X color J (1.23um) & K (2.16um) obs_description = During the final months of 2MASS observatory operations, a campaign of targeted "long exposure" observations was carried out during times when no previously unscanned parts of the sky were available for the main survey. These observations used the same freeze-frame scanning technique employed for the survey, but with READ2-READ1 exposures six times longer than was used for normal survey observations (hence they are referred to as "6x" observations). The 2MASS 6x measurements were intended to probe ~1 magnitude deeper than the main survey in unconfused regions. Approximately 590 deg2 of sky distributed in 30 targeted regions were scanned at least once using the long exposures. Most of this area is concentrated in two large, comprehensive surveys of the Large and Small Magellanic Clouds, 383 deg2 and 127 deg2, respectively. Twenty-eight additional smaller fields were mapped in the 6x mode from both observatories, covering targets that include the Pleiades open cluster, galactic star formation complexes, M31, nearby galaxy clusters and the Lockman Hole. obs_provenance = Colored HiPS built by CDS hips_creator = Fernique P. (CDS) obs_copyright_url = http://www.ipac.caltech.edu/2mass/releases/allsky/doc/seca3_1.html prov_progenitor = IPAC/NASA client_category = Image/Infrared/2MASS/2MASS6X client_sort_key = 04-001-99-00 obs_collection = 2MASS6X color obs_ack = University of Massachusetts & IPAC/Caltech - colored composition by CDS bib_reference = 2006AJ....131.1163S bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2006AJ....131.1163S obs_copyright = University of Massachusetts & IPAC/Caltech t_min = 51488 t_max = 51955 obs_regime = Infrared em_min = 1.147E-6 em_max = 2.303E-6 hips_builder = Aladin/HipsGen v10.123 hips_version = 1.4 hips_release_date = 2019-05-05T04:46Z hips_frame = equatorial hips_order = 9 hips_tile_width = 512 hips_status = public master clonableOnce hips_pixel_scale = 2.236E-4 dataproduct_type = image hips_rgb_red = 2MASS6X J [-1.335 19.4225 40.18 Linear] hips_rgb_blue = 2MASS6X K [-9.683 30.2185 70.12 Linear] hips_estsize = 56370593 hips_creation_date = 2017-03-28T09:49Z hips_hierarchy = median hips_tile_format = png hipsgen_date = 2017-03-28T12:31Z hipsgen_params = out=2MASS6X_color id=CDS/P/2MASS6X/color UPDATE hips_initial_fov = 6.0 hips_initial_ra = 80.4118332 hips_initial_dec = -69.6132765 hips_order_min = 0 dataproduct_subtype = color moc_sky_fraction = 0.01316 hipsgen_date_1 = 2019-05-05T04:46Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/2MASS6X/2MASS6X_color UPDATE hips_service_url = https://alasky.cds.unistra.fr/2MASS6X/2MASS6X_color hips_service_url_1 = https://alaskybis.cds.unistra.fr/2MASS6X/2MASS6X_color hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 9 obs_initial_ra = 80.4118332 obs_initial_dec = -69.6132765 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288412962 ID = CDS/P/ACT2/DR4/CMB hips_doi = 10.26093/cds/aladin/8txd-c4 hips_initial_fov = 102.08333 hips_initial_ra = 196.43333 hips_initial_dec = +8.55417 creator_did = ivo://CDS/P/ACT2/DR4/CMB hips_pixel_bitpix = -64 data_pixel_bitpix = -64 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = median hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra obs_title = ACT2 DR4 CMB obs_collection = ACT2 DR4 CMB obs_description = The Atacama Cosmology Telescope (ACT) is a six-meter diameter telescope on Cerro Toco in the Atacama Desert of northern Chile (image above by Jon Ward). It is designed to make high-resolution measurements of the cosmic microwave background (CMB) temperature and polarization anisotropies and detect massive galaxy clusters via the thermal Sunyaev Zel'dovich (tSZ) effect. Reconstruction of the CMB lensing potential will play a key role in the cosmological detection of neutrino mass, and measuring the imprint of primordial gravitational waves in B-mode polarization could provide unique insights into the early universe and quantum nature of gravity. The majority of the DR4 products use data collected from 2013-16. DR4 also includes data collected from 2008-10. The second-generation, polarization-sensitive receiver ACTPol observed between 2013 and 2016. The four-year survey consists of 17,000 square degrees of the sky mapped at 98 and 150 GHz, with the deepest 600 square degrees at a noise < 10 uK-arcmin. prov_progenitor = https://lambda.gsfc.nasa.gov/product/act/actpol_prod_table.cfm bib_reference = 2020PhRvD.102b3534M bib_reference_url = https://ui.adsabs.harvard.edu/abs/2020PhRvD.102b3534M/abstract obs_copyright = LAMBDA HEASARC obs_copyright_url = https://lambda.gsfc.nasa.gov/ t_min = 54466.6 t_max = 57386.2 obs_regime = Radio client_category = Image/Radio/ACT em_min = 0.00199861 em_max = 0.00305910 hips_builder = Aladin/HipsGen v11.037 hips_version = 1.4 hips_release_date = 2021-04-12T09:58Z hips_frame = equatorial hips_order = 4 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = -327.4 361.3 hips_data_range = -1135 1066 hips_pixel_scale = 0.007157 s_pixel_scale = 0.008333 dataproduct_type = image moc_sky_fraction = 0.0952 hips_estsize = 1040298 hipsgen_date = 2021-04-12T09:58Z hipsgen_params = in=/data-local-zfs/buga/ACT/images_component_separated_maps/images/images/tilec_single_tile_REGION_cmb_map_v1_2_0_joint_fits/ out=HipS_CMB/ creator_did=CDS/P/ACT2/DR4/CMB verbose=4 BLANK=0 hips_creation_date = 2021-04-12T09:58Z hips_service_url = https://alasky.cds.unistra.fr/ACT/DR4/CDS_P_ACT2_DR4_CMB hips_progenitor_url = https://alasky.cds.unistra.fr/ACT/DR4/CDS_P_ACT2_DR4_CMB/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/ACT/DR4/CDS_P_ACT2_DR4_CMB hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 7 obs_initial_ra = 196.43333 obs_initial_dec = +8.55417 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288489438 ID = CDS/P/AKARI/FIS/Color hips_doi = 10.26093/cds/aladin/3rag-15t creator_did = ivo://CDS/P/AKARI/FIS/Color obs_collection = AKARI FIS Color obs_title = AKARI FIS Color WideL (140um), WideS (90um), N60 (65um) obs_description = AKARI (Previously known as ASTRO-F or IRIS - InfraRed Imaging Surveyor) is the second space mission for infrared astronomy in Japan. AKARI was developed by the members of JAXA/ISAS and collaborators. IRAS (Infrared Astronomical Satellite, launched in 1983 by the United Kingdom, the United States, and the Netherlands) carried out the first all-sky survey at infrared wavelengths and made a huge impact on astronomy. The AKARI mission was an ambitious plan to make an all-sky survey with much better sensitivity, spatial resolution and wider wavelength coverage than those of IRAS. All-sky survey obtained by the Far-Infrared Surveyor (FIS) onboard the AKARI satellite, at 65um (Color), 90 um (WIDE-S), 140um (WIDE-L),and 160um (N160). See http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/Doi_AKARI_FIR_AllSkySurvey.pdf. obs_ack = University of Tokyo, ISAS/JAXA, Tohoku University, University of Tsukuba, RAL, and Open University obs_copyright = ISAS/JAXA obs_copyright_url = http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/ client_application = AladinLite client_application = AladinLite client_application = AladinDesktop client_category = Image/Infrared/AKARI-FIS client_sort_key = 04-05-00 hips_release_date = 2019-05-05T04:59Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Fernique P. (CDS) hips_version = 1.4 hips_order = 5 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png jpeg dataproduct_type = image hips_rgb_red = WideLHiPS [0.0 250.0 500.0 Log] hips_rgb_green = WideSHiPS [-1.5 91.75 185.0 Log] hips_rgb_blue = N60HiPS [-1.5 69.25 140.0 Log] moc_access_url = http://alasky.u-strasbg.fr/AKARI-FIS/ColorLSN60/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = ISAS/JAXA bib_reference = 2015PASJ...67...50D bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2015PASJ...67...50D t_min = 53863 t_max = 54338 obs_regime = Infrared em_min = 6.5E-5 em_max = 0.00014 hips_creation_date = 2015-01-09T14:17Z hips_hierarchy = mean hips_pixel_scale = 0.003579 hips_initial_fov = 110.0 hips_initial_ra = 83.5553478 hips_initial_dec = 9.0998893 hips_order_min = 0 dataproduct_subtype = color moc_sky_fraction = 1 hips_estsize = 367003 hipsgen_date = 2019-05-05T04:59Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/AKARI-FIS/ColorLSN60 UPDATE hips_service_url = https://alasky.cds.unistra.fr/AKARI-FIS/ColorLSN60 hips_service_url_1 = https://alaskybis.cds.unistra.fr/AKARI-FIS/ColorLSN60 hips_status_1 = public mirror clonableOnce hips_service_url_2 = https://healpix.ias.u-psud.fr/CDS_P_AKARI_FIS_Color hips_status_2 = public mirror unclonable moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 5 obs_initial_ra = 83.5553478 obs_initial_dec = 9.0998893 obs_initial_fov = 1.8322594196359496 TIMESTAMP = 1729584609321 ID = CDS/P/AKARI/FIS/N160 hips_doi = 10.26093/cds/aladin/23kb-b0r creator_did = ivo://CDS/P/AKARI/FIS/N160 obs_collection = AKARI FIS N160 obs_title = AKARI FIS N160 (160um) obs_description = AKARI (Previously known as ASTRO-F or IRIS - InfraRed Imaging Surveyor) is the second space mission for infrared astronomy in Japan. AKARI was developed by the members of JAXA/ISAS and collaborators. IRAS (Infrared Astronomical Satellite, launched in 1983 by the United Kingdom, the United States, and the Netherlands) carried out the first all-sky survey at infrared wavelengths and made a huge impact on astronomy. The AKARI mission was an ambitious plan to make an all-sky survey with much better sensitivity, spatial resolution and wider wavelength coverage than those of IRAS. All-sky survey obtained by the Far-Infrared Surveyor (FIS) onboard the AKARI satellite, at 65um (Color), 90 um (WIDE-S), 140um (WIDE-L),and 160um (N160). See http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/Doi_AKARI_FIR_AllSkySurvey.pdf. obs_ack = University of Tokyo, ISAS/JAXA, Tohoku University, University of Tsukuba, RAL and Open University obs_copyright = ISAS/JAXA obs_copyright_url = http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/ client_category = Image/Infrared/AKARI-FIS client_sort_key = 04-05-04 hips_release_date = 2019-05-05T05:01Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Fernique P. (CDS) hips_version = 1.4 hips_order = 5 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png fits dataproduct_type = image hips_pixel_cut = 0 500 hips_data_range = -125.7 304.6 moc_access_url = http://alasky.u-strasbg.fr/AKARI-FIS/N160/Moc.fits hips_progenitor_url = https://alasky.cds.unistra.fr/AKARI-FIS/N160/HpxFinder hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = ISAS/JAXA bib_reference = 2015PASJ...67...50D bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2015PASJ...67...50D t_min = 53863 t_max = 54338 obs_regime = Infrared em_min = 0.00016 em_max = 0.00016 hips_creation_date = 2015-01-08T14:34Z hips_hierarchy = mean hips_pixel_scale = 0.003579 hips_initial_fov = 110.0 hips_initial_ra = 83.5553478 hips_initial_dec = 9.0998893 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 17870688 hipsgen_date = 2019-05-05T05:01Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/AKARI-FIS/N160 UPDATE hips_service_url = https://alasky.cds.unistra.fr/AKARI-FIS/N160 hips_service_url_1 = https://alaskybis.cds.unistra.fr/AKARI-FIS/N160 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 41 moc_time_range = 1 moc_order = 5 obs_initial_ra = 83.5553478 obs_initial_dec = 9.0998893 obs_initial_fov = 1.8322594196359496 TIMESTAMP = 1721288413290 ID = CDS/P/AKARI/FIS/N60 hips_doi = 10.26093/cds/aladin/2a4f-2bn creator_did = ivo://CDS/P/AKARI/FIS/N60 obs_collection = AKARI FIS N60 obs_title = AKARI FIS N60 (65um) obs_description = AKARI (Previously known as ASTRO-F or IRIS - InfraRed Imaging Surveyor) is the second space mission for infrared astronomy in Japan. AKARI was developed by the members of JAXA/ISAS and collaborators. IRAS (Infrared Astronomical Satellite, launched in 1983 by the United Kingdom, the United States, and the Netherlands) carried out the first all-sky survey at infrared wavelengths and made a huge impact on astronomy. The AKARI mission was an ambitious plan to make an all-sky survey with much better sensitivity, spatial resolution and wider wavelength coverage than those of IRAS. All-sky survey obtained by the Far-Infrared Surveyor (FIS) onboard the AKARI satellite, at 65um (Color), 90 um (WIDE-S), 140um (WIDE-L),and 160um (N160). See http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/Doi_AKARI_FIR_AllSkySurvey.pdf. obs_ack = University of Tokyo, ISAS/JAXA, Tohoku University, University of Tsukuba, RAL and Open University obs_copyright = ISAS/JAXA obs_copyright_url = http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/ client_category = Image/Infrared/AKARI-FIS client_sort_key = 04-05-01 hips_release_date = 2019-05-05T05:03Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Fernique P. (CDS) hips_version = 1.4 hips_order = 5 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png fits dataproduct_type = image hips_pixel_cut = -1.5 140 hips_data_range = -104.6 251 moc_access_url = http://alasky.u-strasbg.fr/AKARI-FIS/N60/Moc.fits hips_progenitor_url = https://alasky.cds.unistra.fr/AKARI-FIS/N60/HpxFinder hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = ISAS/JAXA bib_reference = 2015PASJ...67...50D bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2015PASJ...67...50D t_min = 53863 t_max = 54338 obs_regime = Infrared em_min = 6.5E-5 em_max = 6.5E-5 hips_creation_date = 2015-01-08T16:04Z hips_hierarchy = mean hips_pixel_scale = 0.003579 hips_initial_fov = 110.0 hips_initial_ra = 83.5553478 hips_initial_dec = 9.0998893 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 17870688 hipsgen_date = 2019-05-05T05:03Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/AKARI-FIS/N60 UPDATE hips_service_url = https://alasky.cds.unistra.fr/AKARI-FIS/N60 hips_service_url_1 = https://alaskybis.cds.unistra.fr/AKARI-FIS/N60 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 41 moc_time_range = 1 moc_order = 5 obs_initial_ra = 83.5553478 obs_initial_dec = 9.0998893 obs_initial_fov = 1.8322594196359496 TIMESTAMP = 1721288413358 ID = CDS/P/AKARI/FIS/WideL hips_doi = 10.26093/cds/aladin/1tkx-knx creator_did = ivo://CDS/P/AKARI/FIS/WideL obs_collection = AKARI FIS WideL obs_title = AKARI FIS WideL (140um) obs_description = AKARI (Previously known as ASTRO-F or IRIS - InfraRed Imaging Surveyor) is the second space mission for infrared astronomy in Japan. AKARI was developed by the members of JAXA/ISAS and collaborators. IRAS (Infrared Astronomical Satellite, launched in 1983 by the United Kingdom, the United States, and the Netherlands) carried out the first all-sky survey at infrared wavelengths and made a huge impact on astronomy. The AKARI mission was an ambitious plan to make an all-sky survey with much better sensitivity, spatial resolution and wider wavelength coverage than those of IRAS. All-sky survey obtained by the Far-Infrared Surveyor (FIS) onboard the AKARI satellite, at 65um (Color), 90 um (WIDE-S), 140um (WIDE-L),and 160um (N160). See http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/Doi_AKARI_FIR_AllSkySurvey.pdf. obs_ack = University of Tokyo, ISAS/JAXA, Tohoku University, University of Tsukuba, RAL and Open University obs_copyright = ISAS/JAXA obs_copyright_url = http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/ client_category = Image/Infrared/AKARI-FIS client_sort_key = 04-05-03 hips_release_date = 2019-05-05T05:05Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Fernique P. (CDS) hips_version = 1.4 hips_order = 5 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png fits dataproduct_type = image hips_pixel_cut = 0 500 hips_data_range = -38.17 154 moc_access_url = http://alasky.u-strasbg.fr/AKARI-FIS/WideL/Moc.fits hips_progenitor_url = https://alasky.cds.unistra.fr/AKARI-FIS/WideL/HpxFinder hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = ISAS/JAXA bib_reference = 2015PASJ...67...50D bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2015PASJ...67...50D t_min = 53863 t_max = 54338 obs_regime = Infrared em_min = 0.00014 em_max = 0.00014 hips_creation_date = 2015-01-08T15:53Z hips_hierarchy = mean hips_pixel_scale = 0.003579 hips_initial_fov = 110.0 hips_initial_ra = 83.5553478 hips_initial_dec = 9.0998893 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 17870688 hipsgen_date = 2019-05-05T05:05Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/AKARI-FIS/WideL UPDATE hips_service_url = https://alasky.cds.unistra.fr/AKARI-FIS/WideL hips_service_url_1 = https://alaskybis.cds.unistra.fr/AKARI-FIS/WideL hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 41 moc_time_range = 1 moc_order = 5 obs_initial_ra = 83.5553478 obs_initial_dec = 9.0998893 obs_initial_fov = 1.8322594196359496 TIMESTAMP = 1721288413410 ID = CDS/P/AKARI/FIS/WideS hips_doi = 10.26093/cds/aladin/3w3d-gt8 creator_did = ivo://CDS/P/AKARI/FIS/WideS obs_collection = AKARI FIS WideS obs_title = AKARI FIS WideS (90um) obs_description = AKARI (Previously known as ASTRO-F or IRIS - InfraRed Imaging Surveyor) is the second space mission for infrared astronomy in Japan. AKARI was developed by the members of JAXA/ISAS and collaborators. IRAS (Infrared Astronomical Satellite, launched in 1983 by the United Kingdom, the United States, and the Netherlands) carried out the first all-sky survey at infrared wavelengths and made a huge impact on astronomy. The AKARI mission was an ambitious plan to make an all-sky survey with much better sensitivity, spatial resolution and wider wavelength coverage than those of IRAS. All-sky survey obtained by the Far-Infrared Surveyor (FIS) onboard the AKARI satellite, at 65um (Color), 90 um (WIDE-S), 140um (WIDE-L),and 160um (N160). See http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/Doi_AKARI_FIR_AllSkySurvey.pdf. obs_ack = University of Tokyo, ISAS/JAXA, Tohoku University, University of Tsukuba, RAL and Open University obs_copyright = ISAS/JAXA obs_copyright_url = http://www.ir.isas.jaxa.jp/AKARI/Archive/Images/FIS_AllSkyMap/ client_category = Image/Infrared/AKARI-FIS client_sort_key = 04-05-02 hips_release_date = 2019-05-05T05:07Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Fernique P. (CDS) hips_version = 1.4 hips_order = 5 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png fits dataproduct_type = image hips_pixel_cut = -1.5 140 hips_data_range = -12.06 38.42 moc_access_url = http://alasky.u-strasbg.fr/AKARI-FIS/WideS/Moc.fits hips_progenitor_url = https://alasky.cds.unistra.fr/AKARI-FIS/WideS/HpxFinder hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = ISAS/JAXA bib_reference = 2015PASJ...67...50D bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2015PASJ...67...50D t_min = 53863 t_max = 54338 obs_regime = Infrared em_min = 9e-5 em_max = 9e-5 hips_creation_date = 2015-01-08T15:45Z hips_hierarchy = mean hips_pixel_scale = 0.003579 hips_initial_fov = 110.0 hips_initial_ra = 83.5553478 hips_initial_dec = 9.0998893 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 17870688 hipsgen_date = 2019-05-05T05:07Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/AKARI-FIS/WideS UPDATE hips_service_url = https://alasky.cds.unistra.fr/AKARI-FIS/WideS hips_service_url_1 = https://alaskybis.cds.unistra.fr/AKARI-FIS/WideS hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 41 moc_time_range = 1 moc_order = 5 obs_initial_ra = 83.5553478 obs_initial_dec = 9.0998893 obs_initial_fov = 1.8322594196359496 TIMESTAMP = 1721288413462 ID = CDS/P/AST3II/DR1 hips_doi = 10.26093/cds/aladin/a99m-82 creator_did = ivo://CDS/P/AST3II/DR1 hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra obs_title = AST3II DR1 obs_collection = AST3II DR1 obs_description = In the austral winters of 2016 and 2017, we used the AST3-II telescope located at the Chinese Kunlun station at Dome A, Antarctica to survey a group of selected fields near the southern ecliptic pole and within the southern continuous viewing zone (CVZ) of Transiting Exoplanet Survey Satellite (TESS; Ricker+ 2009AAS...21430605R). This first data release contains a data set obtained in the austral winter of 2016. obs_ack = Hui Zhang [Nanjing University, China] prov_progenitor = https://cdsarc.cds.unistra.fr/ftp/J/ApJS/240/16/ bib_reference = 2019ApJS..240...16Z bib_reference_url = https://iopscience.iop.org/article/10.3847/1538-4365/aaec0c t_min = 57723 t_max = 58088 obs_regime = Optical em_min = 6.689e-7 em_max = 8.389e-7 client_category = Image/Optical/AST3II hips_builder = Aladin/HipsGen v12.114 hips_version = 1.4 hips_frame = equatorial hips_order = 9 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 103.645455 hips_initial_dec = -71.4490899 hips_initial_fov = 15.0 hips_pixel_scale = 2.236E-4 s_pixel_scale = 2.777E-4 dataproduct_type = image hipsgen_date = 2023-12-22T14:53Z hipsgen_params = in=../../img out=AST3II_blank0/ id=CDS/P/AST3II/DR1 blank=0 "pixelCut=190 450 sqrt" hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwriteTile treeMean hips_release_date = 2023-12-22T14:54Z hips_tile_format = png fits hips_pixel_cut = 190 450 hips_data_range = -7532 23401 moc_sky_fraction = 0.001175 hips_creation_date = 2023-12-22T14:53Z hips_estsize = 6047840 hips_nb_tiles = 10154 hips_check_code = png:3216933585 fits:3501681365 hips_service_url = https://alasky.cds.unistra.fr/AST3II/CDS_P_AST3II_DR1 hips_progenitor_url = https://alasky.cds.unistra.fr/AST3II/CDS_P_AST3II_DR1/HpxFinder moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 9 obs_initial_ra = 103.645455 obs_initial_dec = -71.4490899 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1712902098028 ID = CDS/P/AST3II/DR1/deep hips_doi = 10.26093/cds/aladin/3zh0-kc creator_did = ivo://CDS/P/AST3II/DR1/deep hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra obs_title = AST3II DR1 deep obs_collection = AST3II DR1 deep obs_description = In the austral winters of 2016 and 2017, we used the AST3-II telescope located at the Chinese Kunlun station at Dome A, Antarctica to survey a group of selected fields near the southern ecliptic pole and within the southern continuous viewing zone (CVZ) of Transiting Exoplanet Survey Satellite (TESS; Ricker+ 2009AAS...21430605R). This first data release contains a data set obtained in the austral winter of 2016. obs_ack = Hui Zhang [Nanjing University, China] prov_progenitor = https://cdsarc.cds.unistra.fr/ftp/J/ApJS/240/16/ bib_reference = 2019ApJS..240...16Z bib_reference_url = https://iopscience.iop.org/article/10.3847/1538-4365/aaec0c t_min = 57723 t_max = 58088 obs_regime = Optical em_min = 6.689e-7 em_max = 8.389e-7 client_category = Image/Optical/AST3II hips_builder = Aladin/HipsGen v12.114 hips_version = 1.4 hips_frame = equatorial hips_order = 9 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 103.645455 hips_initial_dec = -71.4490899 hips_initial_fov = 15.0 hips_pixel_scale = 2.236E-4 s_pixel_scale = 2.777E-4 dataproduct_type = image hipsgen_date = 2024-01-02T09:26Z hipsgen_params = in=../../img_deep/ out=AST3II_deep/ id=CDS/P/AST3II/DR1/deep blank=0 "pixelCut=190 450 sqrt" hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwriteTile treeMean hips_release_date = 2024-01-02T09:34Z hips_tile_format = png fits hips_pixel_cut = 190 450 hips_data_range = -16509 50320 moc_sky_fraction = 0.001205 hips_creation_date = 2024-01-02T09:27Z hips_estsize = 6044043 hips_nb_tiles = 10364 hips_check_code = png:935849855 fits:1435826110 hips_service_url = https://alasky.cds.unistra.fr/AST3II/CDS_P_AST3II_DR1_deep hips_progenitor_url = https://alasky.cds.unistra.fr/AST3II/CDS_P_AST3II_DR1_deep/HpxFinder moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 9 obs_initial_ra = 103.645455 obs_initial_dec = -71.4490899 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1712902098100 ID = CDS/P/ATLASGAL hips_doi = 10.26093/cds/aladin/z4q5-68 creator_did = ivo://CDS/P/ATLASGAL obs_collection = ATLASGAL obs_title = ATLASGAL 850 um obs_description = ATLASGAL is the APEX Telescope Large Area Survey of the Galaxy, an observing programme with the LABOCA bolometer array at APEX, located at 5100 m altitude on Chajnantor, Chile. This survey mapped over 400 square degrees at 870 microns in the inner Galaxy, with a uniform sensitivity of a few solar masses at 1 kpc distance. This project is a collaboration between the Max Planck Gesellschaft (MPG: Max Planck Institute fur Radioastronomie, MPIfR Bonn, and Max Planck Institute fur Astronomie, MPIA Heidelberg), the European Southern Observatory (ESO) and the Universidad de Chile. The APEX telescope is ideally located to observe the inner Milky Way. The Large APEX Bolometer Camera (LABOCA) is a 295-element bolometer array observing at 870 um, with a beam size of 19.2 arcsec. Taking advantage of its large field of view (11.4 arcmin) and excellent sensitivity, we started an unbiased survey of the entire Galactic Plane accessible to APEX, with a typical noise level of 50-70 mJy/beam: the APEX Telescope Large Area Survey of the Galaxy (ATLASGAL). hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = median hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra obs_ack = This research has made use of the services of the ESO Science Archive Facility prov_progenitor = ESO archive bib_reference = 2009A&A...504..415S bib_reference_url = http://adsabs.harvard.edu/cgi-bin/nph-bib_query?db_key=AST&bibcode=2009A&A...504..415S obs_copyright = ESO obs_copyright_url = http://archive.eso.org/cms/eso-data-access-policy.html t_min = 54101 t_max = 55197 obs_regime = Infrared em_min = 0.00085 em_max = 0.00085 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T06:41Z hips_frame = equatorial hips_order = 7 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = -0.2481 0.3796 hips_data_range = -1.583 2.641 hips_initial_ra = 293.59154 hips_initial_dec = +19.9723 hips_initial_fov = 3.2 hips_pixel_scale = 8.946E-4 s_pixel_scale = 0.001667 dataproduct_type = image moc_sky_fraction = 0.01097 hips_estsize = 3793968 hipsgen_date = 2017-02-20T14:24Z hipsgen_params = in=SCIENCE_IMAGE_FLUXMAP out=HIPS_apex ivorn=ivo://CDS/P/APEX "Publisher=M.Buga [CDS]" INDEX TILES PNG DETAILS client_application = AladinDesktop client_category = Image/Infrared/APEX hips_creation_date = 2017-02-20T14:24Z hipsgen_date_1 = 2017-02-20T14:25Z hipsgen_params_1 = in=SCIENCE_IMAGE_FLUXMAP out=HIPS_apex ivorn=ivo://CDS/P/APEX "Publisher=M.Buga [CDS]" INDEX TILES PNG DETAILS hips_order_min = 0 hipsgen_date_2 = 2019-05-21T06:41Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/APEX/ATLASGAL UPDATE hips_service_url = https://alasky.cds.unistra.fr/APEX/ATLASGAL hips_progenitor_url = https://alasky.cds.unistra.fr/APEX/ATLASGAL/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/APEX/ATLASGAL hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 12 obs_initial_ra = 293.59154 obs_initial_dec = +19.9723 obs_initial_fov = 0.014314526715905856 TIMESTAMP = 1721288465242 ID = CDS/P/ATLASGAL/APEXPlanck hips_doi = 10.26093/cds/aladin/b0qm-9w creator_did = ivo://CDS/P/ATLASGAL/APEXPlanck obs_collection = ATLASGAL obs_title = ATLASGAL APEX-Planck 850um obs_description = ATLASGAL is the APEX Telescope Large Area Survey of the Galaxy, an observing programme with the LABOCA bolometer array at APEX, located at 5100 m altitude on Chajnantor, Chile. This survey mapped over 400 square degrees at 870 microns in the inner Galaxy, with a uniform sensitivity of a few solar masses at 1 kpc distance. This project is a collaboration between the Max Planck Gesellschaft (MPG: Max Planck Institute fur Radioastronomie, MPIfR Bonn, and Max Planck Institute fur Astronomie, MPIA Heidelberg), the European Southern Observatory (ESO) and the Universidad de Chile. The APEX telescope is ideally located to observe the inner Milky Way. The Large APEX Bolometer Camera (LABOCA) is a 295-element bolometer array observing at 870 um, with a beam size of 19.2 arcsec. Taking advantage of its large field of view (11.4 arcmin) and excellent sensitivity, we started an unbiased survey of the entire Galactic Plane accessible to APEX, with a typical noise level of 50-70 mJy/beam: the APEX Telescope Large Area Survey of the Galaxy (ATLASGAL). The LABOCA data have been combined with the results of the Planck satellite. The method used to combine the Planck and ATLASGAL data together is described in Csengeri et al. (2016). hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = median hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra obs_ack = This research has made use of the services of the ESO Science Archive Facility prov_progenitor = ESO archive bib_reference = 2016A&A...585A.104C bib_reference_url = http://cdsads.u-strasbg.fr/abs/2016A&A...585A.104C obs_copyright = ESO obs_copyright_url = http://archive.eso.org/cms/eso-data-access-policy.html t_min = 54101 t_max = 55197 obs_regime = Infrared em_min = 0.00085 em_max = 0.00085 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T06:42Z hips_frame = equatorial hips_order = 7 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = 0.1005 2.414 hips_data_range = -4.194 12.55 hips_initial_ra = 155.40769 hips_initial_dec = -57.75705 hips_initial_fov = 2.86529 hips_pixel_scale = 8.946E-4 s_pixel_scale = 9.382E-4 dataproduct_type = image moc_sky_fraction = 0.007962 hips_estsize = 3406769 hipsgen_date = 2017-02-20T16:03Z hipsgen_params = in=ANCILLARY_IMAGE out=HIPS_apex2 "Publisher=M.Buga [CDS]" ID=CDS/C/apex2 INDEX TILES PNG DETAILS client_application = AladinDesktop client_category = Image/Infrared/APEX hips_creation_date = 2017-02-20T16:03Z hipsgen_date_1 = 2017-02-20T16:04Z hipsgen_params_1 = in=ANCILLARY_IMAGE out=HIPS_apex2 "Publisher=M.Buga [CDS]" ID=CDS/C/apex2 INDEX TILES PNG DETAILS hips_order_min = 0 hipsgen_date_2 = 2019-05-21T06:42Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/APEX/ATLASGAL_APEXPlanck UPDATE hips_service_url = https://alasky.cds.unistra.fr/APEX/ATLASGAL_APEXPlanck hips_progenitor_url = https://alasky.cds.unistra.fr/APEX/ATLASGAL_APEXPlanck/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/APEX/ATLASGAL_APEXPlanck hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 12 obs_initial_ra = 155.40769 obs_initial_dec = -57.75705 obs_initial_fov = 0.014314526715905856 TIMESTAMP = 1721288465294 ID = CDS/P/Ariel/Voyager client_category = Solar system/Uranus/Ariel hips_initial_fov = 270 hips_initial_ra = 0 hips_initial_dec = +0 prov_progenitor = Caltech/JPL/NASA prov_progenitor_url = https://maps.jpl.nasa.gov/uranus.html obs_ack = From the USGS (Much thanks to Tammy Becker at the USGS.) hips_creator = Fernique P. (CDS) hips_frame = ariel hips_body = ariel creator_did = ivo://CDS/P/Ariel/Voyager obs_title = Ariel Voyager obs_description = Ariel Uranus satellite map mosaicked with Voyager imagery by USGS hips_overlay = mean hips_hierarchy = median hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T07:19Z hips_order = 3 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg hips_pixel_scale = 0.01431 s_pixel_scale = 0.25 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 18357 hipsgen_date = 2018-01-31T06:30Z hipsgen_params = "-hhh=Ariel/Ariel.jpg 1440x720" in=Ariel creator_did=CDS/P/Ariel/Voyager -f partitioning=false maxthread=10 color=jpg INDEX TILES hips_creation_date = 2018-01-31T06:30Z hips_order_min = 0 dataproduct_subtype = color hipsgen_date_1 = 2019-05-21T07:19Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume6/Planets/CDS_P_Ariel_Voyager UPDATE hips_service_url = https://alasky.cds.unistra.fr/Planets/CDS_P_Ariel_Voyager hips_service_url_1 = https://alaskybis.cds.unistra.fr/Planets/CDS_P_Ariel_Voyager hips_status_1 = public mirror clonableOnce client_application = AladinDesktopBeta>=10.040 AladinDesktop>=11.125 moc_type = smoc moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288468522 ID = CDS/P/CFHTLS/D/color/ugi hips_doi = 10.26093/cds/aladin/2cgj-vmf creator_did = ivo://CDS/P/CFHTLS/D/color/ugi obs_collection = CFHTLS D color ugi obs_title = CFHTLS-D-color-ugi obs_description = The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The Deep survey concerns 4 patchsof 1 square-degree. All will be observed in u,g,r,i and z, with very long exposure time obs_copyright = (c) CFH - powered by Terapix - healpixed by CDS obs_copyright_url = http://terapix.iap.fr/rubrique.php?id_rubrique=32 client_category = Image/Optical/CFHTLS/DEEP client_sort_key = 03-04-02-00 hips_release_date = 2019-05-05T05:08Z hips_creator = CDS hips_version = 1.4 hips_order = 12 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = jpeg dataproduct_type = image moc_access_url = http://alasky.u-strasbg.fr/CFHTLS-T0007b/Deep/RGB-UGIm/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = The CFHT Science Archive contains data and meta-data provided by the Canada-France-Hawaii Telescope prov_progenitor = CFHT bib_reference = 2012yCat.2317....0H bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2012yCat.2317....0H bib_reference_url = http://www.cfht.hawaii.edu/Science/CFHTLS/T0007/CFHTLS_T0007-TechnicalDocumentation.pdf t_min = 53887 t_max = 54832 obs_regime = Optical em_min = 3.266e-7 em_max = 8.594e-7 hips_builder = Aladin/HipsGen v10.123 hips_creation_date = 2012-10-08T15:23Z hips_pixel_scale = 2.795E-5 moc_sky_fraction = 1.009E-4 hips_estsize = 2405144993 hipsgen_date = 2017-03-28T09:09Z hipsgen_params = out=RGB-UGIm UPDATE hips_initial_fov = 1.9 hips_initial_ra = 150.0604395 hips_initial_dec = 2.1806837 hips_order_min = 0 dataproduct_subtype = color hipsgen_date_1 = 2019-05-05T05:08Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/CFHTLS-T0007b/Deep/RGB-UGIm UPDATE hips_service_url = https://alasky.cds.unistra.fr/CFHTLS-T0007b/Deep/RGB-UGIm hips_service_url_1 = https://alaskybis.cds.unistra.fr/CFHTLS-T0007b/Deep/RGB-UGIm hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 12 obs_initial_ra = 150.0604395 obs_initial_dec = 2.1806837 obs_initial_fov = 0.014314526715905856 TIMESTAMP = 1721288413518 ID = CDS/P/CFHTLS/D/g hips_doi = 10.26093/cds/aladin/3rkf-ff4 creator_did = ivo://CDS/P/CFHTLS/D/g obs_collection = CFHTLS D g obs_title = CFHTLS-D-g obs_description = The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The Deep survey concerns 4 patchsof 1 square-degree. All will be observed in u,g,r,i and z, with very lon gexposure time obs_copyright = (c) CFH - powered by Terapix - healpixed by CDS obs_copyright_url = http://terapix.iap.fr/rubrique.php?id_rubrique=32 client_category = Image/Optical/CFHTLS/DEEP client_sort_key = 03-04-02-02 hips_release_date = 2019-05-05T05:09Z hips_creator = CDS hips_version = 1.4 hips_order = 12 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = jpeg fits dataproduct_type = image moc_access_url = http://alasky.unistra.fr/CFHTLS-T0007b/Deep/GALLSKY/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = The CFHT Science Archive contains data and meta-data provided by the Canada-France-Hawaii Telescope prov_progenitor = CFHT bib_reference = 2012yCat.2317....0H bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2012yCat.2317....0H bib_reference_url = http://www.cfht.hawaii.edu/Science/CFHTLS/T0007/CFHTLS_T0007-TechnicalDocumentation.pdf t_min = 53887 t_max = 54832 obs_regime = Optical em_min = 3.973e-7 em_max = 5.795e-7 hips_builder = Aladin/HipsGen v10.123 hips_creation_date = 2012-06-07T22:09Z hips_pixel_scale = 2.795E-5 hips_pixel_bitpix = -32 hips_pixel_cut = -0.3581 4.66 moc_sky_fraction = 1.044E-4 hips_estsize = 29427511 hipsgen_date = 2017-03-28T08:57Z hipsgen_params = out=GALLSKY mocorder=11 "pixelCut=-0.3581 4.66" UPDATE hips_initial_fov = 1.9 hips_initial_ra = 150.0604395 hips_initial_dec = 2.1806837 hips_order_min = 0 hipsgen_date_1 = 2019-05-05T05:09Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/CFHTLS-T0007b/Deep/GALLSKY UPDATE hips_service_url = https://alasky.cds.unistra.fr/CFHTLS-T0007b/Deep/GALLSKY hips_service_url_1 = https://alaskybis.cds.unistra.fr/CFHTLS-T0007b/Deep/GALLSKY hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 150.0604395 obs_initial_dec = 2.1806837 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288413598 ID = CDS/P/CFHTLS/D/i hips_doi = 10.26093/cds/aladin/b8z4-73 creator_did = ivo://CDS/P/CFHTLS/D/i obs_collection = CFHTLS D i obs_title = CFHTLS-D-i obs_description = The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The Deep survey concerns 4 patchsof 1 square-degree. All will be observed in u,g,r,i and z, with very lon gexposure time obs_copyright = (c) CFH - powered by Terapix - healpixed by CDS obs_copyright_url = http://terapix.iap.fr/rubrique.php?id_rubrique=32 client_category = Image/Optical/CFHTLS/DEEP client_sort_key = 03-04-02-04 hips_release_date = 2019-05-05T05:09Z hips_creator = CDS hips_version = 1.4 hips_order = 12 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = jpeg fits dataproduct_type = image moc_access_url = http://alasky.u-strasbg.fr/CFHTLS-T0007b/Deep/IALLSKY/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = The CFHT Science Archive contains data and meta-data provided by the Canada-France-Hawaii Telescope prov_progenitor = CFHT bib_reference = 2012yCat.2317....0H bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2012yCat.2317....0H bib_reference_url = http://www.cfht.hawaii.edu/Science/CFHTLS/T0007/CFHTLS_T0007-TechnicalDocumentation.pdf t_min = 53887 t_max = 54832 obs_regime = Optical em_min = 6.696e-7 em_max = 8.594e-7 hips_builder = Aladin/HipsGen v10.123 hips_creation_date = 2012-06-05T14:27Z hips_pixel_scale = 2.795E-5 hips_pixel_bitpix = -32 hips_pixel_cut = -0.5675 4 moc_sky_fraction = 1.044E-4 hips_estsize = 29427511 hipsgen_date = 2017-03-28T09:02Z hipsgen_params = out=IALLSKY mocorder=11 "pixelCut=-0.5675 4" UPDATE hips_initial_fov = 1.9 hips_initial_ra = 150.0604395 hips_initial_dec = 2.1806837 hips_order_min = 0 hipsgen_date_1 = 2019-05-05T05:09Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/CFHTLS-T0007b/Deep/IALLSKY UPDATE hips_service_url = https://alasky.cds.unistra.fr/CFHTLS-T0007b/Deep/IALLSKY hips_service_url_1 = https://alaskybis.cds.unistra.fr/CFHTLS-T0007b/Deep/IALLSKY hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 150.0604395 obs_initial_dec = 2.1806837 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288413666 ID = CDS/P/CFHTLS/D/r hips_doi = 10.26093/cds/aladin/2eem-p8f creator_did = ivo://CDS/P/CFHTLS/D/r obs_collection = CFHTLS D r obs_title = CFHTLS-D-r obs_description = The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The Deep survey concerns 4 patchsof 1 square-degree. All will be observed in u,g,r,i and z, with very lon gexposure time obs_copyright = (c) CFH - powered by Terapix - healpixed by CDS obs_copyright_url = http://terapix.iap.fr/rubrique.php?id_rubrique=32 client_category = Image/Optical/CFHTLS/DEEP client_sort_key = 03-04-02-03 hips_release_date = 2019-05-05T05:10Z hips_creator = CDS hips_version = 1.4 hips_order = 12 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = jpeg fits dataproduct_type = image moc_access_url = http://alasky.u-strasbg.fr/CFHTLS-T0007b/Deep/RALLSKY/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = The CFHT Science Archive contains data and meta-data provided by the Canada-France-Hawaii Telescope prov_progenitor = CFHT bib_reference = 2012yCat.2317....0H bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2012yCat.2317....0H bib_reference_url = http://www.cfht.hawaii.edu/Science/CFHTLS/T0007/CFHTLS_T0007-TechnicalDocumentation.pdf t_min = 53887 t_max = 54832 obs_regime = Optical em_min = 5.407e-7 em_max = 7.037e-7 hips_builder = Aladin/HipsGen v10.123 hips_creation_date = 2012-06-01T15:10Z hips_pixel_scale = 2.795E-5 hips_pixel_bitpix = -32 hips_pixel_cut = -0.6121 3.798 moc_sky_fraction = 1.044E-4 hips_estsize = 29427511 hipsgen_date = 2017-03-28T09:04Z hipsgen_params = out=RALLSKY mocorder=11 "pixelCut=-0.6121 3.798" UPDATE hips_initial_fov = 1.9 hips_initial_ra = 150.0604395 hips_initial_dec = 2.1806837 hips_order_min = 0 hipsgen_date_1 = 2019-05-05T05:10Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/CFHTLS-T0007b/Deep/RALLSKY UPDATE hips_service_url = https://alasky.cds.unistra.fr/CFHTLS-T0007b/Deep/RALLSKY hips_service_url_1 = https://alaskybis.cds.unistra.fr/CFHTLS-T0007b/Deep/RALLSKY hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 150.0604395 obs_initial_dec = 2.1806837 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288413722 ID = CDS/P/CFHTLS/D/u hips_doi = 10.26093/cds/aladin/18xk-5c creator_did = ivo://CDS/P/CFHTLS/D/u obs_collection = CFHTLS D u obs_title = CFHTLS-D-u obs_description = The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The Deep survey concerns 4 patchsof 1 square-degree. All will be observed in u,g,r,i and z, with very lon gexposure time obs_copyright = (c) CFH - powered by Terapix - healpixed by CDS obs_copyright_url = http://terapix.iap.fr/rubrique.php?id_rubrique=32 client_category = Image/Optical/CFHTLS/DEEP client_sort_key = 03-04-02-01 hips_release_date = 2019-05-05T05:10Z hips_creator = CDS hips_version = 1.4 hips_order = 12 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = jpeg fits dataproduct_type = image moc_access_url = http://alasky.u-strasbg.fr/CFHTLS-T0007b/Deep/UALLSKY/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = The CFHT Science Archive contains data and meta-data provided by the Canada-France-Hawaii Telescope prov_progenitor = CFHT bib_reference = 2012yCat.2317....0H bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2012yCat.2317....0H bib_reference_url = http://www.cfht.hawaii.edu/Science/CFHTLS/T0007/CFHTLS_T0007-TechnicalDocumentation.pdf t_min = 53887 t_max = 54832 obs_regime = Optical em_min = 3.266e-7 em_max = 5.169e-7 hips_builder = Aladin/HipsGen v10.123 hips_creation_date = 2012-06-07T22:09Z hips_pixel_scale = 2.795E-5 hips_pixel_bitpix = -32 hips_pixel_cut = -0.4982 3.221 moc_sky_fraction = 1.044E-4 hips_estsize = 29427511 hipsgen_date = 2017-03-28T09:05Z hipsgen_params = out=UALLSKY mocorder=11 "pixelCut=-0.4982 3.221" UPDATE hips_initial_fov = 1.9 hips_initial_ra = 150.0604395 hips_initial_dec = 2.1806837 hips_order_min = 0 hipsgen_date_1 = 2019-05-05T05:10Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/CFHTLS-T0007b/Deep/UALLSKY UPDATE hips_service_url = https://alasky.cds.unistra.fr/CFHTLS-T0007b/Deep/UALLSKY hips_service_url_1 = https://alaskybis.cds.unistra.fr/CFHTLS-T0007b/Deep/UALLSKY hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 150.0604395 obs_initial_dec = 2.1806837 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288413786 ID = CDS/P/CFHTLS/D/z hips_doi = 10.26093/cds/aladin/2933-m9x creator_did = ivo://CDS/P/CFHTLS/D/z obs_collection = CFHTLS D z obs_title = CFHTLS-D-z obs_description = The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The Deep survey concerns 4 patchsof 1 square-degree. All will be observed in u,g,r,i and z, with very lon gexposure time obs_copyright = (c) CFH - powered by Terapix - healpixed by CDS obs_copyright_url = http://terapix.iap.fr/rubrique.php?id_rubrique=32 client_category = Image/Optical/CFHTLS/DEEP client_sort_key = 03-04-02-05 hips_release_date = 2019-05-05T05:10Z hips_creator = CDS hips_version = 1.4 hips_order = 12 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = jpeg fits dataproduct_type = image moc_access_url = http://alasky.u-strasbg.fr/CFHTLS-T0007b/Deep/ZALLSKY/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = The CFHT Science Archive contains data and meta-data provided by the Canada-France-Hawaii Telescope prov_progenitor = CFHT bib_reference = 2012yCat.2317....0H bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2012yCat.2317....0H bib_reference_url = http://www.cfht.hawaii.edu/Science/CFHTLS/T0007/CFHTLS_T0007-TechnicalDocumentation.pdf t_min = 53887 t_max = 54832 obs_regime = Optical em_min = 8.0098e-7 em_max = 1.0226e-6 hips_builder = Aladin/HipsGen v10.123 hips_creation_date = 2012-06-07T22:09Z hips_pixel_scale = 2.795E-5 hips_pixel_bitpix = -32 hips_pixel_cut = -1.691 10 moc_sky_fraction = 1.044E-4 hips_estsize = 29427511 hipsgen_date = 2017-03-28T09:08Z hipsgen_params = out=ZALLSKY mocorder=11 "pixelCut=-1.691 10" UPDATE hips_initial_fov = 1.9 hips_initial_ra = 150.0604395 hips_initial_dec = 2.1806837 hips_order_min = 0 hipsgen_date_1 = 2019-05-05T05:10Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/CFHTLS-T0007b/Deep/ZALLSKY UPDATE hips_service_url = https://alasky.cds.unistra.fr/CFHTLS-T0007b/Deep/ZALLSKY hips_service_url_1 = https://alaskybis.cds.unistra.fr/CFHTLS-T0007b/Deep/ZALLSKY hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 150.0604395 obs_initial_dec = 2.1806837 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288413858 ID = CDS/P/CFHTLS/W/Color/ugi hips_doi = 10.26093/cds/aladin/perk-q6 creator_did = ivo://CDS/P/CFHTLS/W/Color/ugi obs_collection = CFHTLS W Color ugi obs_title = CFHTLS-W-colored-ugi obs_description = The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The WIDE survey concerns 4 patchs, 3 of about 7x7 square-degrees each and 1 of about 4x4 square-degrees. All will be observed in u,g,r,i and z, with about 1 hr exposure time per filter obs_copyright = (c) CFH - powered by Terapix - healpixed by CDS obs_copyright_url = http://terapix.iap.fr/rubrique.php?id_rubrique=32 client_category = Image/Optical/CFHTLS/WIDE client_sort_key = 03-04-01-00 hips_release_date = 2019-05-05T05:10Z hips_creator = CDS hips_version = 1.4 hips_order = 11 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = jpeg dataproduct_type = image moc_access_url = http://alasky.u-strasbg.fr/CFHTLS-T0007b/Wide/RGB-UGIm/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = The CFHT Science Archive contains data and meta-data provided by the Canada-France-Hawaii Telescope prov_progenitor = CFHT bib_reference = 2012yCat.2317....0H bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2012yCat.2317....0H bib_reference_url = http://www.cfht.hawaii.edu/Science/CFHTLS/T0007/CFHTLS_T0007-TechnicalDocumentation.pdf t_min = 53887 t_max = 54832 obs_regime = Optical em_min = 3.266e-7 em_max = 8.594e-7 hips_creation_date = 2012-10-10T03:23Z hips_pixel_scale = 5.591E-5 hips_builder = Aladin/HipsGen v10.123 moc_sky_fraction = 0.003731 hips_estsize = 601286254 hipsgen_date = 2017-03-27T15:44Z hipsgen_params = out=RGB-UGIm UPDATE hips_initial_fov = 15.0 hips_initial_ra = 34.4537828 hips_initial_dec = -7.2030196 hips_order_min = 0 dataproduct_subtype = color hipsgen_date_1 = 2019-05-05T05:10Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/CFHTLS-T0007b/Wide/RGB-UGIm UPDATE hips_service_url = https://alasky.cds.unistra.fr/CFHTLS-T0007b/Wide/RGB-UGIm hips_service_url_1 = https://alaskybis.cds.unistra.fr/CFHTLS-T0007b/Wide/RGB-UGIm hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 34.4537828 obs_initial_dec = -7.2030196 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288413910 ID = CDS/P/CFHTLS/W/g hips_doi = 10.26093/cds/aladin/3qnf-86d creator_did = ivo://CDS/P/CFHTLS/W/g obs_collection = CFHTLS W g obs_title = CFHTLS-W-g obs_description = The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The WIDE survey concerns 4 patchs, 3 of about 7x7 square-degrees each and 1 of about 4x4 square-degrees. All will be observed in u,g,r,i and z, with about 1 hr exposure time per filter obs_copyright = (c) CFH - powered by Terapix - healpixed by CDS obs_copyright_url = http://terapix.iap.fr/rubrique.php?id_rubrique=32 client_category = Image/Optical/CFHTLS/WIDE client_sort_key = 03-04-01-02 hips_release_date = 2019-05-05T05:11Z hips_creator = CDS hips_version = 1.4 hips_order = 11 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = jpeg fits dataproduct_type = image moc_access_url = http://alasky.u-strasbg.fr/CFHTLS-T0007b/Wide/GALLSKY/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = The CFHT Science Archive contains data and meta-data provided by the Canada-France-Hawaii Telescope prov_progenitor = CFHT bib_reference = 2012yCat.2317....0H bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2012yCat.2317....0H bib_reference_url = http://www.cfht.hawaii.edu/Science/CFHTLS/T0007/CFHTLS_T0007-TechnicalDocumentation.pdf t_min = 53887 t_max = 54832 obs_regime = Optical em_min = 3.973e-7 em_max = 5.795e-7 hips_builder = Aladin/HipsGen v10.123 hips_creation_date = 2012-05-24T16:45Z hips_pixel_scale = 5.591E-5 hips_pixel_bitpix = -32 hips_pixel_cut = -1.285 9.754 hipsgen_date = 2017-03-27T15:28Z hipsgen_params = out=GALLSKY "pixelCut=-1.285 9.754" UPDATE hips_initial_fov = 15.0 hips_initial_ra = 34.4537828 hips_initial_dec = -7.2030196 hips_order_min = 0 moc_sky_fraction = 0.003731 hips_estsize = 72897665441 hipsgen_date_1 = 2019-05-05T05:11Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/CFHTLS-T0007b/Wide/GALLSKY UPDATE hips_service_url = https://alasky.cds.unistra.fr/CFHTLS-T0007b/Wide/GALLSKY hips_service_url_1 = https://alaskybis.cds.unistra.fr/CFHTLS-T0007b/Wide/GALLSKY hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 34.4537828 obs_initial_dec = -7.2030196 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288413966 ID = CDS/P/CFHTLS/W/i hips_doi = 10.26093/cds/aladin/4ez3-ea creator_did = ivo://CDS/P/CFHTLS/W/i obs_collection = CFHTLS W i obs_title = CFHTLS-W-i obs_description = The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The WIDE survey concerns 4 patchs, 3 of about 7x7 square-degrees each and 1 of about 4x4 square-degrees. All will be observed in u,g,r,i and z, with about 1 hr exposure time per filter obs_copyright = (c) CFH - powered by Terapix - healpixed by CDS obs_copyright_url = http://terapix.iap.fr/rubrique.php?id_rubrique=32 client_category = Image/Optical/CFHTLS/WIDE client_sort_key = 03-04-01-04 hips_release_date = 2019-05-05T05:15Z hips_creator = CDS hips_version = 1.4 hips_order = 11 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = jpeg fits dataproduct_type = image moc_access_url = http://alasky.u-strasbg.fr/CFHTLS-T0007b/Wide/IALLSKY/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = The CFHT Science Archive contains data and meta-data provided by the Canada-France-Hawaii Telescope prov_progenitor = CFHT bib_reference = 2012yCat.2317....0H bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2012yCat.2317....0H bib_reference_url = http://www.cfht.hawaii.edu/Science/CFHTLS/T0007/CFHTLS_T0007-TechnicalDocumentation.pdf t_min = 53887 t_max = 54832 obs_regime = Optical em_min = 6.696e-7 em_max = 8.594e-7 hips_builder = Aladin/HipsGen v10.123 hips_creation_date = 2012-05-31T13:54Z hips_pixel_scale = 5.591E-5 hips_pixel_bitpix = -32 hips_pixel_cut = -2.619 20.58 moc_sky_fraction = 0.003731 hips_estsize = 272024098 hipsgen_date = 2017-03-27T15:31Z hipsgen_params = out=IALLSKY mocorder=11 "pixelCut=-2.619 20.58" UPDATE hips_initial_fov = 15.0 hips_initial_ra = 34.4537828 hips_initial_dec = -7.2030196 hips_order_min = 0 hipsgen_date_1 = 2019-05-05T05:15Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/CFHTLS-T0007b/Wide/IALLSKY UPDATE hips_service_url = https://alasky.cds.unistra.fr/CFHTLS-T0007b/Wide/IALLSKY hips_service_url_1 = https://alaskybis.cds.unistra.fr/CFHTLS-T0007b/Wide/IALLSKY hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 34.4537828 obs_initial_dec = -7.2030196 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288414034 ID = CDS/P/CFHTLS/W/r hips_doi = 10.26093/cds/aladin/218m-h16 creator_did = ivo://CDS/P/CFHTLS/W/r obs_collection = CFHTLS W r obs_title = CFHTLS-W-r obs_description = The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The WIDE survey concerns 4 patchs, 3 of about 7x7 square-degrees each and 1 of about 4x4 square-degrees. All will be observed in u,g,r,i and z, with about 1 hr exposure time per filter obs_copyright = (c) CFH - powered by Terapix - healpixed by CDS obs_copyright_url = http://terapix.iap.fr/rubrique.php?id_rubrique=32 client_category = Image/Optical/CFHTLS/WIDE client_sort_key = 03-04-01-03 hips_release_date = 2019-05-05T05:15Z hips_creator = CDS hips_version = 1.4 hips_order = 11 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = jpeg fits dataproduct_type = image moc_access_url = http://alasky.u-strasbg.fr/CFHTLS-T0007b/Wide/RALLSKY/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = The CFHT Science Archive contains data and meta-data provided by the Canada-France-Hawaii Telescope prov_progenitor = CFHT bib_reference = 2012yCat.2317....0H bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2012yCat.2317....0H bib_reference_url = http://www.cfht.hawaii.edu/Science/CFHTLS/T0007/CFHTLS_T0007-TechnicalDocumentation.pdf t_min = 53887 t_max = 54832 obs_regime = Optical em_min = 5.407e-7 em_max = 7.037e-7 hips_builder = Aladin/HipsGen v10.123 hips_creation_date = 2012-05-25T16:11Z hips_pixel_scale = 5.591E-5 hips_pixel_bitpix = -32 hips_pixel_cut = -1.754 15.9 hipsgen_date = 2017-03-27T15:34Z hipsgen_params = out=RALLSKY mocorder=11 "pixelCut=-1.754 15.9" UPDATE hips_initial_fov = 15.0 hips_initial_ra = 34.4537828 hips_initial_dec = -7.2030196 hips_order_min = 0 moc_sky_fraction = 0.003731 hips_estsize = 72897665441 hipsgen_date_1 = 2019-05-05T05:15Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/CFHTLS-T0007b/Wide/RALLSKY UPDATE hips_service_url = https://alasky.cds.unistra.fr/CFHTLS-T0007b/Wide/RALLSKY hips_service_url_1 = https://alaskybis.cds.unistra.fr/CFHTLS-T0007b/Wide/RALLSKY hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 34.4537828 obs_initial_dec = -7.2030196 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288414106 ID = CDS/P/CFHTLS/W/u hips_doi = 10.26093/cds/aladin/eexm-c5 creator_did = ivo://CDS/P/CFHTLS/W/u obs_collection = CFHTLS W u obs_title = CFHTLS-W-u obs_description = The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The Deep survey concerns 4 patchs, 3 of about 7x7 square-degrees each and 1 of about 4x4 square-degrees. All will be observed in u,g,r,i and z, with about 1 hr exposure time per filter obs_copyright = (c) CFH - powered by Terapix - healpixed by CDS obs_copyright_url = http://terapix.iap.fr/rubrique.php?id_rubrique=32 client_category = Image/Optical/CFHTLS/WIDE client_sort_key = 03-04-01-01 hips_release_date = 2019-05-05T05:25Z hips_creator = CDS hips_version = 1.4 hips_order = 11 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = jpeg fits dataproduct_type = image moc_access_url = http://alasky.u-strasbg.fr/CFHTLS-T0007b/Wide/UALLSKY/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = The CFHT Science Archive contains data and meta-data provided by the Canada-France-Hawaii Telescope prov_progenitor = CFHT bib_reference = 2012yCat.2317....0H bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2012yCat.2317....0H bib_reference_url = http://www.cfht.hawaii.edu/Science/CFHTLS/T0007/CFHTLS_T0007-TechnicalDocumentation.pdf t_min = 53887 t_max = 54832 obs_regime = Optical em_min = 3.266e-7 em_max = 5.169e-7 hips_builder = Aladin/HipsGen v10.123 hips_creation_date = 2012-06-05T03:20Z hips_pixel_scale = 5.591E-5 hips_pixel_bitpix = -32 hips_pixel_cut = -1.502 11.87 moc_sky_fraction = 0.003731 hips_estsize = 272024098 hipsgen_date = 2017-03-27T15:36Z hipsgen_params = out=UALLSKY mocorder=11 "pixelCut=-1.502 11.87" UPDATE hips_initial_fov = 15.0 hips_initial_ra = 34.4537828 hips_initial_dec = -7.2030196 hips_order_min = 0 hipsgen_date_1 = 2019-05-05T05:25Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/CFHTLS-T0007b/Wide/UALLSKY UPDATE hips_service_url = https://alasky.cds.unistra.fr/CFHTLS-T0007b/Wide/UALLSKY hips_service_url_1 = https://alaskybis.cds.unistra.fr/CFHTLS-T0007b/Wide/UALLSKY hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 34.4537828 obs_initial_dec = -7.2030196 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288414162 ID = CDS/P/CFHTLS/W/z hips_doi = 10.26093/cds/aladin/2653-k0m creator_did = ivo://CDS/P/CFHTLS/W/z obs_collection = CFHTLS W z obs_title = CFHTLS-W-z obs_description = The Canada-France-Hawaii Telescope Legacy Survey is a 5-year program carried out jointly by the Canadian and French agencies. It will use the Megaprime/Megacam instrument mounted at prime focus of the 3.6m CFH telescope during the period 2003-2008. The WIDE survey concerns 4 patchs, 3 of about 7x7 square-degrees each and 1 of about 4x4 square-degrees. All will be observed in u,g,r,i and z, with about 1 hr exposure time per filter obs_copyright = (c) CFH - powered by Terapix - healpixed by CDS obs_copyright_url = http://terapix.iap.fr/rubrique.php?id_rubrique=32 client_category = Image/Optical/CFHTLS/WIDE client_sort_key = 03-04-01-05 hips_release_date = 2019-05-05T05:25Z hips_creator = CDS hips_version = 1.4 hips_order = 11 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = jpeg fits dataproduct_type = image moc_access_url = http://alasky.u-strasbg.fr/CFHTLS-T0007b/Wide/ZALLSKY/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = The CFHT Science Archive contains data and meta-data provided by the Canada-France-Hawaii Telescope prov_progenitor = CFHT bib_reference = 2012yCat.2317....0H bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2012yCat.2317....0H bib_reference_url = http://www.cfht.hawaii.edu/Science/CFHTLS/T0007/CFHTLS_T0007-TechnicalDocumentation.pdf t_min = 53887 t_max = 54832 obs_regime = Optical em_min = 8.009e-7 em_max = 1.0226e-6 hips_builder = Aladin/HipsGen v10.123 hips_creation_date = 2012-05-29T21:35Z hips_pixel_scale = 5.591E-5 hips_pixel_bitpix = -32 hips_pixel_cut = -6.448 59.75 moc_sky_fraction = 0.003731 hips_estsize = 272024098 hipsgen_date = 2017-03-27T15:39Z hipsgen_params = out=ZALLSKY mocorder=11 "pixelCut=-6.448 59.75" UPDATE hips_initial_fov = 15.0 hips_initial_ra = 34.4537828 hips_initial_dec = -7.2030196 hips_order_min = 0 hipsgen_date_1 = 2019-05-05T05:25Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/CFHTLS-T0007b/Wide/ZALLSKY UPDATE hips_service_url = https://alasky.cds.unistra.fr/CFHTLS-T0007b/Wide/ZALLSKY hips_service_url_1 = https://alaskybis.cds.unistra.fr/CFHTLS-T0007b/Wide/ZALLSKY hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 34.4537828 obs_initial_dec = -7.2030196 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288414218 ID = CDS/P/CO hips_doi = 10.26093/cds/aladin/1zd9-hss creator_did = ivo://CDS/P/CO obs_collection = CO composite survey obs_title = CO composite survey obs_description = This survey contains data from the composite CO map constructed by Dame, Hartmann and Thaddeus (2001) from 37 individual surveys of the Galaxy in the CO (1-0) line. Due to the composite nature of the map and processing used to render a uniform S/N appearance, the user is cautioned that angular resolution and sensitivity vary across the map. Survey data are limited to Galactic latitudes |b|<32 deg., with roughly half of that area containing observations.To create this file, the velocity-integrated brightness temperature map, W(CO), was obtained from the CfA Millimeter Wave Group website and then interpolated onto a HEALPix grid with Nside=512. obs_copyright = Composite map by Dame et al (2001,ApJ,547,792), - HEALPixed by LAMBDA obs_copyright_url = http://lambda.gsfc.nasa.gov/product/foreground/fg_WCO_get.cfm client_category = Image/Gas-lines/CO client_sort_key = 06-08-01 hips_creation_date = 2011-02-14T12:00Z hips_release_date = 2019-05-05T06:00Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 3 hips_frame = galactic hips_tile_width = 64 hips_tile_format = jpeg fits dataproduct_type = image moc_access_url = http://alasky.u-strasbg.fr/CO/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = We acknowledge the use of the Legacy Archive for Microwave Background Data Analysis (LAMBDA), part of the High Energy Astrophysics Science Archive Center (HEASARC). HEASARC/LAMBDA is a service of the Astrophysics Science Division at the NASA Goddard Space Flight Center." prov_progenitor = HEASARC/LAMBDA bib_reference = 2001ApJ...547..792D bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2001ApJ...547..792D t_min = 44239 t_max = 51544 obs_regime = Radio em_min = 2.604173540653e-3 em_max = 2.609386874402e-3 hips_pixel_scale = 0.01431 hips_initial_fov = 158.63230142835039 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 1112337 hipsgen_date = 2019-05-05T06:00Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/CO UPDATE hips_service_url = https://alasky.cds.unistra.fr/CO hips_service_url_1 = https://alaskybis.cds.unistra.fr/CO hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288414282 ID = CDS/P/CO-Dame-2022 hips_initial_fov = 360.0 hips_initial_ra = 266.415009 hips_initial_dec = -29.0061110 creator_did = ivo://CDS/P/CO-Dame-2022 hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = Dame and Thaddeus 2022 Velocity Integrated CO Map obs_collection = Dame CO maps obs_description = Data published by Dame & Thaddeus (2022) significantly extends the Galactic plane CO survey of Dame, Hartmann & Thaddeus (2001) with complementary coverage of the entire northern sky (? > -17°). The coverage extension was carried out with the same telescope as was used for the plane survey, the CfA 1.2 m, and perfectly meshes with its irregular boundaries in latitude. The merged survey is released by the authors in the form of CO line spectral data cubes. To create the LAMBDA map, the moment-masked data cube for the combined survey was integrated over +/- 36 km/sec, the full range over which significant emission is detected (see Figure 8 of Dame & Thaddeus 2022; the combined survey does not include the high-velocity observations available from the Dame, Hartmann & Thaddeus 2001 data). The velocity integrated brightness temperature map was then interpolated from the original rectilinear projection onto pixel centers appropriate for HEALPix Nside=256. The LAMBDA map is in units of K-km/sec, and a mask is provided indicating those portions of the sky that are unobserved. obs_ack = We acknowledge the use of the Legacy Archive for Microwave Background Data Analysis (LAMBDA), part of the High Energy Astrophysics Science Archive Center (HEASARC). HEASARC/LAMBDA is a service of the Astrophysics Science Division at the NASA Goddard Space Flight Center." prov_progenitor = HEASARC/LAMBDA bib_reference = 2022ApJS..262....5D bib_reference_url = https://ui.adsabs.harvard.edu/abs/2022ApJS..262....5D obs_copyright = Composite map by Dame & Thaddeus (2022 ApJS, 262, 5) - HEALPixed by LAMBDA obs_copyright_url = https://lambda.gsfc.nasa.gov/product/foreground/fg_wco_dt2022_get.html client_category = Image/Gas-lines/CO obs_regime = Radio em_min = 2.604173540653e-3 em_max = 2.609386874402e-3 hips_builder = Aladin/HipsGen v12.119 hips_version = 1.4 hips_frame = galactic hips_order = 3 hips_order_min = 0 hips_tile_width = 32 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_bitpix = -32 hips_pixel_cut = -1 210 hips_data_range = -382.9 1137 hips_pixel_scale = 0.01431 dataproduct_type = image hipsgen_date = 2024-07-17T09:58Z hipsgen_params = in=lambda_Wco_DT2022.fits out=./hips id=CDS/P/CO-Dame-2022 MAPTILES hips_release_date = 2024-07-17T10:09Z hips_creation_date = 2024-07-17T09:58Z moc_sky_fraction = 1 hipsgen_date_1 = 2024-07-17T10:00Z hipsgen_params_1 = in=lambda_Wco_DT2022.fits out=./hips id=CDS/P/CO-Dame-2022 blank=0 MAPTILES hipsgen_date_2 = 2024-07-17T10:09Z hipsgen_params_2 = in=lambda_Wco_DT2022.fits out=./hips id=CDS/P/CO-Dame-2022 blank=0 "pixelCut=-1 210 log" PNG hips_service_url = https://alasky.cds.unistra.fr/CO-maps/CDS_P_CO-Dame-2022 hips_service_url_1 = https://alaskybis.cds.unistra.fr/CO-maps/CDS_P_CO-Dame-2022 hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 3 obs_initial_ra = 266.415009 obs_initial_dec = -29.0061110 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288498778 ID = CDS/P/COHRS hips_doi = 10.26093/cds/aladin/3ash-cyq creator_did = ivo://CDS/P/COHRS obs_collection = CO High Resolution Survey obs_title = CO High Resolution Survey (HARP/JCMT) obs_description = This survey contains data from the CO High Resolution Survey (COHRS). The data we're taken in the 12CO(J=3-2) line with HARP (JCMT). The FWHM of the observations are 14". THe survey and data products are fully described in Dempsey, Thomas & Currie 2013, ApJS, 209, 8. The data cubes have been collapsed in the velocity axis between -30 and +155km/s to provide 2D integrated maps. These maps are publicly available at CADC (http://dx.doi. org/10.11570/13.0002). These 2D integrated maps were then interpolated onto a HEALPix grid with Nside=65536 at CDS obs_copyright = CANFAR obs_copyright_url = http://www.canfar.phys.uvic.ca/canfar/ client_category = Image/Gas-lines/CO client_sort_key = 06-08-02 hips_creation_date = 2014-03-11T15:59Z hips_release_date = 2019-05-05T05:26Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 7 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png jpeg fits dataproduct_type = image hips_pixel_cut = 6.918 284.2 hips_data_range = 1.571 510.9 hips_initial_ra = 282.93615 hips_initial_dec = +00.12902 hips_initial_fov = 4 moc_access_url = http://alasky.u-strasbg.fr/COHRS/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = CANFAR prov_progenitor = CANFAR - healpixed by CDS bib_reference = 2013ApJS..209....8D bib_reference_url = http://cdsads.u-strasbg.fr/abs/2013ApJS..209....8D t_min = 55197 t_max = 55927 obs_regime = Infrared em_min = 7.9E-4 em_max = 9.2E-4 hips_hierarchy = mean hips_pixel_scale = 8.946E-4 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 0.001495 hips_estsize = 288279674 hipsgen_date = 2019-05-05T05:26Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/COHRS UPDATE hips_service_url = https://alasky.cds.unistra.fr/COHRS hips_service_url_1 = https://alaskybis.cds.unistra.fr/COHRS hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 7 obs_initial_ra = 282.93615 obs_initial_dec = +00.12902 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288414338 ID = CDS/P/Callisto/Voyager-Galileo-simp-1km client_category = Solar system/Jupiter/Callisto hips_initial_fov = 180 hips_initial_ra = 0 hips_initial_dec = +0.0 creator_did = ivo://CDS/P/Callisto/Voyager-Galileo-simp-1km hips_overlay = mean hips_hierarchy = median hips_creator = Fernique P. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = Callisto Voyager-Galileo-simp-1km obs_description = This global map of Callisto utilizes the best image quality and moderate resolution coverage supplied by Galileo SSI (Solid State Imaging instrument) and Voyager 1 and 2. The image processing was performed at USGS using the Integrated Software for Imagers and Spectrometers (ISIS) system. The image data was selected on the basis of overall image quality, reasonable input resolution, and availability of moderate viewing and sun angles for topography. The average input resolution was 1.0 kilometers/pixel. The resolution ranged from 60 km/pixel for gap fill up to 400 meters/pixel. The map projections are based on a sphere having a radius of 2409.3 kilometers. prov_progenitor = Planetary Data System, from USGS Astrogeology Science Center prov_progenitor_url = https://astrogeology.usgs.gov/search/map/Callisto/Voyager-Galileo/callisto_simp_1km hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T07:03Z hips_frame = callisto hips_body = callisto hips_order = 3 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg hips_pixel_scale = 0.01431 s_pixel_scale = 0.02314 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 18357 hipsgen_date = 2018-01-17T16:49Z hipsgen_params = -maxthread=10 in=Callisto creator_did=CDS/P/Callisto/Voyager-Galileo-simp-1km -f color=jpg INDEX TILES hips_creation_date = 2018-01-17T16:49Z hipsgen_date_1 = 2018-01-21T12:41Z hipsgen_params_1 = "hhh=Callisto/Callisto.jpg 15559x7571" partitioning=7571 -maxthread=10 in=Callisto creator_did=CDS/P/Callisto/Voyager-Galileo-simp-1km -f color=jpg INDEX TILES hips_order_min = 0 dataproduct_subtype = color hipsgen_date_2 = 2019-05-21T07:03Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/Planets/CDS_P_Callisto_Voyager-Galileo-simp-1km UPDATE hips_service_url = https://alasky.cds.unistra.fr/Planets/CDS_P_Callisto_Voyager-Galileo-simp-1km hips_service_url_1 = https://alaskybis.cds.unistra.fr/Planets/CDS_P_Callisto_Voyager-Galileo-simp-1km hips_status_1 = public mirror clonableOnce client_application = AladinDesktopBeta>=10.040 AladinDesktop>=11.125 moc_type = smoc moc_order = 3 obs_initial_ra = 0 obs_initial_dec = +0.0 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288466862 ID = CDS/P/Charon/NewHorizon-PIA19866 client_category = Solar system/Pluto/Charon hips_initial_fov = 180 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/Charon/NewHorizon-PIA19866 hips_overlay = mean hips_hierarchy = median hips_creator = Fernique P. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = Charon NewHorizon PIA19866 obs_description = The science team of NASA's New Horizons mission has produced this global map of Pluto's largest moon, Charon. The map includes all available resolved images of the surface acquired between July 7-14, 2015, at pixel resolutions ranging from 40 kilometers (24 miles) on the anti-Pluto facing hemisphere (left and right sides of the map), to 400 meters (1,250 feet) per pixel on portions of the Pluto-facing hemisphere -- the side facing the New Horizons spacecraft when it flew past the dwarf planet -- at map center. Many additional images now stored on the spacecraft's digital data recorders are expected to be transmitted "home" in fall 2015 and these will be used to complete the global map. The map is in simple cylindrical projection, with zero longitude (the Pluto-facing direction) in the center. The Johns Hopkins University Applied Physics Laboratory in Laurel, Maryland, designed, built, and operates the New Horizons spacecraft, and manages the mission for NASA's Science Mission Directorate. The Southwest Research Institute, based in San Antonio, leads the science team, payload operations and encounter science planning. New Horizons is part of the New Frontiers Program managed by NASA's Marshall Space Flight Center in Huntsville, Alabama. obs_ack = ASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute prov_progenitor = JPL/PhotoJournal prov_progenitor_url = https://photojournal.jpl.nasa.gov/catalog/PIA19866 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T07:05Z hips_frame = charon hips_body = charon hips_order = 3 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg hips_pixel_scale = 0.01431 s_pixel_scale = 0.03782 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 18357 hipsgen_date = 2018-01-24T14:27Z hipsgen_params = "hhh=Charon/Charon.jpg 9520x4760" partitioning=4760 -maxthread=10 in=Charon creator_did=CDS/P/Charon/NewHorizon-PIA19866 -f color=jpg INDEX TILES hips_creation_date = 2018-01-24T14:27Z hips_order_min = 0 dataproduct_subtype = color hipsgen_date_1 = 2019-05-21T07:05Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume6/Planets/CDS_P_Charon_NewHorizon-PIA19866 UPDATE hips_service_url = https://alasky.cds.unistra.fr/Planets/CDS_P_Charon_NewHorizon-PIA19866 hips_service_url_1 = https://alaskybis.cds.unistra.fr/Planets/CDS_P_Charon_NewHorizon-PIA19866 hips_status_1 = public mirror clonableOnce client_application = AladinDesktopBeta>=10.040 AladinDesktop>=11.125 moc_type = smoc moc_order = 3 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288467558 ID = CDS/P/Coronelli hips_initial_fov = 360.0 hips_initial_ra = 232.65242 hips_initial_dec = -1.05786 creator_did = ivo://CDS/P/Coronelli hips_overlay = mean hips_hierarchy = median hips_creator = Boch T. (CDS) hips_copyright = CNRS/Unistra. No commercial exploitation nor diffusion of images. Pas d'utilisation commerciale ni de diffusion des images. obs_title = Coronelli obs_collection = Globe céleste de Coronelli de l'Observatoire astronomique de Strasbourg obs_description = Ce Globe céleste de Coronelli datant de 1697 fait partie des collections de l'Observatoire astronomique de Strasbourg. Il a fait l'objet d'une campagne de restauration physique en partenariat avec l'Observatoire astronomique de Strasbourg, le Jardin des sciences de l'Université de Strasbourg, la Fondation Université de Strasbourg et la Bibliothèque nationale et universitaire de Strasbourg. La BNU a pu intervenir pour réaliser quelques 2000 prises de vue ê l'issue de ce processus de restauration, ce qui a permis de produire une version numérisée au format HiPS au Centre de Données astronomiques de Strasbourg. obs_ack = Prises de vues : Jean-Pierre Rosenkranz, Bibliothèque nationale et universitaire de Strasbourg. prov_progenitor = Globe céleste construit en 1697 par Gatellier à partir des gravures du moine cartographe Vincenzo Coronelli. obs_copyright = Jean-Pierre Rosenkranz, Bibliothèque nationale et universitaire de Strasbourg. Pas d'utilisation commerciale ni de diffusion des images. hips_builder = Aladin/HipsGen v11.017 hips_version = 1.4 hips_release_date = 2020-03-06T13:26Z hips_frame = equatorial hips_order = 4 hips_order_min = 0 hips_tile_width = 512 hips_status = public master unclonable hips_tile_format = jpeg png hips_pixel_scale = 0.229 s_pixel_scale = 0.012 dataproduct_type = image dataproduct_subtype = color moc_sky_fraction = 1 hips_estsize = 110106 hipsgen_date = 2020-03-06T13:23Z hipsgen_params = in=input output=CDS_P_Coronelli creator_did=CDS/P/Coronelli partitioning=false maxThread=8 hips_creation_date = 2020-03-06T13:23Z hipsgen_date_1 = 2020-03-06T13:26Z hipsgen_params_1 = in=input output=CDS_P_Coronelli creator_did=CDS/P/Coronelli partitioning=false maxThread=8 jpeg -f hipsgen_date_2 = 2020-03-06T13:26Z hipsgen_params_2 = in=input output=CDS_P_Coronelli creator_did=CDS/P/Coronelli partitioning=false maxThread=8 mode=replacetile jpeg -f hipsgen_date_3 = 2020-03-06T13:26Z hipsgen_params_3 = output=CDS_P_Coronelli creator_did=CDS/P/Coronelli partitioning=false maxThread=8 mode=replacetile jpeg -f hips_service_url = https://alasky.cds.unistra.fr/CDS_P_Coronelli hips_progenitor_url = https://alasky.cds.unistra.fr/CDS_P_Coronelli/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/CDS_P_Coronelli hips_status_1 = public mirror unclonable client_category = Outreach/Constellations moc_type = smoc moc_order = 7 obs_initial_ra = 232.65242 obs_initial_dec = -1.05786 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288490150 ID = CDS/P/DECaLS/DR3/color hips_doi = 10.26093/cds/aladin/112p-t2 creator_did = ivo://CDS/P/DECaLS/DR3/color obs_collection = DECaLS DR3 color obs_title = DECaLS DR3 color obs_description = The Legacy Survey is producing an inference model catalog of the sky from a set of optical and infrared imaging data, comprising 14,000 square deg of extragalactic sky visible from the northern hemisphere in three optical bands (g,r,z) and four infrared bands. The sky coverage is approximately bounded by -18deg < delta < +84deg in celestial coordinates and |b||b| > 18deg in Galactic coordinates. The DECam Legacy Survey is providing these data in the equatorial region at delta < +30deg using the Dark Energy Camera on the Blanco Telescope. The color images are based on the g,r,z filters. Data Release 3 (DR3) is the third public data release of images and catalogs for the DECam Legacy Survey (DECaLS). Images from DECaLS g,r,z-band observations (NOAO survey program 0404; https://www.noao.edu/perl/abstract?2014B-0404) are included from August 2014 through March 2016. DR3 also includes DECam data from a range of non-DECaLS surveys, including observations that were conducted from September 2012 to March 2016. In total, the optical data covers a disjoint footprint with 4300 square deg in g-band, 4600 square deg in r-band and 8100 square deg in z-band, of which 4200 square deg has been observed in all three optical filters. hips_overlay = border_fading hips_hierarchy = first hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg prov_progenitor = http://legacysurvey.org/dr3/files/ bib_reference_url = http://legacysurvey.org/files/LargeSurvey.pdf obs_copyright = DECam Legacy Survey obs_copyright_url = http://legacysurvey.org/ t_min = 56870 t_max = 57478 obs_regime = Optical client_category = Image/Optical/DECaLS client_application = AladinDesktop em_min = 390e-9 em_max = 1026e-9 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T09:17Z hips_frame = equatorial hips_order = 11 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg hips_initial_ra = 327.90213 hips_initial_dec = +7.49996 hips_initial_fov = 0.262 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.277E-5 dataproduct_type = image moc_sky_fraction = 0.2275 hips_estsize = 273621139 hips_creation_date = 2017-01-21T22:35Z hips_order_min = 0 dataproduct_subtype = color hipsgen_date = 2019-05-21T09:17Z hipsgen_params = out=/asd-volumes/sc1-asd-volume1/DECaLS/DR3/color UPDATE hips_service_url = https://alasky.cds.unistra.fr/DECaLS/DR3/color hips_service_url_1 = https://alaskybis.cds.unistra.fr/DECaLS/DR3/color hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 327.90213 obs_initial_dec = +7.49996 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288465166 ID = CDS/P/DECaLS/DR5/color hips_doi = 10.26093/cds/aladin/1gw2-vkr creator_did = ivo://CDS/P/DECaLS/DR5/color obs_title = DECaLS DR5 color obs_collection = DECaLS DR5 color obs_description = The Legacy Survey is producing an inference model catalog of the sky from a set of optical and infrared imaging data, comprising 14,000 square degrees of extragalactic sky visible from the northern hemisphere in three optical bands (g,r,z) and four infrared bands. The sky coverage is approximately bounded by -18deg < delta < +84deg in celestial coordinates and |b||b| > 18deg in Galactic coordinates. The DECam Legacy Survey is providing these data in the equatorial region at delta < +30deg using the Dark Energy Camera on the Blanco Telescope. The color images are based on the g,r,z filters. Data Release 5 (DR5) is the fifth public data release of the Legacy Surveys. DR5 imaging is first reduced through the NOAO Community Pipeline before being processed using the Tractor. Images from DECaLS g,r,z-band observations are included from August 2014 through May 2017. DR5 also includes DECam data from a range of non-DECaLS surveys, including observations that were conducted from September 2012 to May 2017. hips_initial_fov = 0.262 hips_initial_ra = 237.53874 hips_initial_dec = +26.49996 hips_overlay = mean hips_hierarchy = mean hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra prov_progenitor = http://portal.nersc.gov/project/cosmo/data/legacysurvey/dr5/coadd/ bib_reference_url = http://legacysurvey.org/files/LargeSurvey.pdf obs_copyright = DECam Legacy Survey obs_copyright_url = http://legacysurvey.org/ t_min = 56171 t_max = 57874 obs_regime = Optical em_min = 390e-9 em_max = 1026e-9 client_category = Image/Optical/DECaLS client_application = AladinLite client_application = AladinDesktop hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T09:20Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.277E-5 dataproduct_type = image moc_sky_fraction = 0.269 hips_estsize = 323453605 hipsgen_date = 2018-06-07T05:18Z hipsgen_params = in=jpg/ out=/data3/buga/DECaLS_DR5/Hips_DECaLS_DR5_color_mean skyval=true creator_did=CDS/C/DECaLS/DR5/color verbose=3 method=MEAN color=true INDEX TILES DETAILS hips_creation_date = 2018-06-07T05:18Z dataproduct_subtype = color hipsgen_date_1 = 2019-05-21T09:20Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume1/DECaLS/DR5/color UPDATE hips_service_url = https://alasky.cds.unistra.fr/DECaLS/DR5/color hips_service_url_1 = https://alaskybis.cds.unistra.fr/DECaLS/DR5/color hips_status_1 = public mirror clonableOnce hips_service_url_2 = https://healpix.ias.u-psud.fr/CDS_P_DECaLS_DR5_color hips_status_2 = public mirror unclonable moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 237.53874 obs_initial_dec = +26.49996 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1729584609937 ID = CDS/P/DECaLS/DR5/g hips_doi = 10.26093/cds/aladin/2481-9fw creator_did = ivo://CDS/P/DECaLS/DR5/g obs_title = DECaLS DR5 g obs_collection = DECaLS DR5 g obs_description = The Legacy Survey is producing an inference model catalog of the sky from a set of optical and infrared imaging data, comprising 14,000 square degrees of extragalactic sky visible from the northern hemisphere in three optical bands (g,r,z) and four infrared bands. The sky coverage is approximately bounded by -18deg < delta < +84deg in celestial coordinates and |b||b| > 18deg in Galactic coordinates. The DECam Legacy Survey is providing these data in the equatorial region at delta < +30deg using the Dark Energy Camera on the Blanco Telescope. The color images are based on the g,r,z filters. Data Release 5 (DR5) is the fifth public data release of the Legacy Surveys. DR5 imaging is first reduced through the NOAO Community Pipeline before being processed using the Tractor. Images from DECaLS g,r,z-band observations are included from August 2014 through May 2017. DR5 also includes DECam data from a range of non-DECaLS surveys, including observations that were conducted from September 2012 to May 2017. hips_initial_fov = 0.262 hips_initial_ra = 237.53874 hips_initial_dec = +26.49996 hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_skyval_method = TRUE hips_skyval_value = -0.002 0.2 -4.239427832886577 12.596703300252557 hips_overlay = mean hips_hierarchy = mean hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra prov_progenitor = http://portal.nersc.gov/project/cosmo/data/legacysurvey/dr5/coadd/ bib_reference_url = http://legacysurvey.org/files/LargeSurvey.pdf obs_copyright = DECam Legacy Survey obs_copyright_url = http://legacysurvey.org/ t_min = 56171 t_max = 57874 obs_regime = Optical em_min = 3.876e-7 em_max = 5.808e-7 client_category = Image/Optical/DECaLS hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-23T06:38Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = -0.002 0.2 hips_data_range = -4.239 12.6 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.277E-5 dataproduct_type = image moc_sky_fraction = 0.1967 hips_estsize = 14308421415 hipsgen_date = 2018-09-29T08:59Z hipsgen_params = in=/data3/buga/DECaLS_DR5/images_g/ out=/data3/buga/DECaLS_DR5/Hips_DECaLS_DR5_g_mean_BLANK skyval=true creator_did=CDS/C/DECaLS/DR5/g verbose=3 BLANK=0 "hips_pixel_cut=-0.002 0.2 sqrt" method=MEAN INDEX TILES DETAILS PNG hips_creation_date = 2018-09-29T08:59Z hipsgen_date_1 = 2018-10-03T13:13Z hipsgen_params_1 = in=/data3/buga/DECaLS_DR5/images_g/ out=/data3/buga/DECaLS_DR5/Hips_DECaLS_DR5_g_mean_BLANK skyval=true creator_did=CDS/C/DECaLS/DR5/g verbose=3 BLANK=0 "hips_pixel_cut=-0.002 0.2 sqrt" method=MEAN INDEX TILES DETAILS PNG hipsgen_date_2 = 2018-10-12T22:16Z hipsgen_params_2 = in=/data3/buga/DECaLS_DR5/images_g/ out=/data3/buga/DECaLS_DR5/Hips_DECaLS_DR5_g_mean_BLANK -f creator_did=CDS/C/DECaLS/DR5/g verbose=3 BLANK=0 "hips_pixel_cut=-0.002 0.2 sqrt" method=MEAN TILES DETAILS PNG hipsgen_date_3 = 2018-10-13T01:18Z hipsgen_params_3 = in=/data3/buga/DECaLS_DR5/images_g/ out=/data3/buga/DECaLS_DR5/Hips_DECaLS_DR5_g_mean_BLANK -f creator_did=CDS/C/DECaLS/DR5/g verbose=3 BLANK=0 "hips_pixel_cut=-0.002 0.2 sqrt" method=MEAN TILES DETAILS PNG hipsgen_date_4 = 2018-10-17T09:17Z hipsgen_params_4 = in=/data3/buga/DECaLS_DR5/images_g/ out=/data3/buga/DECaLS_DR5/Hips_DECaLS_DR5_g_mean_BLANK -f creator_did=CDS/C/DECaLS/DR5/g verbose=3 BLANK=0 "hips_pixel_cut=-0.002 0.2 sqrt" method=MEAN TILES DETAILS PNG hipsgen_date_5 = 2019-05-23T06:38Z hipsgen_params_5 = out=/asd-volumes/sc1-asd-volume1/DECaLS/DR5/g UPDATE hips_service_url = https://alasky.cds.unistra.fr/DECaLS/DR5/g hips_progenitor_url = https://alasky.cds.unistra.fr/DECaLS/DR5/g/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/DECaLS/DR5/g hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 20 moc_time_range = 68 moc_order = 9 obs_initial_ra = 237.53874 obs_initial_dec = +26.49996 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288479010 ID = CDS/P/DECaLS/DR5/r hips_doi = 10.26093/cds/aladin/3jnt-g8q creator_did = ivo://CDS/P/DECaLS/DR5/r obs_title = DECaLS DR5 r obs_collection = DECaLS DR5 r obs_description = The Legacy Survey is producing an inference model catalog of the sky from a set of optical and infrared imaging data, comprising 14,000 square degrees of extragalactic sky visible from the northern hemisphere in three optical bands (g,r,z) and four infrared bands. 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(CDS) hips_copyright = CNRS/Unistra prov_progenitor = http://portal.nersc.gov/project/cosmo/data/legacysurvey/dr5/coadd/ bib_reference_url = http://legacysurvey.org/files/LargeSurvey.pdf obs_copyright = DECam Legacy Survey obs_copyright_url = http://legacysurvey.org/ t_min = 56171 t_max = 57874 obs_regime = Optical em_min = 5.618e-7 em_max = 7.26e-7 client_category = Image/Optical/DECaLS hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-06-18T11:15Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = -0.002 0.127 hips_data_range = -7.359 21.5 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.277E-5 dataproduct_type = image moc_sky_fraction = 0.1971 hips_estsize = 15604853394 hipsgen_date = 2019-04-01T18:02Z hipsgen_params = in=/data1/buga/DECaLS_DR5/images_r/ out=r/ creator_did=CDS/P/DECaLS/DR5/r verbose=4 BLANK=0 method=MEAN "hips_pixel_cut=-0.002 0.127 sqrt" maxThread=10 TILES PNG DETAILS hips_creation_date = 2019-04-01T18:02Z hipsgen_date_1 = 2019-04-08T09:22Z hipsgen_params_1 = in=/data1/buga/DECaLS_DR5/images_r/ out=r/ creator_did=CDS/P/DECaLS/DR5/r verbose=4 BLANK=0 method=MEAN "hips_pixel_cut=-0.002 0.127 sqrt" PNG DETAILS hipsgen_date_2 = 2019-06-18T11:15Z hipsgen_params_2 = out=r UPDATE hips_service_url = https://alasky.cds.unistra.fr/DECaLS/DR5/r hips_progenitor_url = https://alasky.cds.unistra.fr/DECaLS/DR5/r/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/DECaLS/DR5/r hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 237.53874 obs_initial_dec = +26.49996 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288479066 ID = CDS/P/DECaPS/DR1/color hips_doi = 10.26093/cds/aladin/2e9s-tgp creator_did = ivo://CDS/P/DECaPS/DR1/color client_category = Image/Optical/DECaPS client_application = AladinDesktop hips_initial_fov = 10 hips_initial_ra = 188.9290792 hips_initial_dec = -63.3032221 hips_overlay = mean hips_hierarchy = mean hips_creator = Boch T. (CDS) obs_title = DECaPS DR1 color obs_collection = DECam Plane Survey DR1 color (g, r, z bands) obs_description = The DECam Plane Survey is a five-band optical and near-infrared survey of the southern Galactic plane with the Dark Energy Camera at Cerro Tololo. The survey is designed to reach past the mainsequence turn-off at the distance of the Galactic center through a reddening E(B - V ) of 1.5 mag. Typical single-exposure depths are 23.7, 22.8, 22.3, 21.9, and 21.0 mag in the grizY bands, with seeing around 100. The footprint covers the Galactic plane with |b| <= 4 degrees , 5 degrees > l > 120 degrees prov_progenitor = http://portal.nersc.gov/project/cosmo/data/decaps/dr1/coadd/ bib_reference = 2018ApJS..234...39S bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2018ApJS..234...39S obs_copyright = DECaM Plane Survey / NOAO obs_copyright_url = http://decaps.skymaps.info/ t_min = 57460 t_max = 57876 em_min = 3.805e-7 em_max = 10.150e-7 obs_regime = Optical hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-22T13:57Z hips_frame = equatorial hips_order = 11 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png jpeg hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.277E-5 dataproduct_type = image moc_sky_fraction = 0.03543 hips_estsize = 106532961 hipsgen_date = 2018-01-02T16:02Z hipsgen_params = tiles hips_creation_date = 2018-01-02T16:02Z hipsgen_date_1 = 2018-01-31T09:33Z hipsgen_params_1 = color=png mode=keeptile tiles hips_order_min = 0 dataproduct_subtype = color hipsgen_date_2 = 2019-05-22T13:57Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume2/DECaPS/DR1/color UPDATE hips_service_url = https://alasky.cds.unistra.fr/DECaPS/DR1/color hips_service_url_1 = https://alaskybis.cds.unistra.fr/DECaPS/DR1/color hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 188.9290792 obs_initial_dec = -63.3032221 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288475442 ID = CDS/P/DECaPS/DR1/g hips_doi = 10.26093/cds/aladin/2j9t-aa4 client_category = Image/Optical/DECaPS hips_initial_fov = 10 hips_initial_ra = 188.9290792 hips_initial_dec = -63.3032221 creator_did = ivo://CDS/P/DECaPS/DR1/g hips_pixel_bitpix = 16 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = mean hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = DECaPS DR1 g obs_collection = DECam Plane Survey DR1 g band obs_description = The DECam Plane Survey is a five-band optical and near-infrared survey of the southern Galactic plane with the Dark Energy Camera at Cerro Tololo. The survey is designed to reach past the mainsequence turn-off at the distance of the Galactic center through a reddening E(B - V ) of 1.5 mag. Typical single-exposure depths are 23.7, 22.8, 22.3, 21.9, and 21.0 mag in the grizY bands, with seeing around 100. The footprint covers the Galactic plane with |b| <= 4deg , 5deg > l > -120deg prov_progenitor = http://portal.nersc.gov/project/cosmo/data/decaps/dr1/coadd/ bib_reference = 2018ApJS..234...39S bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2018ApJS..234...39S obs_copyright = DECaM Plane Survey / NOAO obs_copyright_url = http://decaps.skymaps.info/ t_min = 57460 t_max = 57876 obs_regime = Optical em_min = 3.805e-7 em_max = 5.645e-7 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-22T14:08Z hips_frame = equatorial hips_order = 11 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png jpeg fits hips_pixel_cut = -7.105E-15 0.5 hips_data_range = -40 140 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.277E-5 dataproduct_type = image moc_sky_fraction = 0.0351 hips_estsize = 1377036753 hipsgen_date = 2018-01-11T10:59Z hipsgen_params = mode=keeptile tiles hips_creation_date = 2018-01-11T10:59Z hipsgen_date_1 = 2018-01-11T13:05Z hipsgen_params_1 = mode=keeptile tiles hipsgen_date_2 = 2018-01-11T13:07Z hipsgen_params_2 = jpeg hipsgen_date_3 = 2018-01-11T13:07Z hipsgen_params_3 = jpeg hipsgen_date_4 = 2018-01-11T13:09Z hipsgen_params_4 = jpeg hipsgen_date_5 = 2018-01-11T13:19Z hipsgen_params_5 = jpeg hipsgen_date_6 = 2018-01-12T09:59Z hipsgen_params_6 = mode=replacetile jpeg hipsgen_date_7 = 2018-01-18T08:21Z hipsgen_params_7 = maxThread=24 tiles hipsgen_date_8 = 2018-01-18T08:56Z hipsgen_params_8 = jpeg hipsgen_date_9 = 2018-01-18T13:10Z hipsgen_params_9 = mode=replacetile jpeg hipsgen_date_10 = 2018-01-19T03:17Z hipsgen_params_10 = mode=replacetile png hips_order_min = 0 hipsgen_date_11 = 2019-05-22T14:08Z hipsgen_params_11 = out=/asd-volumes/sc1-asd-volume2/DECaPS/DR1/g UPDATE hips_service_url = https://alasky.cds.unistra.fr/DECaPS/DR1/g hips_service_url_1 = https://alaskybis.cds.unistra.fr/DECaPS/DR1/g hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 188.9290792 obs_initial_dec = -63.3032221 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288475498 ID = CDS/P/DECaPS/DR2/Y hips_doi = 10.26093/cds/aladin/1kvn-2np client_category = Image/Optical/DECaPS/DR2 hips_initial_fov = 60.0 hips_initial_ra = 188.9290792 hips_initial_dec = -63.3032221 moc_sky_fraction = 0.06582 creator_did = ivo://CDS/P/DECaPS/DR2/Y hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = mean hips_creator = Buga M. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = DECaPS DR2 Y obs_collection = DECam Plane Survey DR2 Y band obs_description = DECaPS2 is a five-band optical and near-infrared survey of the southern Galactic plane with the Dark Energy Camera (DECam) on the 4.0m Blanco telescope at the Cerro Tololo Inter-American Observatory in Chile. The survey is designed to reach past the main-sequence turn-off at the distance of the Galactic center through a reddening E(B-V) of 1.5 mag, with a typical single-exposure depth of 23.7, 22.7, 22.2, 21.7, and 20.9 mag in the grizY bands, and with average seeing around 1''. The footprint covers | b | < 10 deg , 6 deg > l > - 124 deg (essentially the low latitude Galactic plane south of delta < - 24 deg , a total of about 2700 square degrees (6.5% of the sky). DECaPS2 simultaneously solves for the positions and fluxes of all the sources in each image, delivering positions and fluxes of 3.32 billion stars with up to 5 mmag repeatability. Most of these objects are highly reddened and deep in the Galactic disk, probing the structure and properties of the Milky Way and its interstellar medium. bib_reference = 2022arXiv220611909S bib_reference_url = https://ui.adsabs.harvard.edu/abs/2022arXiv220611909S/abstract obs_copyright = DECaM Plane Survey / NOIRLab obs_copyright_url = http://decaps.skymaps.info/ t_min = 57460 t_max = 58606 obs_regime = Optical em_min = 9.5e-7 em_max = 1.034e-6 hips_builder = Aladin/HipsGen v12.021 hips_version = 1.4 hips_release_date = 2022-12-14T06:13Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = 0 6 hips_data_range = -0.0011 -0.0011 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.277E-5 dataproduct_type = image hipsgen_date = 2022-12-13T03:56Z hipsgen_params = -f tiles hips_creation_date = 2022-12-13T03:56Z hipsgen_date_1 = 2022-12-13T11:39Z hipsgen_params_1 = png hipsgen_date_2 = 2022-12-14T04:17Z hipsgen_params_2 = -f tiles png hips_service_url = https://alasky.cds.unistra.fr/DECaPS/DR2/CDS_P_DECaPS_DR2_Y hips_service_url_1 = https://alaskybis.cds.unistra.fr/DECaPS/DR2/CDS_P_DECaPS_DR2_Y hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 188.9290792 obs_initial_dec = -63.3032221 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288493738 ID = CDS/P/DECaPS/DR2/color hips_doi = 10.26093/cds/aladin/2pq9-w4b client_category = Image/Optical/DECaPS/DR2 hips_initial_fov = 60.0 hips_initial_ra = 188.9290792 hips_initial_dec = -63.3032221 moc_sky_fraction = 0.06619 creator_did = ivo://CDS/P/DECaPS/DR2/color hips_overlay = mean hips_hierarchy = mean hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = DECaPS DR2 color obs_collection = DECam Plane Survey DR2 color (g, r, z bands) obs_description = DECaPS2 is a five-band optical and near-infrared survey of the southern Galactic plane with the Dark Energy Camera (DECam) on the 4.0m Blanco telescope at the Cerro Tololo Inter-American Observatory in Chile. The survey is designed to reach past the main-sequence turn-off at the distance of the Galactic center through a reddening E(B-V) of 1.5 mag, with a typical single-exposure depth of 23.7, 22.7, 22.2, 21.7, and 20.9 mag in the grizY bands, and with average seeing around 1''. The footprint covers | b | < 10 deg , 6 deg > l > - 124 deg (essentially the low latitude Galactic plane south of delta < - 24 deg , a total of about 2700 square degrees (6.5% of the sky). DECaPS2 simultaneously solves for the positions and fluxes of all the sources in each image, delivering positions and fluxes of 3.32 billion stars with up to 5 mmag repeatability. Most of these objects are highly reddened and deep in the Galactic disk, probing the structure and properties of the Milky Way and its interstellar medium. bib_reference = 2022arXiv220611909S bib_reference_url = https://ui.adsabs.harvard.edu/abs/2022arXiv220611909S/abstract obs_copyright = DECaM Plane Survey / NOIRLab obs_copyright_url = http://decaps.skymaps.info/ t_min = 57460 t_max = 58606 em_min = 3.805e-7 em_max = 10.150e-7 obs_regime = Optical hips_builder = Aladin/HipsGen v12.001 hips_version = 1.4 hips_release_date = 2022-11-10T09:42Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.277E-5 dataproduct_type = image hipsgen_date = 2022-11-07T22:06Z hipsgen_params = tiles hips_creation_date = 2022-11-07T22:06Z hipsgen_date_1 = 2022-11-09T19:18Z hipsgen_params_1 = region=3/457 tiles hipsgen_date_2 = 2022-11-10T07:55Z hipsgen_params_2 = mode=replacetile region=3/450 tiles hipsgen_date_3 = 2022-11-10T08:09Z hipsgen_params_3 = mode=replacetile region=3/457 tiles hipsgen_date_4 = 2022-11-10T08:29Z hipsgen_params_4 = mode=replacetile "region=3/451,3/456" tiles hipsgen_date_5 = 2022-11-10T09:07Z hipsgen_params_5 = mode=replacetile "region=3/448,3/663" tiles dataproduct_subtype = color hipsgen_date_6 = 2022-11-10T09:42Z hipsgen_params_6 = mode=replacetile "region=3/661,3/660,3/657" tiles client_application = AladinLite client_application = AladinDesktop hips_service_url = https://alasky.cds.unistra.fr/DECaPS/DR2/CDS_P_DECaPS_DR2_color hips_service_url_1 = https://alaskybis.cds.unistra.fr/DECaPS/DR2/CDS_P_DECaPS_DR2_color hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 188.9290792 obs_initial_dec = -63.3032221 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288493374 ID = CDS/P/DECaPS/DR2/g hips_doi = 10.26093/cds/aladin/2kdq-5rx client_category = Image/Optical/DECaPS/DR2 hips_initial_fov = 60.0 hips_initial_ra = 188.9290792 hips_initial_dec = -63.3032221 moc_sky_fraction = 0.06596 creator_did = ivo://CDS/P/DECaPS/DR2/g hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = mean hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = DECaPS DR2 g obs_collection = DECam Plane Survey DR2 g band obs_description = DECaPS2 is a five-band optical and near-infrared survey of the southern Galactic plane with the Dark Energy Camera (DECam) on the 4.0m Blanco telescope at the Cerro Tololo Inter-American Observatory in Chile. The survey is designed to reach past the main-sequence turn-off at the distance of the Galactic center through a reddening E(B-V) of 1.5 mag, with a typical single-exposure depth of 23.7, 22.7, 22.2, 21.7, and 20.9 mag in the grizY bands, and with average seeing around 1''. The footprint covers | b | < 10 deg , 6 deg > l > - 124 deg (essentially the low latitude Galactic plane south of delta < - 24 deg , a total of about 2700 square degrees (6.5% of the sky). DECaPS2 simultaneously solves for the positions and fluxes of all the sources in each image, delivering positions and fluxes of 3.32 billion stars with up to 5 mmag repeatability. Most of these objects are highly reddened and deep in the Galactic disk, probing the structure and properties of the Milky Way and its interstellar medium. bib_reference = 2022arXiv220611909S bib_reference_url = https://ui.adsabs.harvard.edu/abs/2022arXiv220611909S/abstract obs_copyright = DECaM Plane Survey / NOIRLab obs_copyright_url = http://decaps.skymaps.info/ t_min = 57460 t_max = 58606 em_min = 3.805e-7 em_max = 5.645e-7 obs_regime = Optical hips_builder = Aladin/HipsGen v12.021 hips_version = 1.4 hips_release_date = 2022-11-23T10:06Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = 0 0.5 hips_data_range = -0.0011 -0.0011 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.277E-5 dataproduct_type = image hipsgen_date = 2022-11-22T19:02Z hipsgen_params = tiles hips_creation_date = 2022-11-22T19:02Z hipsgen_date_1 = 2022-11-23T08:30Z hipsgen_params_1 = png hipsgen_date_2 = 2022-11-23T08:40Z hipsgen_params_2 = PNG -f hipsgen_date_3 = 2022-11-23T10:06Z hipsgen_params_3 = mode=replacetile PNG hips_service_url = https://alasky.cds.unistra.fr/DECaPS/DR2/CDS_P_DECaPS_DR2_g hips_service_url_1 = https://alaskybis.cds.unistra.fr/DECaPS/DR2/CDS_P_DECaPS_DR2_g hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 188.9290792 obs_initial_dec = -63.3032221 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288493434 ID = CDS/P/DECaPS/DR2/i hips_doi = 10.26093/cds/aladin/10p7-egt client_category = Image/Optical/DECaPS/DR2 hips_initial_fov = 60.0 hips_initial_ra = 188.9290792 hips_initial_dec = -63.3032221 moc_sky_fraction = 0.06604 creator_did = ivo://CDS/P/DECaPS/DR2/i hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = mean hips_creator = Buga M. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = DECaPS DR2 i obs_collection = DECam Plane Survey DR2 i band obs_description = DECaPS2 is a five-band optical and near-infrared survey of the southern Galactic plane with the Dark Energy Camera (DECam) on the 4.0m Blanco telescope at the Cerro Tololo Inter-American Observatory in Chile. The survey is designed to reach past the main-sequence turn-off at the distance of the Galactic center through a reddening E(B-V) of 1.5 mag, with a typical single-exposure depth of 23.7, 22.7, 22.2, 21.7, and 20.9 mag in the grizY bands, and with average seeing around 1''. The footprint covers | b | < 10 deg , 6 deg > l > - 124 deg (essentially the low latitude Galactic plane south of delta < - 24 deg , a total of about 2700 square degrees (6.5% of the sky). DECaPS2 simultaneously solves for the positions and fluxes of all the sources in each image, delivering positions and fluxes of 3.32 billion stars with up to 5 mmag repeatability. Most of these objects are highly reddened and deep in the Galactic disk, probing the structure and properties of the Milky Way and its interstellar medium. bib_reference = 2022arXiv220611909S bib_reference_url = https://ui.adsabs.harvard.edu/abs/2022arXiv220611909S/abstract obs_copyright = DECaM Plane Survey / NOIRLab obs_copyright_url = http://decaps.skymaps.info/ t_min = 57460 t_max = 58606 obs_regime = Optical em_min = 7.04e-7 em_max = 8.58e-7 hips_builder = Aladin/HipsGen v12.021 hips_version = 1.4 hips_release_date = 2022-12-03T15:51Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = 0 1.4 hips_data_range = -0.0011 -0.0011 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.277E-5 dataproduct_type = image hipsgen_date = 2022-12-01T00:35Z hipsgen_params = tiles hips_creation_date = 2022-12-01T00:35Z hipsgen_date_1 = 2022-12-01T07:03Z hipsgen_params_1 = png hipsgen_date_2 = 2022-12-01T09:31Z hipsgen_params_2 = mode=replacetile png hipsgen_date_3 = 2022-12-03T00:26Z hipsgen_params_3 = tiles hipsgen_date_4 = 2022-12-03T15:51Z hipsgen_params_4 = png hips_service_url = https://alasky.cds.unistra.fr/DECaPS/DR2/CDS_P_DECaPS_DR2_i hips_service_url_1 = https://alaskybis.cds.unistra.fr/DECaPS/DR2/CDS_P_DECaPS_DR2_i hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 188.9290792 obs_initial_dec = -63.3032221 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288493602 ID = CDS/P/DECaPS/DR2/r hips_doi = 10.26093/cds/aladin/35gc-wzp client_category = Image/Optical/DECaPS/DR2 hips_initial_fov = 60.0 hips_initial_ra = 188.9290792 hips_initial_dec = -63.3032221 moc_sky_fraction = 0.06592 creator_did = ivo://CDS/P/DECaPS/DR2/r hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = mean hips_creator = Buga M. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = DECaPS DR2 r obs_collection = DECam Plane Survey DR2 r band obs_description = DECaPS2 is a five-band optical and near-infrared survey of the southern Galactic plane with the Dark Energy Camera (DECam) on the 4.0m Blanco telescope at the Cerro Tololo Inter-American Observatory in Chile. The survey is designed to reach past the main-sequence turn-off at the distance of the Galactic center through a reddening E(B-V) of 1.5 mag, with a typical single-exposure depth of 23.7, 22.7, 22.2, 21.7, and 20.9 mag in the grizY bands, and with average seeing around 1''. The footprint covers | b | < 10 deg , 6 deg > l > - 124 deg (essentially the low latitude Galactic plane south of delta < - 24 deg , a total of about 2700 square degrees (6.5% of the sky). DECaPS2 simultaneously solves for the positions and fluxes of all the sources in each image, delivering positions and fluxes of 3.32 billion stars with up to 5 mmag repeatability. Most of these objects are highly reddened and deep in the Galactic disk, probing the structure and properties of the Milky Way and its interstellar medium. bib_reference = 2022arXiv220611909S bib_reference_url = https://ui.adsabs.harvard.edu/abs/2022arXiv220611909S/abstract obs_copyright = DECaM Plane Survey / NOIRLab obs_copyright_url = http://decaps.skymaps.info/ t_min = 57460 t_max = 58606 obs_regime = Optical em_min = 5.65e-7 em_max = 7.17e-7 hips_builder = Aladin/HipsGen v12.021 hips_version = 1.4 hips_release_date = 2022-12-01T10:05Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = 0 1.4 hips_data_range = -0.0011 -0.0011 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.277E-5 dataproduct_type = image hipsgen_date = 2022-11-30T05:49Z hipsgen_params = tiles hips_creation_date = 2022-11-30T05:49Z hipsgen_date_1 = 2022-11-30T07:37Z hipsgen_params_1 = png hipsgen_date_2 = 2022-11-30T07:43Z hipsgen_params_2 = PNG hipsgen_date_3 = 2022-11-30T07:45Z hipsgen_params_3 = PNG hipsgen_date_4 = 2022-11-30T11:16Z hipsgen_params_4 = mode=replacetile PNG hipsgen_date_5 = 2022-11-30T14:48Z hipsgen_params_5 = -f hipsgen_date_6 = 2022-12-01T10:05Z hipsgen_params_6 = mode=replacetile png hips_service_url = https://alasky.cds.unistra.fr/DECaPS/DR2/CDS_P_DECaPS_DR2_r hips_service_url_1 = https://alaskybis.cds.unistra.fr/DECaPS/DR2/CDS_P_DECaPS_DR2_r hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 188.9290792 obs_initial_dec = -63.3032221 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288493510 ID = CDS/P/DECaPS/DR2/z hips_doi = 10.26093/cds/aladin/32xv-yy4 client_category = Image/Optical/DECaPS/DR2 hips_initial_fov = 60.0 hips_initial_ra = 188.9290792 hips_initial_dec = -63.3032221 moc_sky_fraction = 0.06589 creator_did = ivo://CDS/P/DECaPS/DR2/z hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = mean hips_creator = Buga M. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = DECaPS DR2 z obs_collection = DECam Plane Survey DR2 z band obs_description = DECaPS2 is a five-band optical and near-infrared survey of the southern Galactic plane with the Dark Energy Camera (DECam) on the 4.0m Blanco telescope at the Cerro Tololo Inter-American Observatory in Chile. The survey is designed to reach past the main-sequence turn-off at the distance of the Galactic center through a reddening E(B-V) of 1.5 mag, with a typical single-exposure depth of 23.7, 22.7, 22.2, 21.7, and 20.9 mag in the grizY bands, and with average seeing around 1''. The footprint covers | b | < 10 deg , 6 deg > l > - 124 deg (essentially the low latitude Galactic plane south of delta < - 24 deg , a total of about 2700 square degrees (6.5% of the sky). DECaPS2 simultaneously solves for the positions and fluxes of all the sources in each image, delivering positions and fluxes of 3.32 billion stars with up to 5 mmag repeatability. Most of these objects are highly reddened and deep in the Galactic disk, probing the structure and properties of the Milky Way and its interstellar medium. bib_reference = 2022arXiv220611909S bib_reference_url = https://ui.adsabs.harvard.edu/abs/2022arXiv220611909S/abstract obs_copyright = DECaM Plane Survey / NOIRLab obs_copyright_url = http://decaps.skymaps.info/ t_min = 57460 t_max = 58606 obs_regime = Optical em_min = 8.46e-7 em_max = 1e-6 hips_builder = Aladin/HipsGen v12.021 hips_version = 1.4 hips_release_date = 2022-12-03T15:52Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = 0 1.4 hips_data_range = -0.0011 -0.0011 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.277E-5 dataproduct_type = image hipsgen_date = 2022-12-03T06:55Z hipsgen_params = -f tiles hips_creation_date = 2022-12-03T06:55Z hipsgen_date_1 = 2022-12-03T15:52Z hipsgen_params_1 = png hips_service_url = https://alasky.cds.unistra.fr/DECaPS/DR2/CDS_P_DECaPS_DR2_z hips_service_url_1 = https://alaskybis.cds.unistra.fr/DECaPS/DR2/CDS_P_DECaPS_DR2_z hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 188.9290792 obs_initial_dec = -63.3032221 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288493666 ID = CDS/P/DENIS/I creator_did = ivo://CDS/P/DENIS/I hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = DENIS I obs_collection = DENIS obs_description = DENIS is a project to survey the all-southern sky simultaneously in three wavelength bands (Gunn-i 0.82 µm; J, 1.25 µm; and Ks, 2.15 µm) with limiting magnitudes 18.5, 16.5 and 14.0, respectively. The observations are performed with the 1m-ESO telescope at La Silla (Chile). The DENIS instrument is made up of a 3-channel camera built of commercially available detector arrays by the Observatoire de Paris and with major contributions from other European Institutes, notably: the IAS in Frascati, the Observatoire de Grenoble, the University of Innsbruck, the Observatoire de Lyon, and the IAC in Tenerife. The survey is carried out by observing strips of 30° in declination and 12 arcminutes in Right Ascension with an overlap of 2 arcminutes between consecutive strips. The observations started at the end of 1995 and have been completed on Sept. 9, 2001. The data are reduced in two consecutive steps, the image processing and source extraction, which are performed at the Institut d'Astrophysique de Paris. The position of a general extracted point source is provided with an accuracy better than 1 arcsec and its magnitude to better than 0.1 mag. obs_ack = The DENIS project has been partly funded by the SCIENCE and the HCM plans of the European Commission under grants CT920791 and CT940627. It is supported by INSU, MEN and CNRS in France, by the State of Baden-Württemberg in Germany, by DGICYT in Spain, by CNR in Italy, by FFwFBWF in Austria, by FAPESP in Brazil, by OTKA grants F-4239 and F-013990 in Hungary, and by the ESO C&EE grant A-04-046. prov_progenitor = Observatoire Paris Meudon bib_reference = 1997Msngr..87...27E bib_reference_url = https://ui.adsabs.harvard.edu/abs/1997Msngr..87...27E/abstract obs_copyright = © DENIS Consortium - INSU/CNRS t_min = 50040.0 t_max = 52138.0 obs_regime = Infrared em_min = 7.00728e-7 em_max = 9.14e-7 client_category = Image/Infrared/DENIS hips_builder = Aladin/HipsGen v12.135 hips_version = 1.4 hips_release_date = 2024-08-28T09:11Z hips_frame = equatorial hips_order = 9 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_bitpix = -32 hips_pixel_cut = -12.49 293.5 hips_initial_ra = 181.818133 hips_initial_dec = -62.7025304 hips_initial_fov = 220.0 hips_pixel_scale = 0.229 s_pixel_scale = 2.783E-4 dataproduct_type = image moc_sky_fraction = 0.5085 hipsgen_date = 2024-07-31T14:40Z hips_creation_date = 2024-07-31T14:40Z hipsgen_date_1 = 2024-08-01T10:52Z data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwrite treeMean hips_data_range = -5036 14990 hips_data_minmax = -17435 162828 hips_service_url = https://alasky.cds.unistra.fr/DENIS/CDS_P_DENIS_I hips_progenitor_url = https://alasky.cds.unistra.fr/DENIS/CDS_P_DENIS_I/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/DENIS/CDS_P_DENIS_I hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 9 obs_initial_ra = 181.818133 obs_initial_dec = -62.7025304 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1726214834817 ID = CDS/P/DES-DR1/ColorIRG hips_doi = 10.26093/cds/aladin/3dv3-t03 hips_initial_fov = 0.5 hips_initial_ra = 53.4019083 hips_initial_dec = -36.1406582 creator_did = ivo://CDS/P/DES-DR1/ColorIRG hips_creator = Fernique P. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = DES-DR1 color (I-R-G bands) obs_description = The Dark Energy Survey (DES) is a 5000 square degree grizY survey of the Southern sky aimed at understanding the accelerating expansion rate of the Universe. DES is using four complementary methods to do this: weak gravitational lensing, galaxy cluster counts, baryon acoustic oscillations, and Type Ia supernovae. DES uses the 3 square degree Dark Energy Camera (DECam), a 570 Megapixel CCD imaging camera installed at the prime focus of on the Blanco 4m telescope at the Cerro Tololo Interamerican Observatory in northern Chile. The survey is being performed over a period of five years (2013-2018), and is recording information from roughly 300 million distant galaxies and 100 million Milky Way stars. The DES-DR1 colored HiPS has been generated from I, R and G HiPS based on Lupton simplified algorithm by CDS. obs_ack = The NOAO Data Lab is operated by the National Optical Astronomy Observatory, the national center for ground-based nighttime astronomy in the United States operated by the Association of Universities for Research in Astronomy (AURA) under cooperative agreement with the National Science Foundation - The University of Strasbourg and the French CNRS. prov_progenitor = HiPS I, HiPS R and HiPS G bib_reference = 2018ApJS..239...18A bib_reference_url = https://ui.adsabs.harvard.edu/abs/2018ApJS..239...18A/abstract client_category = Image/Optical/DES t_min = 56519 t_max = 57430 obs_regime = Optical em_min = 3.939e-7 em_max = 8.646e-7 hips_builder = Aladin/HipsGen v11.008 hips_version = 1.4 hips_release_date = 2020-02-01T16:15Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master unclonable hips_pixel_scale = 5.591E-5 dataproduct_type = image dataproduct_subtype = color hips_rgb_red = DES-DR1 i [lupton min=-0.01 scale=0.012 Q=30.0] hips_rgb_green = DES-DR1 r [lupton min=-0.01 scale=0.017 Q=30.0] hips_rgb_blue = DES-DR1 g [lupton min=-0.01 scale=0.025 Q=30.0] moc_sky_fraction = 0.1274 hips_estsize = 229803620 hips_creation_date = 2020-01-20T15:32Z hips_hierarchy = mean hips_tile_format = png hipsgen_date = 2020-01-23T07:28Z hipsgen_params = inRed=CDS_P_DES-DR1_i inGreen=CDS_P_DES-DR1_r inBlue=CDS_P_DES-DR1_g color=png filter=gauss luptonM=-0.01 luptonS=0.012/0.017/0.025 luptonQ=30.0 creator_did=cds/P/DES-DR1/ColorIRG out=CDS_P_DES-DR1_ColorIRG -maxthread=10 method=mean -f RGB hips_service_url = https://alasky.cds.unistra.fr/DES/CDS_P_DES-DR1_ColorIRG hips_service_url_1 = https://alaskybis.cds.unistra.fr/DES/CDS_P_DES-DR1_ColorIRG hips_status_1 = public mirror unclonable moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 53.4019083 obs_initial_dec = -36.1406582 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288484658 ID = CDS/P/DES-DR1/Y hips_doi = 10.26093/cds/aladin/3q39-v1w hips_initial_fov = 0.5 hips_initial_ra = 53.4019083 hips_initial_dec = -36.1406582 creator_did = ivo://CDS/P/DES-DR1/Y hips_pixel_bitpix = 16 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = mean hips_creator = Buga M. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = DES-DR1 Y obs_collection = DES-DR1 Y obs_description = The Dark Energy Survey (DES) is a 5000 square degree grizY survey of the Southern sky aimed at understanding the accelerating expansion rate of the Universe. DES is using four complementary methods to do this: weak gravitational lensing, galaxy cluster counts, baryon acoustic oscillations, and Type Ia supernovae. DES uses the 3 square degree Dark Energy Camera (DECam), a 570 Megapixel CCD imaging camera installed at the prime focus of on the Blanco 4m telescope at the Cerro Tololo Interamerican Observatory in northern Chile. The survey is being performed over a period of five years (2013-2018), and is recording information from roughly 300 million distant galaxies and 100 million Milky Way stars. obs_ack = The NOAO Data Lab is operated by the National Optical Astronomy Observatory, the national center for ground-based nighttime astronomy in the United States operated by the Association of Universities for Research in Astronomy (AURA) under cooperative agreement with the National Science Foundation. prov_progenitor = NOAO Data Lab bib_reference = 2018ApJS..239...18A bib_reference_url = https://ui.adsabs.harvard.edu/abs/2018ApJS..239...18A/abstract client_category = Deprecated/HiPS/CDS/Optical/DES t_min = 56519 t_max = 57430 obs_regime = Optical em_min = 9.4e-7 em_max = 1.0805e-6 hips_builder = Aladin/HipsGen v10.130 hips_version = 1.4 hips_release_date = 2019-07-05T16:10Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_cut = -1 400 hips_data_range = -1000 16000 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.305E-5 dataproduct_type = image moc_sky_fraction = 0.127 hips_estsize = 4793892484 hipsgen_date = 2019-07-04T23:53Z hipsgen_params = maxthread=30 in=images_Y/ out=hips_Y/ "-hips_pixel_cut=-1 400 Asinh" "hips_data_range=-1000 16000" hips_pixel_bitpix=16 creator_did=CDS/P/DES-DR1/Y partitioning=5000 -method=MEAN blank=0 "fitskeys=MJD-OBS TILENAME TILEID EXPTIME" TILES JPEG DETAILS hips_creation_date = 2019-07-04T23:53Z hipsgen_date_1 = 2019-07-05T16:10Z hipsgen_params_1 = maxthread=30 in=images_Y/ out=hips_Y/ "-hips_pixel_cut=-1 400 Asinh" "hips_data_range=-1000 16000" hips_pixel_bitpix=16 creator_did=CDS/P/DES-DR1/Y partitioning=5000 -method=MEAN blank=0 "fitskeys=MJD-OBS TILENAME TILEID EXPTIME" TILES JPEG DETAILS hips_service_url = https://alasky.cds.unistra.fr/DES/CDS_P_DES-DR1_Y hips_progenitor_url = https://alasky.cds.unistra.fr/DES/CDS_P_DES-DR1_Y/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/DES/CDS_P_DES-DR1_Y hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 53.4019083 obs_initial_dec = -36.1406582 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288484598 ID = CDS/P/DES-DR1/g hips_doi = 10.26093/cds/aladin/qnbw-cq hips_initial_fov = 0.5 hips_initial_ra = 53.4019083 hips_initial_dec = -36.1406582 creator_did = ivo://CDS/P/DES-DR1/g hips_pixel_bitpix = 16 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = mean hips_creator = Fernique P. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = DES-DR1 g obs_collection = DES DR1 obs_description = The dard Energy Survey (DES) is a 5000 square degree grizY survey of the Southern sky aimed understanding the accelerating explansion rate of the universe. DES is using four complementary methods to do this: weak gravitational lensing, galaxy cluster counts, baryon acoustic oscillations, and Type Ia supernovae. DES uses the 3 square degree Dark Energy Camera (DECam), a 570 Megapixel CCD imaging camera installed at the prime focus of on the Blanco 4m telescope at the Cerro Tololo Interamerican Observatory in northern Chile. The survey is being performed over a period of five years (2013-2018), and is recording information from roughly 300 million distant galaxies and 100 million Milky Way stars. obs_ack = The NOAO Data Lab is operated by the National Optical Astrnomy Observatory, the national center for ground-based nighttime astronomy in the United States operated by the Association of Universities for Research in Astronomy (AURA) under cooperative agreement with the National Science Foundation prov_progenitor = NOAO Data Lab bib_reference = 2018ApJS..239...18A bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2018ApJS..239...18A client_category = Deprecated/HiPS/CDS/Optical/DES t_min = 56519 t_max = 57430 obs_regime = Optical em_min = 3.939e-7 em_max = 5.528e-7 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-23T13:18Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_cut = -1 400 hips_pixel_function = asinh hips_data_range = -1000 16000 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.305E-5 dataproduct_type = image moc_sky_fraction = 0.1284 hipsgen_date = 2019-03-05T13:24Z hipsgen_params = maxthread=50 in=/data4/Pierre/DES/g out=/data3/Pierre/CDS_P_DES-DR1_g "-hips_pixel_cut=-1 400 Asinh" "hips_data_range=-1000 16000" hips_pixel_bitpix=16 creator_did=CDS/P/DES-DR1/g partitioning=5000 -method=MEAN -f pilot=100 blank=0 "fitskeys=MJD-OBS TILENAME TILEID EXPTIME" INDEX TILES DETAILS -color hips_creation_date = 2019-03-05T13:24Z hipsgen_date_1 = 2019-03-05T18:14Z hipsgen_params_1 = maxthread=50 in=/data4/Pierre/DES/g out=/data3/Pierre/CDS_P_DES-DR1_g "-hips_pixel_cut=-1 400 Asinh" "hips_data_range=-1000 16000" hips_pixel_bitpix=16 creator_did=CDS/P/DES-DR1/g partitioning=5000 -method=MEAN -f pilot=100 blank=0 "fitskeys=MJD-OBS TILENAME TILEID EXPTIME" INDEX TILES DETAILS hipsgen_date_2 = 2019-03-06T03:56Z hipsgen_params_2 = maxthread=50 in=/data4/Pierre/DES/g out=/data3/Pierre/CDS_P_DES-DR1_g "-hips_pixel_cut=-1 400 Asinh" "hips_data_range=-1000 16000" hips_pixel_bitpix=16 creator_did=CDS/P/DES-DR1/g partitioning=5000 -method=MEAN -f blank=0 "fitskeys=MJD-OBS TILENAME TILEID EXPTIME" INDEX TILES DETAILS hipsgen_date_3 = 2019-03-06T22:01Z hipsgen_params_3 = maxthread=50 in=/data4/Pierre/DES/g out=/data3/Pierre/CDS_P_DES-DR1_g "-hips_pixel_cut=-1 400 Asinh" "hips_data_range=-1000 16000" hips_pixel_bitpix=16 creator_did=CDS/P/DES-DR1/g partitioning=5000 -method=MEAN blank=0 "fitskeys=MJD-OBS TILENAME TILEID EXPTIME" JPEG hips_estsize = 4794283561 hipsgen_date_4 = 2019-05-23T13:18Z hipsgen_params_4 = out=/asd-volumes/sc1-asd-volume5/DES/CDS_P_DES-DR1_g UPDATE hips_service_url = https://alasky.cds.unistra.fr/DES/CDS_P_DES-DR1_g hips_progenitor_url = https://alasky.cds.unistra.fr/DES/CDS_P_DES-DR1_g/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/DES/CDS_P_DES-DR1_g hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 20 moc_time_range = 63 moc_order = 10 obs_initial_ra = 53.4019083 obs_initial_dec = -36.1406582 obs_initial_fov = 0.057258106863623426 TIMESTAMP = 1721288484370 ID = CDS/P/DES-DR1/i hips_doi = 10.26093/cds/aladin/34ev-q4g hips_initial_fov = 0.5 hips_initial_ra = 53.4019083 hips_initial_dec = -36.1406582 creator_did = ivo://CDS/P/DES-DR1/i hips_pixel_bitpix = 16 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = mean hips_creator = Buga M. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = DES-DR1 i obs_collection = DES-DR1 i obs_description = The Dark Energy Survey (DES) is a 5000 square degree grizY survey of the Southern sky aimed at understanding the accelerating expansion rate of the Universe. DES is using four complementary methods to do this: weak gravitational lensing, galaxy cluster counts, baryon acoustic oscillations, and Type Ia supernovae. DES uses the 3 square degree Dark Energy Camera (DECam), a 570 Megapixel CCD imaging camera installed at the prime focus of on the Blanco 4m telescope at the Cerro Tololo Interamerican Observatory in northern Chile. The survey is being performed over a period of five years (2013-2018), and is recording information from roughly 300 million distant galaxies and 100 million Milky Way stars. obs_ack = The NOAO Data Lab is operated by the National Optical Astronomy Observatory, the national center for ground-based nighttime astronomy in the United States operated by the Association of Universities for Research in Astronomy (AURA) under cooperative agreement with the National Science Foundation. prov_progenitor = NOAO Data Lab bib_reference = 2018ApJS..239...18A bib_reference_url = https://ui.adsabs.harvard.edu/abs/2018ApJS..239...18A/abstract client_category = Deprecated/HiPS/CDS/Optical/DES t_min = 56519 t_max = 57430 obs_regime = Optical em_min = 6.950e-7 em_max = 8.646e-7 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-23T13:27Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_cut = -1 400 hips_data_range = -1000 16000 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.305E-5 dataproduct_type = image moc_sky_fraction = 0.127 hips_estsize = 4794283561 hipsgen_date = 2019-05-07T14:35Z hipsgen_params = maxthread=50 in=/data3/buga/DES/images_fits_image_r_mais_i/ out=HiPS_DES_i/ "-hips_pixel_cut=-1 400 Asinh" "hips_data_range=-1000 16000" hips_pixel_bitpix=16 creator_did=CDS/P/DES-DR1/i partitioning=5000 -method=MEAN blank=0 "fitskeys=MJD-OBS TILENAME TILEID EXPTIME" TILES JPEG DETAILS hips_creation_date = 2019-05-07T14:35Z hipsgen_date_1 = 2019-05-08T05:10Z hipsgen_params_1 = maxthread=50 in=/data3/buga/DES/images_fits_image_r_mais_i/ out=HiPS_DES_i/ "-hips_pixel_cut=-1 400 Asinh" "hips_data_range=-1000 16000" hips_pixel_bitpix=16 creator_did=CDS/P/DES-DR1/i partitioning=5000 -method=MEAN blank=0 "fitskeys=MJD-OBS TILENAME TILEID EXPTIME" TILES JPEG DETAILS hipsgen_date_2 = 2019-05-23T13:27Z hipsgen_params_2 = out=/volume5/DES/CDS_P_DES-DR1_i UPDATE hips_service_url = https://alasky.cds.unistra.fr/DES/CDS_P_DES-DR1_i hips_progenitor_url = https://alasky.cds.unistra.fr/DES/CDS_P_DES-DR1_i/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/DES/CDS_P_DES-DR1_i hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 53.4019083 obs_initial_dec = -36.1406582 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288484478 ID = CDS/P/DES-DR1/r hips_doi = 10.26093/cds/aladin/118g-5bw hips_initial_fov = 0.5 hips_initial_ra = 53.4019083 hips_initial_dec = -36.1406582 creator_did = ivo://CDS/P/DES-DR1/r hips_pixel_bitpix = 16 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = mean hips_creator = Buga M. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = DES-DR1 r obs_collection = DES-DR1 r obs_description = The Dark Energy Survey (DES) is a 5000 square degree grizY survey of the Southern sky aimed at understanding the accelerating expansion rate of the Universe. DES is using four complementary methods to do this: weak gravitational lensing, galaxy cluster counts, baryon acoustic oscillations, and Type Ia supernovae. DES uses the 3 square degree Dark Energy Camera (DECam), a 570 Megapixel CCD imaging camera installed at the prime focus of on the Blanco 4m telescope at the Cerro Tololo Interamerican Observatory in northern Chile. The survey is being performed over a period of five years (2013-2018), and is recording information from roughly 300 million distant galaxies and 100 million Milky Way stars. obs_ack = The NOAO Data Lab is operated by the National Optical Astronomy Observatory, the national center for ground-based nighttime astronomy in the United States operated by the Association of Universities for Research in Astronomy (AURA) under cooperative agreement with the National Science Foundation. prov_progenitor = NOAO Data Lab bib_reference = 2018ApJS..239...18A bib_reference_url = https://ui.adsabs.harvard.edu/abs/2018ApJS..239...18A/abstract client_category = Deprecated/HiPS/CDS/Optical/DES t_min = 56519 t_max = 57430 obs_regime = Optical em_min = 5.506e-7 em_max = 7.238e-7 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-06-04T12:40Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_cut = -1 400 hips_data_range = -1000 16000 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.305E-5 dataproduct_type = image moc_sky_fraction = 0.127 hips_estsize = 4793510329 hipsgen_date = 2019-04-19T17:58Z hipsgen_params = maxthread=50 in=/data4/buga/DES/images_i/ out=CDS_P_DES-DR1_r/ "-hips_pixel_cut=-1 400 Asinh" "hips_data_range=-1000 16000" hips_pixel_bitpix=16 creator_did=CDS/P/DES-DR1/r partitioning=5000 -method=MEAN blank=0 "fitskeys=MJD-OBS TILENAME TILEID EXPTIME" TILES JPEG DETAILS hips_creation_date = 2019-04-19T17:58Z hipsgen_date_1 = 2019-04-20T10:27Z hipsgen_params_1 = maxthread=50 in=/data4/buga/DES/images_i/ out=CDS_P_DES-DR1_r/ "-hips_pixel_cut=-1 400 Asinh" "hips_data_range=-1000 16000" hips_pixel_bitpix=16 creator_did=CDS/P/DES-DR1/r partitioning=5000 -method=MEAN blank=0 "fitskeys=MJD-OBS TILENAME TILEID EXPTIME" TILES JPEG DETAILS hipsgen_date_2 = 2019-06-04T12:40Z hipsgen_params_2 = out=CDS_P_DES-DR1_r UPDATE hips_service_url = https://alasky.cds.unistra.fr/DES/CDS_P_DES-DR1_r hips_progenitor_url = https://alasky.cds.unistra.fr/DES/CDS_P_DES-DR1_r/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/DES/CDS_P_DES-DR1_r hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 53.4019083 obs_initial_dec = -36.1406582 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288484426 ID = CDS/P/DES-DR1/z hips_doi = 10.26093/cds/aladin/1657-7ae hips_initial_fov = 0.5 hips_initial_ra = 53.4019083 hips_initial_dec = -36.1406582 creator_did = ivo://CDS/P/DES-DR1/z hips_pixel_bitpix = 16 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = mean hips_creator = Buga M. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = DES-DR1 z obs_collection = DES-DR1 z obs_description = The Dark Energy Survey (DES) is a 5000 square degree grizY survey of the Southern sky aimed at understanding the accelerating expansion rate of the Universe. DES is using four complementary methods to do this: weak gravitational lensing, galaxy cluster counts, baryon acoustic oscillations, and Type Ia supernovae. DES uses the 3 square degree Dark Energy Camera (DECam), a 570 Megapixel CCD imaging camera installed at the prime focus of on the Blanco 4m telescope at the Cerro Tololo Interamerican Observatory in northern Chile. The survey is being performed over a period of five years (2013-2018), and is recording information from roughly 300 million distant galaxies and 100 million Milky Way stars. obs_ack = The NOAO Data Lab is operated by the National Optical Astronomy Observatory, the national center for ground-based nighttime astronomy in the United States operated by the Association of Universities for Research in Astronomy (AURA) under cooperative agreement with the National Science Foundation. prov_progenitor = NOAO Data Lab bib_reference = 2018ApJS..239...18A bib_reference_url = https://ui.adsabs.harvard.edu/abs/2018ApJS..239...18A/abstract client_category = Deprecated/HiPS/CDS/Optical/DES t_min = 56519 t_max = 57430 obs_regime = Optical em_min = 8.284e-7 em_max = 1.0102e-6 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-06-11T13:41Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_cut = -1 400 hips_data_range = -1000 16000 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.305E-5 dataproduct_type = image moc_sky_fraction = 0.1271 hips_estsize = 4794283561 hipsgen_date = 2019-05-30T01:48Z hipsgen_params = maxthread=40 in=images_z/ out=hips_z/ "-hips_pixel_cut=-1 400 Asinh" "hips_data_range=-1000 16000" hips_pixel_bitpix=16 creator_did=CDS/P/DES-DR1/i partitioning=5000 -method=MEAN blank=0 "fitskeys=MJD-OBS TILENAME TILEID EXPTIME" -f INDEX TILES JPEG DETAILS hips_creation_date = 2019-05-30T01:48Z hipsgen_date_1 = 2019-05-30T01:55Z hipsgen_params_1 = maxthread=40 in=images_z/ out=hips_z/ "-hips_pixel_cut=-1 400 Asinh" "hips_data_range=-1000 16000" hips_pixel_bitpix=16 creator_did=CDS/P/DES-DR1/i partitioning=5000 -method=MEAN blank=0 "fitskeys=MJD-OBS TILENAME TILEID EXPTIME" -f INDEX TILES JPEG DETAILS hipsgen_date_2 = 2019-05-30T17:35Z hipsgen_params_2 = maxthread=40 in=images_z/ out=hips_z/ "-hips_pixel_cut=-1 400 Asinh" "hips_data_range=-1000 16000" hips_pixel_bitpix=16 creator_did=CDS/P/DES-DR1/i partitioning=5000 -method=MEAN blank=0 "fitskeys=MJD-OBS TILENAME TILEID EXPTIME" -f INDEX TILES JPEG DETAILS hipsgen_date_3 = 2019-06-11T13:41Z hipsgen_params_3 = out=CDS_P_DES-DR1_z UPDATE hips_service_url = https://alasky.cds.unistra.fr/DES/CDS_P_DES-DR1_z hips_progenitor_url = https://alasky.cds.unistra.fr/DES/CDS_P_DES-DR1_z/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/DES/CDS_P_DES-DR1_z hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 53.4019083 obs_initial_dec = -36.1406582 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288484530 ID = CDS/P/DES-DR2/ColorIRG hips_doi = 10.26093/cds/aladin/r8cm-r0 hips_initial_fov = 0.3 hips_initial_ra = 31.5154083 hips_initial_dec = -27.4936367 moc_sky_fraction = 0.1261 creator_did = ivo://CDS/P/DES-DR2/ColorIRG hips_creator = Boch T. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = DES-DR2 ColorIRG obs_collection = DES-DR2 ColorIRG obs_description = The second public data release of the Dark Energy Survey, DES DR2, based on optical/near-infrared imaging by the Dark Energy Camera mounted on the 4 m Blanco telescope at Cerro Tololo Inter-American Observatory in Chile. DES DR2 includes ~691 million distinct astronomical objects detected in 10,169 coadded image tiles of size 0.534 deg2 produced from 76,217 single epoch images. obs_ack = https://www.darkenergysurvey.org/the-des-project/data-access/ prov_progenitor = https://desdr-server.ncsa.illinois.edu/ bib_reference = 2021ApJS..255...20A bib_reference_url = https://ui.adsabs.harvard.edu/abs/2021ApJS..255...20A/abstract obs_copyright = DECaM Plane Survey / NOAO obs_copyright_url = http://decaps.skymaps.info/ client_category = Image/Optical/DES t_min = 56519 t_max = 58492 obs_regime = Optical em_min = 3.939e-7 em_max = 8.646e-7 hips_builder = Aladin/HipsGen v12.033 hips_version = 1.4 hips_release_date = 2023-02-22T01:30Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_tile_format = png hips_status = public master clonableOnce hips_pixel_scale = 5.591E-5 dataproduct_type = image hips_rgb_red = DES-DR2 i [lupton min=0.02 scale=0.005 Q=30.0] hips_rgb_green = DES-DR2 r [lupton min=0.02 scale=0.005 Q=30.0] hips_rgb_blue = DES-DR2 g [lupton min=0.02 scale=0.007 Q=30.0] hipsgen_date = 2023-02-15T10:28Z hipsgen_params = inRed=../CDS_P_DES-DR2_i inGreen=../CDS_P_DES-DR2_r inBlue=../CDS_P_DES-DR2_g color=png luptonM=0.02 luptonS=0.005/0.005/0.007 luptonQ=30.0 id=cds/P/DES-DR2/ColorIRG out=./CDS_P_DES-DR2_ColorIRG -maxthread=12 RGB hips_creation_date = 2023-02-15T10:28Z hipsgen_date_1 = 2023-02-15T14:00Z hipsgen_params_1 = inRed=../CDS_P_DES-DR2_i inGreen=../CDS_P_DES-DR2_r inBlue=../CDS_P_DES-DR2_g color=png luptonM=0.02 luptonS=0.005/0.005/0.007 luptonQ=30.0 id=cds/P/DES-DR2/ColorIRG out=./CDS_P_DES-DR2_ColorIRG -maxthread=12 tree hips_overlay = overlayMean mergeOverwriteTile treeMedian dataproduct_subtype = color hips_service_url = https://alasky.cds.unistra.fr/DES/DR2/CDS_P_DES-DR2_ColorIRG hips_service_url_1 = https://alaskybis.cds.unistra.fr/DES/DR2/CDS_P_DES-DR2_ColorIRG hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 31.5154083 obs_initial_dec = -27.4936367 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288494130 ID = CDS/P/DES-DR2/Y hips_doi = 10.26093/cds/aladin/3p74-mk5 creator_did = ivo://CDS/P/DES-DR2/Y hips_creator = Buga M. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = DES-DR2 Y obs_collection = DES-DR2 Y obs_description = The second public data release of the Dark Energy Survey, DES DR2, based on optical/near-infrared imaging by the Dark Energy Camera mounted on the 4 m Blanco telescope at Cerro Tololo Inter-American Observatory in Chile. DES DR2 includes ~691 million distinct astronomical objects detected in 10,169 coadded image tiles of size 0.534 deg2 produced from 76,217 single epoch images. obs_ack = https://www.darkenergysurvey.org/the-des-project/data-access/ prov_progenitor = https://desdr-server.ncsa.illinois.edu/ bib_reference = 2021ApJS..255...20A bib_reference_url = https://ui.adsabs.harvard.edu/abs/2021ApJS..255...20A/abstract obs_copyright = DECaM Plane Survey / NOAO obs_copyright_url = http://decaps.skymaps.info/ client_category = Image/Optical/DES t_min = 56519 t_max = 58492 obs_regime = Optical em_min = 9.4e-7 em_max = 1.0805e-6 hips_builder = Aladin/HipsGen v12.033 hips_version = 1.4 hips_release_date = 2023-02-13T17:14Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_pixel_cut = -1.2 400 hips_data_range = -64669 193357 hips_initial_fov = 0.3 hips_initial_ra = 31.5154083 hips_initial_dec = -27.4936367 moc_sky_fraction = 0.1261 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.305E-5 dataproduct_type = image hipsgen_date = 2023-02-01T10:35Z hipsgen_params = cache=./tmp in=../boch/DES-DR2/data/Y/ out=HiPS_Y/ id=CDS/P/DES-DR2/Y partitioning=false TILES hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeKeepTile treeMean hips_creation_date = 2023-02-01T10:35Z hips_tile_format = png fits hipsgen_date_1 = 2023-02-10T18:04Z hipsgen_params_1 = cache=./tmp in=../boch/DES-DR2/data/Y/ out=/data3/buga/DES/DES_DR2/HiPS_Y/ id=CDS/P/DES-DR2/Y partitioning=false mode=keeptile TILES hipsgen_date_2 = 2023-02-13T17:14Z hipsgen_params_2 = cache=./tmp in=../boch/DES-DR2/data/Y/ out=/data3/buga/DES/DES_DR2/HiPS_Y/ id=CDS/P/DES-DR2/Y partitioning=false "pixelCut=-1.2 400 asinh" mode=mean PNG hips_service_url = https://alasky.cds.unistra.fr/DES/DR2/CDS_P_DES-DR2_Y hips_progenitor_url = https://alasky.cds.unistra.fr/DES/DR2/CDS_P_DES-DR2_Y/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/DES/DR2/CDS_P_DES-DR2_Y hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 31.5154083 obs_initial_dec = -27.4936367 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288494046 ID = CDS/P/DES-DR2/g hips_doi = 10.26093/cds/aladin/ph6k-ye hips_initial_fov = 0.3 hips_initial_ra = 31.5154083 hips_initial_dec = -27.4936367 creator_did = ivo://CDS/P/DES-DR2/g hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = median hips_creator = Boch T. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = DES-DR2 g obs_collection = DES-DR2 g obs_description = The second public data release of the Dark Energy Survey, DES DR2, is based on optical/near-infrared imaging by the Dark Energy Camera mounted on the 4 m Blanco telescope at Cerro Tololo Inter-American Observatory in Chile. DES DR2 includes ~691 million distinct astronomical objects detected in 10,169 coadded image tiles of size 0.534 deg2 produced from 76,217 single epoch images. obs_ack = https://www.darkenergysurvey.org/the-des-project/data-access/ prov_progenitor = https://desdr-server.ncsa.illinois.edu/ bib_reference = 2021ApJS..255...20A bib_reference_url = https://ui.adsabs.harvard.edu/abs/2021ApJS..255...20A/abstract obs_copyright = DECaM Plane Survey / NOAO obs_copyright_url = http://decaps.skymaps.info/ client_category = Image/Optical/DES t_min = 56519 t_max = 58492 obs_regime = Optical em_min = 3.805e-7 em_max = 5.645e-7 hips_builder = Aladin/HipsGen v12.001 hips_version = 1.4 hips_release_date = 2022-12-25T04:30Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = -1.2 400 hips_data_range = -7446 22297 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.305E-5 dataproduct_type = image hipsgen_date = 2022-12-21T11:39Z hipsgen_params = cache=./tmp in=data/g out=hips/ creator_did=CDS/P/DES-DR2/g partitioning=false TILES hips_creation_date = 2022-12-21T11:39Z hipsgen_date_1 = 2022-12-22T08:44Z hipsgen_params_1 = cache=./tmp in=data/g out=hips/ creator_did=CDS/P/DES-DR2/g partitioning=false "hips_pixel_cut=-1.2 400 asinh" method=mean PNG -f hips_service_url = https://alasky.cds.unistra.fr/DES/DR2/CDS_P_DES-DR2_g hips_progenitor_url = https://alasky.cds.unistra.fr/DES/DR2/CDS_P_DES-DR2_g/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/DES/DR2/CDS_P_DES-DR2_g hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 0.1261 moc_order = 11 obs_initial_ra = 31.5154083 obs_initial_dec = -27.4936367 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288493814 ID = CDS/P/DES-DR2/i hips_doi = 10.26093/cds/aladin/35ap-rp9 creator_did = ivo://CDS/P/DES-DR2/i hips_creator = Buga M. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = DES-DR2 i obs_collection = DES-DR2 i obs_description = The second public data release of the Dark Energy Survey, DES DR2, based on optical/near-infrared imaging by the Dark Energy Camera mounted on the 4 m Blanco telescope at Cerro Tololo Inter-American Observatory in Chile. DES DR2 includes ~691 million distinct astronomical objects detected in 10,169 coadded image tiles of size 0.534 deg2 produced from 76,217 single epoch images. obs_ack = https://www.darkenergysurvey.org/the-des-project/data-access/ prov_progenitor = https://desdr-server.ncsa.illinois.edu/ bib_reference = 2021ApJS..255...20A bib_reference_url = https://ui.adsabs.harvard.edu/abs/2021ApJS..255...20A/abstract obs_copyright = DECaM Plane Survey / NOAO obs_copyright_url = http://decaps.skymaps.info/ client_category = Image/Optical/DES t_min = 56519 t_max = 58492 obs_regime = Optical em_min = 6.950e-7 em_max = 8.646e-7 hips_builder = Aladin/HipsGen v12.033 hips_version = 1.4 hips_release_date = 2023-02-05T15:28Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_pixel_cut = -1 400 hips_data_range = -5370 16013 hips_initial_fov = 0.3 hips_initial_ra = 31.5154083 hips_initial_dec = -27.4936367 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.305E-5 dataproduct_type = image hipsgen_date = 2023-01-31T15:38Z hipsgen_params = cache=./tmp in=../boch/DES-DR2/data/i out=HiPS_i/ id=CDS/P/DES-DR2/i partitioning=false TILES hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeKeepTile treeMean hips_creation_date = 2023-01-31T15:38Z hips_tile_format = png fits hipsgen_date_1 = 2023-02-02T03:30Z hipsgen_params_1 = cache=./tmp in=../boch/DES-DR2/data/i out=HiPS_i/ id=CDS/P/DES-DR2/i partitioning=false mode=keeptile TILES hipsgen_date_2 = 2023-02-05T15:28Z hipsgen_params_2 = cache=./tmp in=../boch/DES-DR2/data/i out=HiPS_i/ id=CDS/P/DES-DR2/i partitioning=false "pixelCut=-1 400 asinh" mode=mean PNG hips_service_url = https://alasky.cds.unistra.fr/DES/DR2/CDS_P_DES-DR2_i hips_progenitor_url = https://alasky.cds.unistra.fr/DES/DR2/CDS_P_DES-DR2_i/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/DES/DR2/CDS_P_DES-DR2_i hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 0.1261 moc_order = 11 obs_initial_ra = 31.5154083 obs_initial_dec = -27.4936367 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288493974 ID = CDS/P/DES-DR2/r hips_doi = 10.26093/cds/aladin/10cx-as5 hips_initial_fov = 0.3 hips_initial_ra = 31.5154083 hips_initial_dec = -27.4936367 creator_did = ivo://CDS/P/DES-DR2/r hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = median hips_creator = Boch T. (CDS) hips_copyright = Université de Strasbourg/CNRS obs_title = DES-DR2 r obs_collection = DES-DR2 r obs_description = The second public data release of the Dark Energy Survey, DES DR2, is based on optical/near-infrared imaging by the Dark Energy Camera mounted on the 4 m Blanco telescope at Cerro Tololo Inter-American Observatory in Chile. DES DR2 includes ~691 million distinct astronomical objects detected in 10,169 coadded image tiles of size 0.534 deg2 produced from 76,217 single epoch images. obs_ack = https://www.darkenergysurvey.org/the-des-project/data-access/ prov_progenitor = https://desdr-server.ncsa.illinois.edu/ bib_reference = 2021ApJS..255...20A bib_reference_url = https://ui.adsabs.harvard.edu/abs/2021ApJS..255...20A/abstract obs_copyright = DECaM Plane Survey / NOAO obs_copyright_url = http://decaps.skymaps.info/ client_category = Image/Optical/DES t_min = 56519 t_max = 58492 obs_regime = Optical em_min = 5.65e-7 em_max = 7.17e-7 hips_builder = Aladin/HipsGen v12.001 hips_version = 1.4 hips_release_date = 2023-01-19T06:13Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = -1.2 400 hips_data_range = -10260 30731 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.305E-5 dataproduct_type = image hipsgen_date = 2023-01-06T16:45Z hipsgen_params = cache=./tmp in=data/r out=hips/ creator_did=CDS/P/DES-DR2/r partitioning=false TILES hips_creation_date = 2023-01-06T16:45Z hipsgen_date_1 = 2023-01-19T06:13Z hipsgen_params_1 = cache=./tmp in=data/r out=hips/ creator_did=CDS/P/DES-DR2/r partitioning=false "hips_pixel_cut=-1.2 400 asinh" method=mean PNG hips_service_url = https://alasky.cds.unistra.fr/DES/DR2/CDS_P_DES-DR2_r hips_progenitor_url = https://alasky.cds.unistra.fr/DES/DR2/CDS_P_DES-DR2_r/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/DES/DR2/CDS_P_DES-DR2_r hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 0.1261 moc_order = 11 obs_initial_ra = 31.5154083 obs_initial_dec = -27.4936367 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288493894 ID = CDS/P/DES-DR2/z hips_doi = 10.26093/cds/aladin/171a-8rq creator_did = ivo://CDS/P/DES-DR2/z hips_creator = Buga M. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = DES-DR2 z obs_collection = DES-DR2 z obs_description = The second public data release of the Dark Energy Survey, DES DR2, based on optical/near-infrared imaging by the Dark Energy Camera mounted on the 4 m Blanco telescope at Cerro Tololo Inter-American Observatory in Chile. DES DR2 includes ~691 million distinct astronomical objects detected in 10,169 coadded image tiles of size 0.534 deg2 produced from 76,217 single epoch images. obs_ack = https://www.darkenergysurvey.org/the-des-project/data-access/ prov_progenitor = https://desdr-server.ncsa.illinois.edu/ bib_reference = 2021ApJS..255...20A bib_reference_url = https://ui.adsabs.harvard.edu/abs/2021ApJS..255...20A/abstract obs_copyright = DECaM Plane Survey / NOAO obs_copyright_url = http://decaps.skymaps.info/ client_category = Image/Optical/DES t_min = 56519 t_max = 58492 obs_regime = Optical em_min = 8.284e-7 em_max = 1.0102e-6 hips_builder = Aladin/HipsGen v12.033 hips_version = 1.4 hips_release_date = 2023-03-03T05:08Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_pixel_cut = -1.2 400 hips_data_range = -7514 22361 hips_initial_fov = 0.3 hips_initial_ra = 31.5154083 hips_initial_dec = -27.4936367 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.305E-5 dataproduct_type = image hipsgen_date = 2023-02-14T00:12Z hipsgen_params = cache=./tmp in=/data-test-iscsi/boch/DES-DR2/data/z out=HiPS_z/ id=CDS/P/DES-DR2/z partitioning=false TILES hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeKeepTile treeMean hips_creation_date = 2023-02-14T00:12Z hips_tile_format = png fits hipsgen_date_1 = 2023-02-25T23:07Z hipsgen_params_1 = cache=./tmp in=/data-test-iscsi/boch/DES-DR2/data/z out=HiPS_z/ id=CDS/P/DES-DR2/z partitioning=false mode=keeptile TILES hipsgen_date_2 = 2023-03-03T05:08Z hipsgen_params_2 = cache=./tmp in=/data-test-iscsi/boch/DES-DR2/data/z out=HiPS_z/ id=CDS/P/DES-DR2/z partitioning=false "pixelCut=-1.2 400 asinh" mode=mean PNG hips_service_url = https://alasky.cds.unistra.fr/DES/DR2/CDS_P_DES-DR2_z hips_progenitor_url = https://alasky.cds.unistra.fr/DES/DR2/CDS_P_DES-DR2_z/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/DES/DR2/CDS_P_DES-DR2_z hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 0.1261 moc_order = 11 obs_initial_ra = 31.5154083 obs_initial_dec = -27.4936367 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288494206 ID = CDS/P/DESI-Legacy-Surveys/DR10/color hips_doi = 10.26093/cds/aladin/k3kq-9e creator_did = ivo://CDS/P/DESI-Legacy-Surveys/DR10/color client_category = Image/Optical/Legacy Surveys hips_creator = Boch T. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = DESI Legacy Surveys color (g, r, i, z) obs_collection = DESI Legacy Surveys obs_description = The DESI Legacy Imaging Surveys (http://legacysurvey.org/) are a combination of three public projects (the Dark Energy Camera Legacy Survey, the Beijing-Arizona Sky Survey, and the Mayall z-band Legacy Survey) that will jointly image ?14,000 deg2 of the extragalactic sky visible from the northern hemisphere in three optical bands (g, r, and z) using telescopes at the Kitt Peak National Observatory and the Cerro Tololo Inter-American Observatory. The combined survey footprint is split into two contiguous areas by the Galactic plane. The optical imaging is conducted using a unique strategy of dynamically adjusting the exposure times and pointing selection during observing that results in a survey of nearly uniform depth. As of DR10, the Legacy Surveys inference model is being self-consistently expanded to > 20,000 square degrees by incorporating additional DECam data from NOIRLab that includes extra optical bands (g, r, i, z). obs_ack = https://www.legacysurvey.org/acknowledgment/ prov_progenitor = https://portal.nersc.gov/cfs/cosmo/data/legacysurvey/dr10/south/coadd/ bib_reference = 2019AJ....157..168D bib_reference_url = https://ui.adsabs.harvard.edu/abs/2019AJ....157..168D/abstract obs_copyright = DESI Imaging Legacy Surveys obs_copyright_url = https://www.legacysurvey.org/acknowledgment/ obs_regime = Optical em_min = 3.9e-7 em_max = 1.02e-6 hips_builder = Aladin/HipsGen v12.044 hips_version = 1.4 hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 190.0040433 hips_initial_dec = -5.2893305 hips_initial_fov = 1.0 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.277E-5 dataproduct_type = image hipsgen_date = 2023-03-08T08:10Z hipsgen_params = id=CDS/P/Legacy-Surveys/color in=data/color out=hips/CDS_P_Legacy-Surveys_color partitioning=false color=png mode=median TILES hips_release_date = 2023-03-10T08:55Z hips_tile_format = png hipsgen_date_1 = 2023-03-08T14:03Z hipsgen_params_1 = id=CDS/P/Legacy-Surveys/color in=data/color out=hips/CDS_P_Legacy-Surveys_color partitioning=false color=png mode=median ALLSKY hips_creation_date = 2023-03-08T14:03Z hipsgen_date_2 = 2023-03-09T07:40Z hipsgen_params_2 = id=CDS/P/Legacy-Surveys/color in=data/color out=hips/CDS_P_Legacy-Surveys_color partitioning=false color=png mode=median ALLSKY hipsgen_date_3 = 2023-03-09T13:42Z hipsgen_params_3 = id=CDS/P/Legacy-Surveys/color in=data/color out=hips/CDS_P_Legacy-Surveys_color partitioning=false color=png mode=median ALLSKY hipsgen_date_4 = 2023-03-10T07:10Z hipsgen_params_4 = id=CDS/P/Legacy-Surveys/color in=data/color out=hips/CDS_P_Legacy-Surveys_color partitioning=false color=png mode=median ALLSKY hipsgen_date_5 = 2023-03-10T08:54Z hipsgen_params_5 = id=CDS/P/Legacy-Surveys/color in=data/color out=hips/CDS_P_Legacy-Surveys_color partitioning=false color=png mode=median ALLSKY hips_overlay = overlayMean mergeOverwriteTile treeMedian dataproduct_subtype = color moc_sky_fraction = 0.5554 hips_service_url = https://alasky.cds.unistra.fr/DESI-legacy-surveys/DR10/CDS_P_DESI-Legacy-Surveys_DR10_color hips_progenitor_url = https://alasky.cds.unistra.fr/DESI-legacy-surveys/DR10/CDS_P_DESI-Legacy-Surveys_DR10_color/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/DESI-legacy-surveys/DR10/CDS_P_DESI-Legacy-Surveys_DR10_color hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 11 obs_initial_ra = 190.0040433 obs_initial_dec = -5.2893305 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288494274 ID = CDS/P/DESI-Legacy-Surveys/DR10/g hips_doi = 10.26093/cds/aladin/296y-bgk creator_did = ivo://CDS/P/DESI-Legacy-Surveys/DR10/g client_category = Image/Optical/Legacy Surveys hips_creator = Boch T. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = DESI Legacy Surveys g obs_collection = DESI Legacy Surveys obs_description = The DESI Legacy Imaging Surveys (http://legacysurvey.org/) are a combination of three public projects (the Dark Energy Camera Legacy Survey, the Beijing-Arizona Sky Survey, and the Mayall z-band Legacy Survey) that will jointly image ?14,000 deg2 of the extragalactic sky visible from the northern hemisphere in three optical bands (g, r, and z) using telescopes at the Kitt Peak National Observatory and the Cerro Tololo Inter-American Observatory. The combined survey footprint is split into two contiguous areas by the Galactic plane. The optical imaging is conducted using a unique strategy of dynamically adjusting the exposure times and pointing selection during observing that results in a survey of nearly uniform depth. As of DR10, the Legacy Surveys inference model is being self-consistently expanded to > 20,000 square degrees by incorporating additional DECam data from NOIRLab that includes extra optical bands (g, r, i, z). obs_ack = https://www.legacysurvey.org/acknowledgment/ prov_progenitor = https://portal.nersc.gov/cfs/cosmo/data/legacysurvey/dr10/south/coadd/ bib_reference = 2019AJ....157..168D bib_reference_url = https://ui.adsabs.harvard.edu/abs/2019AJ....157..168D/abstract obs_copyright = DESI Imaging Legacy Surveys obs_copyright_url = https://www.legacysurvey.org/acknowledgment/ obs_regime = Optical em_min = 3.876e-7 em_max = 5.808e-7 hips_builder = Aladin/HipsGen v12.044 hips_version = 1.4 hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_tile_format = fits png hips_status = public master clonableOnce hips_initial_ra = 190.0040433 hips_initial_dec = -5.2893305 hips_initial_fov = 1.0 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.277E-5 dataproduct_type = image hipsgen_date = 2023-03-28T12:08Z hipsgen_params = id=CDS/P/DESI-Legacy-Surveys/DR10/g in=data/g out=hips/CDS_P_Legacy-Surveys_g partitioning=false -cache=./tmp TILES hips_release_date = 2023-04-05T10:37Z hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeMean treeMean hips_creation_date = 2023-03-30T07:12Z hips_data_range = -21.91 65.54 moc_sky_fraction = 0.5356 hips_pixel_cut = -0.0015 0.5 asinh hips_service_url = https://alasky.cds.unistra.fr/DESI-legacy-surveys/DR10/CDS_P_DESI-Legacy-Surveys_DR10_g hips_progenitor_url = https://alasky.cds.unistra.fr/DESI-legacy-surveys/DR10/CDS_P_DESI-Legacy-Surveys_DR10_g/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/DESI-legacy-surveys/DR10/CDS_P_DESI-Legacy-Surveys_DR10_g hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 11 obs_initial_ra = 190.0040433 obs_initial_dec = -5.2893305 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288494342 ID = CDS/P/DESI-Legacy-Surveys/DR10/i hips_doi = 10.26093/cds/aladin/1txe-0rm creator_did = ivo://CDS/P/DESI-Legacy-Surveys/DR10/i hips_creator = Buga M. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = DESI Legacy Survey i obs_collection = DESI Legacy Survey obs_description = The DESI Legacy Imaging Surveys (http://legacysurvey.org/) are a combination of three public projects (the Dark Energy Camera Legacy Survey, the Beijing-Arizona Sky Survey, and the Mayall z-band Legacy Survey) that will jointly image ~14,000 deg2 of the extragalactic sky visible from the northern hemisphere in three optical bands (g, r and z) using telescopes at the Kitt Peak National Observatory and the Cerro Tololo Inter-American Observatory. The combined survey footprint is split into two contigous areas by the Galactic plane. The optical imaging is conducted using a unique strategy of dynamically adjusting the exposure times and pointing selection during observing that results in a survey of nearly uniform depth. As of DR10, the Legacy Surveys inference model is being self-consistently expanded to > 20,000 square degrees by incorporating additional DECam data from NOIRLab that includes extra optical bands (g, r, i, z). obs_ack = https://www.legacysurvey.org/acknowledgment/ prov_progenitor = https:/portal.nersc.gov/cfs/cosmo/data/legacysurvey/dr10/south/coadd/ bib_reference = 2019AJ....157..168D bib_reference_url = https://ui.adsabs.harvard.edu/abs/2019AJ....157..168D/abstract obs_copyright = DESI Imaging Legacy Surveys obs_copyright_url = https://legacysurvey.org/acknowledgment/ t_min = 56878 t_max = 58549 obs_regime = Optical em_min = 7.1e-7 em_max = 8.57e-7 client_category = Image/Optical/Legacy Surveys hips_builder = Aladin/HipsGen v12.055 hips_version = 1.4 hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_bitpix = -32 hips_pixel_cut = -0.001 0.5 hips_data_range = -14.82 44.3 hips_initial_ra = 190.0040433 hips_initial_dec = -5.2893305 hips_initial_fov = 1.0 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.277E-5 dataproduct_type = image data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeKeepTile treeMean hips_release_date = 2023-05-16T18:44Z moc_sky_fraction = 0.4485 hipsgen_date = 2023-05-16T02:09Z hipsgen_params = id=CDS/P/DESI-Legacy-Surveys/DR10/i in=i out=HiPS_i/ partitioning=false -cache=./tmp mode=keeptile TILES hips_creation_date = 2023-05-16T02:09Z hipsgen_date_1 = 2023-05-16T18:44Z hipsgen_params_1 = id=CDS/P/DESI-Legacy-Surveys/DR10/i in=i out=HiPS_i/ partitioning=false -cache=./tmp mode=median "pixelCut=-0.001 0.5 asinh" PNG hips_service_url = https://alasky.cds.unistra.fr/DESI-legacy-surveys/DR10/CDS_P_DESI-Legacy-Surveys_DR10_i hips_progenitor_url = https://alasky.cds.unistra.fr/DESI-legacy-surveys/DR10/CDS_P_DESI-Legacy-Surveys_DR10_i/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/DESI-legacy-surveys/DR10/CDS_P_DESI-Legacy-Surveys_DR10_i hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 190.0040433 obs_initial_dec = -5.2893305 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288494414 ID = CDS/P/DESI-Legacy-Surveys/DR10/r hips_doi = 10.26093/cds/aladin/3zv5-jqr creator_did = ivo://CDS/P/DESI-Legacy-Surveys/DR10/r client_category = Image/Optical/Legacy Surveys hips_creator = Buga M. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = DESI Legacy Survey r obs_collection = DESI Legacy Survey obs_description = The DESI Legacy Imaging Surveys (http://legacysurvey.org/) are a combination of three public projects (the Dark Energy Camera Legacy Survey, the Beijing-Arizona Sky Survey, and the Mayall z-band Legacy Survey) that will jointly image ~14,000 deg2 of the extragalactic sky visible from the northern hemisphere in three optical bands (g, r and z) using telescopes at the Kitt Peak National Observatory and the Cerro Tololo Inter-American Observatory. The combined survey footprint is split into two contigous areas by the Galactic plane. The optical imaging is conducted using a unique strategy of dynamically adjusting the exposure times and pointing selection during observing that results in a survey of nearly uniform depth. As of DR10, the Legacy Surveys inference model is being self-consistently expanded to > 20,000 square degrees by incorporating additional DECam data from NOIRLab that includes extra optical bands (g, r, i, z). obs_ack = https://www.legacysurvey.org/acknowledgment/ prov_progenitor = https:/portal.nersc.gov/cfs/cosmo/data/legacysurvey/dr10/south/coadd/ bib_reference = 2019AJ....157..168D bib_reference_url = https://ui.adsabs.harvard.edu/abs/2019AJ....157..168D/abstract obs_copyright = DESI Imaging Legacy Surveys obs_copyright_url = https://legacysurvey.org/acknowledgment/ t_min = 56878 t_max = 58549 obs_regime = Optical em_min = 5.618e-7 em_max = 7.26e-7 hips_builder = Aladin/HipsGen v12.055 hips_version = 1.4 hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 190.0040433 hips_initial_dec = -5.2893305 hips_initial_fov = 1.0 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.277E-5 dataproduct_type = image hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeKeepTile treeMean hips_release_date = 2023-06-30T13:12Z hips_tile_format = png fits hips_pixel_cut = -0.1321 10.17 hips_data_range = -29.81 88.51 moc_sky_fraction = 0.5009 hipsgen_date = 2023-05-20T22:28Z hipsgen_params = id=CDS/P/DESI-Legacy-Surveys/DR10/r in=bande_r/r out=bande_r/HiPS_r/ partitioning=false -cache=./tmp INDEX TILES hips_creation_date = 2023-05-20T22:28Z hipsgen_date_1 = 2023-06-15T02:09Z hipsgen_params_1 = id=CDS/P/DESI-Legacy-Surveys/DR10/r in=bande_r/r out=bande_r/HiPS_r/ partitioning=false -cache=./tmp mode=median "pixelCut=-0.001 0.5 asinh" PNG hipsgen_date_2 = 2023-06-30T13:12Z hipsgen_params_2 = id=CDS/P/DESI-Legacy-Surveys/DR10/r in=bande_r/r out=bande_r/HiPS_r/ partitioning=false -cache=./tmp mode=keeptile TILES hips_service_url = https://alasky.cds.unistra.fr/DESI-legacy-surveys/DR10/CDS_P_DESI-Legacy-Surveys_DR10_r hips_progenitor_url = https://alasky.cds.unistra.fr/DESI-legacy-surveys/DR10/CDS_P_DESI-Legacy-Surveys_DR10_r/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/DESI-legacy-surveys/DR10/CDS_P_DESI-Legacy-Surveys_DR10_r hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 190.0040433 obs_initial_dec = -5.2893305 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288494530 ID = CDS/P/DESI-Legacy-Surveys/DR10/z hips_doi = 10.26093/cds/aladin/3rpj-gpa creator_did = ivo://CDS/P/DESI-Legacy-Surveys/DR10/z client_category = Image/Optical/Legacy Surveys hips_creator = Buga M. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = DESI Legacy Surveys z obs_collection = DESI Legacy Surveys obs_description = The DESI Legacy Imaging Surveys (http://legacysurvey.org/) are a combination of three public projects (the Dark Energy Camera Legacy Survey, the Beijing-Arizona Sky Survey, and the Mayall z-band Legacy Survey) that will jointly image ?14,000 deg2 of the extragalactic sky visible from the northern hemisphere in three optical bands (g, r, and z) using telescopes at the Kitt Peak National Observatory and the Cerro Tololo Inter-American Observatory. The combined survey footprint is split into two contiguous areas by the Galactic plane. The optical imaging is conducted using a unique strategy of dynamically adjusting the exposure times and pointing selection during observing that results in a survey of nearly uniform depth. As of DR10, the Legacy Surveys inference model is being self-consistently expanded to > 20,000 square degrees by incorporating additional DECam data from NOIRLab that includes extra optical bands (g, r, i, z). obs_ack = https://www.legacysurvey.org/acknowledgment/ prov_progenitor = https://portal.nersc.gov/cfs/cosmo/data/legacysurvey/dr10/south/coadd/ bib_reference = 2019AJ....157..168D bib_reference_url = https://ui.adsabs.harvard.edu/abs/2019AJ....157..168D/abstract obs_copyright = DESI Imaging Legacy Surveys obs_copyright_url = https://www.legacysurvey.org/acknowledgment/ obs_regime = Optical em_min = 8.252e-7 em_max = 1.0145e-6 hips_builder = Aladin/HipsGen v12.055 hips_version = 1.4 hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 190.0040433 hips_initial_dec = -5.2893305 hips_initial_fov = 1.0 hips_pixel_scale = 5.591E-5 s_pixel_scale = 7.277E-5 dataproduct_type = image hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwriteTile treeMean hips_release_date = 2023-09-05T04:19Z hips_tile_format = png fits hips_pixel_cut = -0.001 0.6 hips_data_range = -38.07 113.7 moc_sky_fraction = 0.5161 hipsgen_date = 2023-08-07T18:02Z hipsgen_params = id=CDS/P/DESI-Legacy-Surveys/DR10/z in=bande_z/z out=bande_z/HiPS_z/ partitioning=false -cache=./tmp TILES hips_creation_date = 2023-08-07T18:02Z hipsgen_date_1 = 2023-08-16T20:22Z hipsgen_params_1 = id=CDS/P/DESI-Legacy-Surveys/DR10/z in=bande_z/z out=bande_z/HiPS_z/ partitioning=false -cache=./tmp mode=median "pixelcut=0.001 1 asinh" PNG hipsgen_date_2 = 2023-09-04T16:45Z hipsgen_params_2 = id=CDS/P/DESI-Legacy-Surveys/DR10/z -clean in=bande_z/z out=bande_z/HiPS_z/ partitioning=false -cache=./tmp mode=median "pixelcut=-0.001 0.6 asinh" PNG hips_service_url = https://alasky.cds.unistra.fr/DESI-legacy-surveys/DR10/CDS_P_DESI-Legacy-Surveys_DR10_z hips_progenitor_url = https://alasky.cds.unistra.fr/DESI-legacy-surveys/DR10/CDS_P_DESI-Legacy-Surveys_DR10_z/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/DESI-legacy-surveys/DR10/CDS_P_DESI-Legacy-Surveys_DR10_z hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 11 obs_initial_ra = 190.0040433 obs_initial_dec = -5.2893305 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288494634 ID = CDS/P/DM/I/345/gaia2 hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/I/345/gaia2 obs_title = Density map for Gaia DR2 (I/345/gaia2) client_category = Ancillary/GaiaDR2 prov_did = ivo://CDS/I/345/gaia2 hips_builder = Aladin/HipsGen v11.071 hips_version = 1.4 hips_release_date = 2022-03-01T13:45Z hips_frame = equatorial hips_order = 4 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png jpeg fits hips_pixel_bitpix = -32 hips_pixel_cut = 0 55 hips_data_range = -83 249 hips_pixel_scale = 0.007157 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 4596125 hipsgen_date = 2018-04-17T10:01Z hipsgen_params = in=density-maps/gaia-DR2-dens-map-8192.hpx out=density-maps/hips-gaia-DR2-density-map -creator_did=ivo://CDS/P/DM/I/345/gaia2 "-hips_pixel_cut=0 40 sqrt" -method=mean MAPTILES JPEG hips_creation_date = 2018-04-17T10:01Z hipsgen_date_1 = 2018-04-17T10:02Z hipsgen_params_1 = in=density-maps/gaia-DR2-dens-map-8192.hpx out=density-maps/hips-gaia-DR2-density-map -creator_did=ivo://CDS/P/DM/I/345/gaia2 "-hips_pixel_cut=0 40 sqrt" -method=mean MAPTILES JPEG hipsgen_date_2 = 2018-04-17T10:34Z hipsgen_params_2 = in=density-maps/gaia-DR2-dens-map-8192.hpx out=density-maps/hips-gaia-DR2-density-map -creator_did=ivo://CDS/P/DM/I/345/gaia2 "-hips_pixel_cut=0 55 sqrt" -method=mean MAPTILES JPEG hipsgen_date_3 = 2018-04-17T10:36Z hipsgen_params_3 = in=density-maps/gaia-DR2-dens-map-8192.hpx out=density-maps/hips-gaia-DR2-density-map -creator_did=ivo://CDS/P/DM/I/345/gaia2 "-hips_pixel_cut=0 55 sqrt" -method=mean MAPTILES JPEG hipsgen_date_4 = 2019-06-27T10:19Z hipsgen_params_4 = out=/data/footprints/tables/vizier/I_345_gaia2/hips-density-map UPDATE hipsgen_date_5 = 2022-03-01T13:38Z hipsgen_params_5 = out=hips-density-map creator_did=ivo://CDS/P/DM/I/345/gaia2 PNG hipsgen_date_6 = 2022-03-01T13:42Z hipsgen_params_6 = out=hips-density-map creator_did=ivo://CDS/P/DM/I/345/gaia2 "-pixelcut=0 55 log" PNG hipsgen_date_7 = 2022-03-01T13:45Z hipsgen_params_7 = out=hips-density-map creator_did=ivo://CDS/P/DM/I/345/gaia2 "-pixelcut=0 55 log" mode=keeptile PNG hips_service_url = https://alasky.cds.unistra.fr/ancillary/GaiaDR2/hips-density-map hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/GaiaDR2/hips-density-map hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 9 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288478778 ID = CDS/P/DM/I/350/gaiaedr3 hips_initial_fov = 130.0 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 creator_did = ivo://CDS/P/DM/I/350/gaiaedr3 hips_creator = Boch T. (CDS) hips_copyright = CNRS/Unistra obs_title = Density map for Gaia EDR3 (I/350/gaiaedr3) obs_collection = Gaia obs_copyright = ESA/Gaia mission/DPAC obs_copyright_url = https://dx.doi.org/10.5270/esa-1ugzkg7 data_bunit = sr-1 client_category = Ancillary/GaiaEDR3 prov_did = ivo://CDS/I/350/gaiaedr3 hips_builder = Aladin/HipsGen v11.025 hips_version = 1.4 hips_release_date = 2020-11-27T06:48Z hips_frame = equatorial hips_order = 7 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_bitpix = -32 hips_pixel_cut = 0 12000 hips_pixel_scale = 0.007157 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 4486027 hipsgen_date = 2020-11-27T06:47Z hipsgen_params = in=density-maps/gaia-EDR3-dens-map-8192.hpx out=density-maps/hips-gaia-EDR3-density-map -creator_did=ivo://CDS/P/DM/I/350/gaiaedr3 "-hips_pixel_cut=0 55 sqrt" -method=mean MAPTILES JPEG hips_creation_date = 2020-11-27T06:47Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/GaiaEDR3/density-map hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/GaiaEDR3/density-map hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 7 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288487850 ID = CDS/P/DM/I/355/gaiadr3 hips_initial_fov = 130.0 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 creator_did = ivo://CDS/P/DM/I/355/gaiadr3 hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = Gaia DR3 density map obs_collection = Gaia obs_copyright = ESA/Gaia mission/DPAC obs_copyright_url = https://doi.org/10.5270/esa-qa4lep3 data_bunit = sr-1 client_category = Ancillary/GaiaDR3 prov_did = ivo://CDS/I/355/gaiadr3 hips_builder = Aladin/HipsGen v11.071 hips_version = 1.4 hips_release_date = 2022-06-15T09:24Z hips_frame = equatorial hips_order = 7 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_bitpix = -32 hips_pixel_cut = 0 20000 hips_pixel_scale = 8.946E-4 dataproduct_type = image moc_sky_fraction = 1 hips_creation_date = 2022-06-12T06:47Z hips_estsize = 287105287 hipsgen_date = 2022-06-13T13:06Z hipsgen_params = out=hips-density TREE hipsgen_date_1 = 2022-06-15T07:02Z hipsgen_params_1 = "hips_pixel_cut=0 20000 log" out=density-map method=MEAN JPEG -f hipsgen_date_2 = 2022-06-15T07:17Z hipsgen_params_2 = "hips_pixel_cut=0 20000 log" out=density-map maxThread=16 method=MEAN JPEG -f hips_service_url = https://alasky.cds.unistra.fr/ancillary/GaiaDR3/density-map hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/GaiaDR3/density-map hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 7 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288488266 ID = CDS/P/DM/flux-Bp/I/345/gaia2 hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/flux-Bp/I/345/gaia2 hips_creator = Boch T. (CDS) obs_title = Bp flux map for table I/345/gaia2 (Gaia DR2) obs_regime = Optical em_min = 3.28045e-07 em_max = 6.71903e-07 prov_did = ivo://CDS/I/345/gaia2 client_category = Ancillary/GaiaDR2 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T08:57Z hips_frame = equatorial hips_order = 4 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_bitpix = -32 hips_pixel_cut = 0 100000 hips_data_range = -2.521E8 7.565E8 hips_pixel_scale = 0.007157 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 4486027 hipsgen_date = 2018-04-17T07:37Z hipsgen_params = in=density-maps/param-weighted/gaia-DR2-Bp-map.hpx out=density-maps/param-weighted/hips-gaia-DR2-flux-Bp -creator_did=ivo://CDS/P/DM/flux-Bp/I/345/out "-hips_pixel_cut=0 200000 sqrt" -method=mean MAPTILES JPEG hips_creation_date = 2018-04-17T07:37Z hipsgen_date_1 = 2018-04-17T07:38Z hipsgen_params_1 = in=density-maps/param-weighted/gaia-DR2-Bp-map.hpx out=density-maps/param-weighted/hips-gaia-DR2-flux-Bp -creator_did=ivo://CDS/P/DM/flux-Bp/I/345/out "-hips_pixel_cut=0 200000 sqrt" -method=mean MAPTILES JPEG hipsgen_date_2 = 2018-04-17T08:02Z hipsgen_params_2 = in=density-maps/param-weighted/gaia-DR2-Bp-map.hpx out=density-maps/param-weighted/hips-gaia-DR2-flux-Bp -creator_did=ivo://CDS/P/DM/flux-Bp/I/345/out "-hips_pixel_cut=0 100000 sqrt" -method=mean MAPTILES JPEG hipsgen_date_3 = 2018-04-17T08:03Z hipsgen_params_3 = in=density-maps/param-weighted/gaia-DR2-Bp-map.hpx out=density-maps/param-weighted/hips-gaia-DR2-flux-Bp -creator_did=ivo://CDS/P/DM/flux-Bp/I/345/out "-hips_pixel_cut=0 100000 sqrt" -method=mean MAPTILES JPEG hipsgen_date_4 = 2019-05-21T08:57Z hipsgen_params_4 = out=/asd-volumes/sc1-asd-volume6/ancillary/GaiaDR2/Bp-flux-map UPDATE hips_service_url = https://alasky.cds.unistra.fr/ancillary/GaiaDR2/Bp-flux-map hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/GaiaDR2/Bp-flux-map hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 9 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288478430 ID = CDS/P/DM/flux-Bp/I/350/gaiaedr3 hips_initial_fov = 130.0 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 creator_did = ivo://CDS/P/DM/flux-Bp/I/350/gaiaedr3 hips_creator = Boch T. (CDS) hips_copyright = CNRS/Unistra obs_title = Bp flux map for table I/350/gaiaedr3 (Gaia EDR3) obs_collection = Gaia obs_copyright = ESA/Gaia mission/DPAC obs_copyright_url = https://dx.doi.org/10.5270/esa-1ugzkg7 obs_regime = Optical em_min = 3.29283e-7 em_max = 6.73811e-7 data_bunit = count.s-1.sr-1 client_category = Ancillary/GaiaEDR3 prov_did = ivo://CDS/I/350/gaiaedr3 hips_builder = Aladin/HipsGen v11.025 hips_version = 1.4 hips_release_date = 2020-11-27T12:53Z hips_frame = equatorial hips_order = 7 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_bitpix = -32 dataproduct_type = image moc_sky_fraction = 1 hips_creation_date = 2019-05-21T08:57Z hips_pixel_scale = 8.946E-4 hips_estsize = 287105287 hipsgen_date = 2020-11-26T10:02Z hipsgen_params = out=hips-flux/save/bp-flux TREE hipsgen_date_1 = 2020-11-26T10:52Z hipsgen_params_1 = out=hips-flux/bp-flux TREE hipsgen_date_2 = 2020-11-26T10:56Z hipsgen_params_2 = out=hips-flux/bp-flux TREE hipsgen_date_3 = 2020-11-26T11:01Z hipsgen_params_3 = out=hips-flux/bp-flux TREE hipsgen_date_4 = 2020-11-26T11:17Z hipsgen_params_4 = out=hips-flux/bp-flux TREE hipsgen_date_5 = 2020-11-26T11:21Z hipsgen_params_5 = out=hips-flux/bp-flux TREE hipsgen_date_6 = 2020-11-26T11:22Z hipsgen_params_6 = out=hips-flux/bp-flux TREE hipsgen_date_7 = 2020-11-26T12:56Z hipsgen_params_7 = out=hips-flux/bp-flux TREE hipsgen_date_8 = 2020-11-27T07:42Z hipsgen_params_8 = out=hips-flux/bp-flux TREE hips_pixel_cut = 0 2.0E7 hipsgen_date_9 = 2020-11-27T12:53Z hipsgen_params_9 = out=hips-flux/bp-flux "pixelCut=0 2e7 log" JPEG hips_service_url = https://alasky.cds.unistra.fr/ancillary/GaiaEDR3/Bp-flux-map hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/GaiaEDR3/Bp-flux-map hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 7 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288487630 ID = CDS/P/DM/flux-Bp/I/355/gaiadr3 hips_initial_fov = 130.0 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 creator_did = ivo://CDS/P/DM/flux-Bp/I/355/gaiadr3 hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = Bp flux map for table I/355/gaiadr3 (Gaia DR3) obs_collection = Gaia obs_copyright = ESA/Gaia mission/DPAC obs_copyright_url = https://doi.org/10.5270/esa-qa4lep3 obs_regime = Optical em_min = 3.29283e-7 em_max = 6.73811e-7 data_bunit = count.s-1.sr-1 client_category = Ancillary/GaiaDR3 prov_did = ivo://CDS/I/355/gaiadr3 hips_builder = Aladin/HipsGen v11.071 hips_version = 1.4 hips_release_date = 2022-06-16T09:03Z hips_frame = equatorial hips_order = 7 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_bitpix = -32 dataproduct_type = image moc_sky_fraction = 1 hips_creation_date = 2022-06-12T22:59Z hips_pixel_scale = 8.946E-4 hips_pixel_cut = 0 2.0E7 hips_estsize = 287105287 hipsgen_date = 2022-06-14T14:17Z hipsgen_params = "hips_pixel_cut=0 2e7 asinh" out=bp-flux "hips_pixel_cut=0 20000000 asinh" JPEG hipsgen_date_1 = 2022-06-15T06:54Z hipsgen_params_1 = "hips_pixel_cut=0 2e7 asinh" out=bp-flux "hips_pixel_cut=0 20000000 asinh" method=MEAN JPEG -f hipsgen_date_2 = 2022-06-16T06:43Z hipsgen_params_2 = "hips_pixel_cut=0 2e7 asinh" out=bp-flux "hips_pixel_cut=0 20000000 asinh" method=MEAN JPEG -f hipsgen_date_3 = 2022-06-16T07:05Z hipsgen_params_3 = "hips_pixel_cut=0 2e7 asinh" out=bp-flux "hips_pixel_cut=0 20000000 asinh" method=MEAN JPEG -f hips_service_url = https://alasky.cds.unistra.fr/ancillary/GaiaDR3/Bp-flux-map hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/GaiaDR3/Bp-flux-map hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 7 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288487962 ID = CDS/P/DM/flux-G/I/345/gaia2 hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/flux-G/I/345/gaia2 hips_creator = Boch T. (CDS) obs_title = G flux map for table I/345/gaia2 (Gaia DR2) obs_regime = Optical em_min = 3.30660e-07 em_max = 10.45065e-07 prov_did = ivo://CDS/I/345/gaia2 client_category = Ancillary/GaiaDR2 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T08:57Z hips_frame = equatorial hips_order = 4 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_bitpix = -32 hips_pixel_cut = 0 200000 hips_data_range = -3.760E8 1.128E9 hips_pixel_scale = 0.007157 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 4486027 hipsgen_date = 2018-04-17T07:05Z hipsgen_params = in=density-maps/param-weighted/gaia-DR2-G-map.hpx out=density-maps/param-weighted/hips-gaia-DR2-flux-G -creator_did=ivo://CDS/P/DM/flux-G/I/345/out "-hips_pixel_cut=0 200000 sqrt" -method=mean MAPTILES JPEG hips_creation_date = 2018-04-17T07:05Z hipsgen_date_1 = 2018-04-17T07:08Z hipsgen_params_1 = in=density-maps/param-weighted/gaia-DR2-G-map.hpx out=density-maps/param-weighted/hips-gaia-DR2-flux-G -creator_did=ivo://CDS/P/DM/flux-G/I/345/out "-hips_pixel_cut=0 200000 sqrt" -method=mean MAPTILES JPEG hipsgen_date_2 = 2019-05-21T08:57Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/ancillary/GaiaDR2/G-flux-map UPDATE hips_service_url = https://alasky.cds.unistra.fr/ancillary/GaiaDR2/G-flux-map hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/GaiaDR2/G-flux-map hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 9 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288478570 ID = CDS/P/DM/flux-G/I/350/gaiaedr3 hips_initial_fov = 130.0 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 creator_did = ivo://CDS/P/DM/flux-G/I/350/gaiaedr3 hips_creator = Boch T. (CDS) hips_copyright = CNRS/Unistra obs_title = G flux map for table I/350/gaiaedr3 (Gaia EDR3) obs_collection = Gaia obs_copyright = ESA/Gaia mission/DPAC obs_copyright_url = https://dx.doi.org/10.5270/esa-1ugzkg7 obs_regime = Optical em_min = 3.29402e-7 em_max = 10.30196e-7 data_bunit = count.s-1.sr-1 client_category = Ancillary/GaiaEDR3 prov_did = ivo://CDS/I/350/gaiaedr3 hips_builder = Aladin/HipsGen v11.025 hips_version = 1.4 hips_release_date = 2020-11-27T15:11Z hips_frame = equatorial hips_order = 7 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_bitpix = -32 dataproduct_type = image moc_sky_fraction = 1 hips_creation_date = 2019-05-21T08:57Z hips_pixel_scale = 8.946E-4 hips_estsize = 287105287 hipsgen_date = 2020-11-26T10:02Z hipsgen_params = out=hips-flux/save/bp-flux TREE hipsgen_date_1 = 2020-11-26T10:52Z hipsgen_params_1 = out=hips-flux/bp-flux TREE hipsgen_date_2 = 2020-11-26T10:56Z hipsgen_params_2 = out=hips-flux/bp-flux TREE hipsgen_date_3 = 2020-11-26T11:01Z hipsgen_params_3 = out=hips-flux/bp-flux TREE hipsgen_date_4 = 2020-11-26T11:17Z hipsgen_params_4 = out=hips-flux/bp-flux TREE hipsgen_date_5 = 2020-11-26T11:21Z hipsgen_params_5 = out=hips-flux/bp-flux TREE hipsgen_date_6 = 2020-11-26T11:22Z hipsgen_params_6 = out=hips-flux/bp-flux TREE hipsgen_date_7 = 2020-11-26T12:56Z hipsgen_params_7 = out=hips-flux/bp-flux TREE hipsgen_date_8 = 2020-11-26T15:09Z hipsgen_params_8 = out=hips-flux/g-flux TREE hipsgen_date_9 = 2020-11-27T10:18Z hipsgen_params_9 = out=hips-flux/g-flux TREE hips_pixel_cut = 0 2.0E7 hipsgen_date_10 = 2020-11-27T15:11Z hipsgen_params_10 = out=hips-flux/g-flux "pixelCut=0 2e7 log" JPEG hips_service_url = https://alasky.cds.unistra.fr/ancillary/GaiaEDR3/G-flux-map hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/GaiaEDR3/G-flux-map hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 7 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288487742 ID = CDS/P/DM/flux-G/I/355/gaiadr3 creator_did = ivo://CDS/P/DM/flux-G/I/355/gaiadr3 hips_initial_fov = 130.0 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = G flux map for table I/355/gaiadr3 (Gaia DR3) obs_collection = Gaia obs_copyright = ESA/Gaia mission/DPAC obs_copyright_url = https://doi.org/10.5270/esa-qa4lep3 obs_regime = Optical em_min = 3.29402e-7 em_max = 10.30196e-7 data_bunit = count.s-1.sr-1 client_category = Ancillary/GaiaDR3 prov_did = ivo://CDS/I/355/gaiadr3 hips_builder = Aladin/HipsGen v11.071 hips_version = 1.4 hips_release_date = 2022-06-16T14:31Z hips_frame = equatorial hips_order = 7 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_bitpix = -32 hips_pixel_scale = 8.946E-4 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 287105287 hipsgen_date = 2022-06-12T22:59Z hipsgen_params = out=hips-flux/bp-flux TREE hips_creation_date = 2022-06-12T22:59Z hipsgen_date_1 = 2022-06-13T01:55Z hipsgen_params_1 = out=hips-flux/g-flux TREE hipsgen_date_2 = 2022-06-16T12:26Z hipsgen_params_2 = "hips_pixel_cut=0 2e7 asinh" out=g-flux "hips_pixel_cut=0 20000000 asinh" method=MEAN JPEG -f hips_pixel_cut = 0 2.0E7 hips_service_url = https://alasky.cds.unistra.fr/ancillary/GaiaDR3/G-flux-map hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/GaiaDR3/G-flux-map hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 7 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288488014 ID = CDS/P/DM/flux-Rp/I/345/gaia2 hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/flux-Rp/I/345/gaia2 hips_creator = Boch T. (CDS) obs_title = Rp flux map for table I/345/gaia2 (Gaia DR2) obs_regime = Optical em_min = 6.25497e-07 em_max = 10.60579e-07 prov_did = ivo://CDS/I/345/gaia2 client_category = Ancillary/GaiaDR2 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T08:57Z hips_frame = equatorial hips_order = 4 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_bitpix = -32 hips_pixel_cut = 0 100000 hips_data_range = -1.383E8 4.150E8 hips_pixel_scale = 0.007157 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 4486027 hipsgen_date = 2018-04-17T08:17Z hipsgen_params = in=density-maps/param-weighted/gaia-DR2-Rp-map.hpx out=density-maps/param-weighted/hips-gaia-DR2-flux-Rp -creator_did=ivo://CDS/P/DM/flux-Rp/I/345/out "-hips_pixel_cut=0 100000 sqrt" -method=mean MAPTILES JPEG hips_creation_date = 2018-04-17T08:17Z hipsgen_date_1 = 2018-04-17T08:18Z hipsgen_params_1 = in=density-maps/param-weighted/gaia-DR2-Rp-map.hpx out=density-maps/param-weighted/hips-gaia-DR2-flux-Rp -creator_did=ivo://CDS/P/DM/flux-Rp/I/345/out "-hips_pixel_cut=0 100000 sqrt" -method=mean MAPTILES JPEG hipsgen_date_2 = 2019-05-21T08:57Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/ancillary/GaiaDR2/Rp-flux-map UPDATE hips_service_url = https://alasky.cds.unistra.fr/ancillary/GaiaDR2/Rp-flux-map hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/GaiaDR2/Rp-flux-map hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 9 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288478642 ID = CDS/P/DM/flux-Rp/I/350/gaiaedr3 hips_initial_fov = 130.0 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 creator_did = ivo://CDS/P/DM/flux-Rp/I/350/gaiaedr3 hips_creator = Boch T. (CDS) hips_copyright = CNRS/Unistra obs_title = Rp flux map for table I/350/gaiaedr3 (Gaia EDR3) obs_collection = Gaia obs_copyright = ESA/Gaia mission/DPAC obs_copyright_url = https://dx.doi.org/10.5270/esa-1ugzkg7 obs_regime = Optical em_min = 6.19605e-7 em_max = 10.42296e-7 data_bunit = count.s-1.sr-1 client_category = Ancillary/GaiaEDR3 prov_did = ivo://CDS/I/350/gaiaedr3 hips_builder = Aladin/HipsGen v11.025 hips_version = 1.4 hips_release_date = 2020-11-27T14:11Z hips_frame = equatorial hips_order = 7 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_bitpix = -32 dataproduct_type = image moc_sky_fraction = 1 hips_creation_date = 2019-05-21T08:57Z hips_pixel_scale = 8.946E-4 hips_estsize = 287105287 hipsgen_date = 2020-11-26T10:02Z hipsgen_params = out=hips-flux/save/bp-flux TREE hipsgen_date_1 = 2020-11-26T10:52Z hipsgen_params_1 = out=hips-flux/bp-flux TREE hipsgen_date_2 = 2020-11-26T10:56Z hipsgen_params_2 = out=hips-flux/bp-flux TREE hipsgen_date_3 = 2020-11-26T11:01Z hipsgen_params_3 = out=hips-flux/bp-flux TREE hipsgen_date_4 = 2020-11-26T11:17Z hipsgen_params_4 = out=hips-flux/bp-flux TREE hipsgen_date_5 = 2020-11-26T11:21Z hipsgen_params_5 = out=hips-flux/bp-flux TREE hipsgen_date_6 = 2020-11-26T11:22Z hipsgen_params_6 = out=hips-flux/bp-flux TREE hipsgen_date_7 = 2020-11-26T12:56Z hipsgen_params_7 = out=hips-flux/bp-flux TREE hipsgen_date_8 = 2020-11-26T14:07Z hipsgen_params_8 = out=hips-flux/rp-flux TREE hipsgen_date_9 = 2020-11-26T14:17Z hipsgen_params_9 = out=hips-flux/rp-flux mode=keeptile TREE hipsgen_date_10 = 2020-11-26T14:45Z hipsgen_params_10 = out=hips-flux/rp-flux TREE hipsgen_date_11 = 2020-11-27T08:52Z hipsgen_params_11 = out=hips-flux/rp-flux TREE hips_pixel_cut = 0 2.0E7 hipsgen_date_12 = 2020-11-27T14:11Z hipsgen_params_12 = out=hips-flux/rp-flux "pixelCut=0 2e7 log" JPEG hips_service_url = https://alasky.cds.unistra.fr/ancillary/GaiaEDR3/Rp-flux-map hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/GaiaEDR3/Rp-flux-map hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 7 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288487794 ID = CDS/P/DM/flux-Rp/I/355/gaiadr3 creator_did = ivo://CDS/P/DM/flux-Rp/I/355/gaiadr3 hips_initial_fov = 130.0 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = Rp flux map for table I/355/gaiadr3 (Gaia DR3) obs_collection = Gaia obs_copyright = ESA/Gaia mission/DPAC obs_copyright_url = https://doi.org/10.5270/esa-qa4lep3 obs_regime = Optical em_min = 6.19605e-7 em_max = 10.42296e-7 data_bunit = count.s-1.sr-1 client_category = Ancillary/GaiaDR3 prov_did = ivo://CDS/I/355/gaiadr3 hips_builder = Aladin/HipsGen v11.071 hips_version = 1.4 hips_release_date = 2022-06-16T12:25Z hips_frame = galactic hips_order = 7 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_bitpix = -32 hips_pixel_scale = 8.946E-4 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 287105287 hipsgen_date = 2022-06-12T22:59Z hipsgen_params = out=hips-flux/bp-flux TREE hips_creation_date = 2022-06-12T22:59Z hipsgen_date_1 = 2022-06-13T00:27Z hipsgen_params_1 = out=hips-flux/rp-flux TREE hipsgen_date_2 = 2022-06-16T09:08Z hipsgen_params_2 = "hips_pixel_cut=0 2e7 asinh" out=rp-flux "hips_pixel_cut=0 20000000 asinh" method=MEAN JPEG -f hips_pixel_cut = 0 2.0E7 hips_service_url = https://alasky.cds.unistra.fr/ancillary/GaiaDR3/Rp-flux-map hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/GaiaDR3/Rp-flux-map hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 7 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288488070 ID = CDS/P/DM/flux-color-Rp-G-Bp/I/345/gaia2 hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/flux-color-Rp-G-Bp/I/345/gaia2 hips_creator = Boch T. (CDS) obs_title = Color flux map for I/345/gaia2 (Gaia DR2) obs_regime = Optical prov_did = ivo://CDS/I/345/gaia2 client_category = Ancillary/GaiaDR2 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T08:57Z hips_frame = equatorial hips_order = 4 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg hips_pixel_scale = 0.007157 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 73407 hips_creation_date = 2018-04-17T07:37Z hips_pixel_cut = 0 100000 hips_data_range = -2.521E8 7.565E8 hipsgen_date = 2018-04-19T12:45Z hipsgen_params = out=density-maps/param-weighted/test -order=3 allsky hipsgen_date_1 = 2018-04-19T12:46Z hipsgen_params_1 = out=density-maps/param-weighted/test color=jpeg -order=3 allsky hips_order_min = 0 dataproduct_subtype = color hipsgen_date_2 = 2019-05-21T08:57Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/ancillary/GaiaDR2/color-Rp-G-Bp-flux-map UPDATE hips_service_url = https://alasky.cds.unistra.fr/ancillary/GaiaDR2/color-Rp-G-Bp-flux-map hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/GaiaDR2/color-Rp-G-Bp-flux-map hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 9 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288478498 ID = CDS/P/DM/flux-color-Rp-G-Bp/I/350/gaiaedr3 hips_initial_fov = 130.0 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 creator_did = ivo://CDS/P/DM/flux-color-Rp-G-Bp/I/350/gaiaedr3 hips_creator = Boch T. (CDS) hips_copyright = CNRS/Unistra obs_title = Color flux map for I/350/gaiaedr3 (Gaia EDR3) obs_collection = Gaia obs_copyright = ESA/Gaia mission/DPAC obs_copyright_url = https://dx.doi.org/10.5270/esa-1ugzkg7 obs_regime = Optical em_min = 3.29283e-7 em_max = 10.42296e-7 client_category = Ancillary/GaiaEDR3 prov_did = ivo://CDS/I/350/gaiaedr3 hips_version = 1.4 hips_frame = equatorial hips_order = 7 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg dataproduct_type = image moc_sky_fraction = 1 hips_creation_date = 2020-11-26T16:37Z hips_release_date = 2020-11-27T12:53Z hips_order_min = 0 dataproduct_subtype = color hips_service_url = https://alasky.cds.unistra.fr/ancillary/GaiaEDR3/color-Rp-G-Bp-flux-map hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/GaiaEDR3/color-Rp-G-Bp-flux-map hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 7 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288487682 ID = CDS/P/DM/flux-color-Rp-G-Bp/I/355/gaiadr3 hips_initial_fov = 130.0 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 creator_did = ivo://CDS/P/DM/flux-color-Rp-G-Bp/I/355/gaiadr3 hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = Color flux map for I/355/gaiadr3 (Gaia DR3) obs_collection = Gaia obs_description = This color flux map has been created from Gaia DR3 individual sources data (fluxes in Rp=red, G=green, Bp=blue filters) obs_copyright = ESA/Gaia mission/DPAC obs_copyright_url = https://doi.org/10.5270/esa-qa4lep3 obs_regime = Optical em_min = 3.29283e-7 em_max = 10.42296e-7 client_category = Ancillary/GaiaDR3 prov_did = ivo://CDS/I/355/gaiadr3 hips_version = 1.4 hips_frame = equatorial hips_order = 7 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg dataproduct_type = image moc_sky_fraction = 1 hips_creation_date = 2022-06-12T16:37Z hips_release_date = 2022-06-16T09:03Z hips_order_min = 0 dataproduct_subtype = color hips_service_url = https://alasky.cds.unistra.fr/ancillary/GaiaDR3/color-Rp-G-Bp-flux-map hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/GaiaDR3/color-Rp-G-Bp-flux-map hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 7 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288487906 ID = CDS/P/DM/radial-velocity/I/345/gaia2 hips_initial_fov = 140 hips_initial_ra = 266.4168330 hips_initial_dec = -29.0078 creator_did = ivo://CDS/P/DM/radial-velocity/I/345/gaia2 hips_creator = Boch T. (CDS) obs_title = Radial velocity map for I/345/gaia2 (Gaia DR2) prov_did = ivo://CDS/I/345/gaia2 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T08:58Z hips_frame = equatorial hips_order = 3 hips_tile_width = 32 hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_bitpix = -32 hips_pixel_cut = -55 60 hips_data_range = -422.4 473.9 hips_pixel_scale = 0.01431 dataproduct_type = image client_category = Ancillary/GaiaDR2 moc_sky_fraction = 1 hips_estsize = 1121512 hipsgen_date = 2018-04-26T21:33Z hipsgen_params = in=density-maps/param-weighted/gaia-DR2-radial-velocity-map.hpx out=density-maps/param-weighted/hips-gaia-DR2-radial-velocity -creator_did=ivo://CDS/P/DM/radial-velocity/I/345/gaia2 "-hips_pixel_cut=0 100000 sqrt" -method=mean MAPTILES hips_creation_date = 2018-04-26T21:33Z hipsgen_date_1 = 2018-04-26T21:40Z hipsgen_params_1 = in=density-maps/param-weighted/gaia-DR2-radial-velocity-map.hpx out=density-maps/param-weighted/hips-gaia-DR2-radial-velocity -creator_did=ivo://CDS/P/DM/radial-velocity/I/345/gaia2 "-hips_pixel_cut=0 100000 sqrt" -method=mean allsky hipsgen_date_2 = 2018-04-26T21:58Z hipsgen_params_2 = in=density-maps/param-weighted/gaia-DR2-radial-velocity-map.hpx out=density-maps/param-weighted/hips-gaia-DR2-radial-velocity -creator_did=ivo://CDS/P/DM/radial-velocity/I/345/gaia2 "-hips_pixel_cut=-55 60" -method=mean MAPTILES JPEG hips_order_min = 0 hipsgen_date_3 = 2018-04-26T21:58Z hipsgen_params_3 = in=density-maps/param-weighted/gaia-DR2-radial-velocity-map.hpx out=density-maps/param-weighted/hips-gaia-DR2-radial-velocity -creator_did=ivo://CDS/P/DM/radial-velocity/I/345/gaia2 "-hips_pixel_cut=-55 60" -method=mean MAPTILES JPEG hipsgen_date_4 = 2018-04-26T22:03Z hipsgen_params_4 = in=density-maps/param-weighted/gaia-DR2-radial-velocity-map.hpx out=density-maps/param-weighted/hips-gaia-DR2-radial-velocity -creator_did=ivo://CDS/P/DM/radial-velocity/I/345/gaia2 "-hips_pixel_cut=-55 60" -method=mean MAPTILES JPEG hipsgen_date_5 = 2018-04-26T22:03Z hipsgen_params_5 = in=density-maps/param-weighted/gaia-DR2-radial-velocity-map.hpx out=density-maps/param-weighted/hips-gaia-DR2-radial-velocity -creator_did=ivo://CDS/P/DM/radial-velocity/I/345/gaia2 "-hips_pixel_cut=-55 60" -method=mean MAPTILES JPEG hipsgen_date_6 = 2019-05-21T08:58Z hipsgen_params_6 = out=/asd-volumes/sc1-asd-volume6/ancillary/GaiaDR2/radial-velocity-map UPDATE hips_service_url = https://alasky.cds.unistra.fr/ancillary/GaiaDR2/radial-velocity-map hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/GaiaDR2/radial-velocity-map hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 7 obs_initial_ra = 266.4168330 obs_initial_dec = -29.0078 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288478702 ID = CDS/P/DM/radial-velocity/I/355/gaiadr3 hips_initial_fov = 130 hips_initial_ra = 266.4168330 hips_initial_dec = -29.0078 creator_did = ivo://CDS/P/DM/radial-velocity/I/355/gaiadr3 hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = Gaia DR3 radial velocity map obs_collection = Gaia obs_copyright = ESA/Gaia mission/DPAC obs_copyright_url = https://doi.org/10.5270/esa-qa4lep3 client_category = Ancillary/GaiaDR3 prov_did = ivo://CDS/I/355/gaiadr3 hips_builder = Aladin/HipsGen v11.071 hips_version = 1.4 hips_release_date = 2022-06-16T11:51Z hips_frame = equatorial hips_order = 3 hips_order_min = 0 hips_tile_width = 256 hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_bitpix = -32 hips_pixel_cut = -60 60 hips_data_range = -1630 1622 hips_pixel_scale = 0.01431 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 1121512 hipsgen_date = 2022-06-16T11:46Z hipsgen_params = in=density-maps/param-weighted/gaia-DR3-radial-velocity-map.hpx creator_did=CDS/P/DM/radial-velocity/I/355/gaiadr3 MAPTILES hips_creation_date = 2022-06-16T11:46Z hipsgen_date_1 = 2022-06-16T11:48Z hipsgen_params_1 = in=density-maps/param-weighted/gaia-DR3-radial-velocity-map.hpx creator_did=CDS/P/DM/radial-velocity/I/355/gaiadr3 "hips_pixel_cut=-60 60" JPEG hipsgen_date_2 = 2022-06-16T11:51Z hipsgen_params_2 = in=density-maps/param-weighted/gaia-DR3-radial-velocity-map.hpx creator_did=CDS/P/DM/radial-velocity/I/355/gaiadr3 "hips_pixel_cut=-60 60" JPEG -f dataproduct_subtype = color hips_service_url = https://alasky.cds.unistra.fr/ancillary/GaiaDR3/radial-velocity hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/GaiaDR3/radial-velocity hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 7 obs_initial_ra = 266.4168330 obs_initial_dec = -29.0078 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288488158 ID = CDS/P/DM/simbad-biblio/allObjects client_category = Ancillary/Simbad bibliography hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 330.0 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 creator_did = ivo://CDS/P/DM/simbad-biblio/allObjects hips_creator = CDS obs_title = Simbad heatmap - all objects obs_description = This is the density map of objects in SIMBAD database, weighted by the number of citations, as of January 2023 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:49Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = 0.7382 115.7 hips_data_range = -6740 20221 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:49Z hipsgen_params = "title=Simbad heatmap - all objects" "creator=CDS Simbad" "pixelCut=0.738188 115.651042 sqrt" id=ivo://CDS/P/DM/simbad-biblio/allObjects in=/tmp/tmpjik2thj7 out=/var/www/hips-simbad/data/simbad-biblio/allObjects mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:49Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/allObjects hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/allObjects hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288482522 ID = CDS/P/DM/simbad-biblio/otypes/Galaxy client_category = Ancillary/Simbad bibliography/By object types hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/otypes/Galaxy hips_creator = CDS obs_title = Simbad heatmap - Galaxy hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:50Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -0.001503 32.48 hips_data_range = -5591 16772 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:50Z hipsgen_params = "title=Simbad heatmap - Galaxy" "creator=CDS Simbad" "pixelCut=-0.001503 32.476658 sqrt" id=ivo://CDS/P/DM/simbad-biblio/otypes/Galaxy in=/tmp/tmpev142kln out=/var/www/hips-simbad/data/simbad-biblio/Galaxy mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:50Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/Galaxy hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/Galaxy hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288482574 ID = CDS/P/DM/simbad-biblio/otypes/HII client_category = Ancillary/Simbad bibliography/By object types hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/otypes/HII hips_creator = CDS obs_title = Simbad heatmap - HII hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:51Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -0.003484 2 hips_data_range = -119.9 359.5 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:50Z hipsgen_params = "title=Simbad heatmap - HII" "creator=CDS Simbad" "pixelCut=-0.003484 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/otypes/HII in=/tmp/tmpw3j8qpc8 out=/var/www/hips-simbad/data/simbad-biblio/HII mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:50Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/HII hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/HII hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288482630 ID = CDS/P/DM/simbad-biblio/otypes/Infrared client_category = Ancillary/Simbad bibliography/By object types hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/otypes/Infrared hips_creator = CDS obs_title = Simbad heatmap - Infrared hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:51Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -5.12E-4 2 hips_data_range = -53.72 161.1 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:51Z hipsgen_params = "title=Simbad heatmap - Infrared" "creator=CDS Simbad" "pixelCut=-0.000512 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/otypes/Infrared in=/tmp/tmphvjrp9ll out=/var/www/hips-simbad/data/simbad-biblio/Infrared mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:51Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/Infrared hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/Infrared hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288482698 ID = CDS/P/DM/simbad-biblio/otypes/Nebula client_category = Ancillary/Simbad bibliography/By object types hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/otypes/Nebula hips_creator = CDS obs_title = Simbad heatmap - Nebula hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:50Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -0.00518 2.42 hips_data_range = -294.2 882.4 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:50Z hipsgen_params = "title=Simbad heatmap - Nebula" "creator=CDS Simbad" "pixelCut=-0.005180 2.419778 sqrt" id=ivo://CDS/P/DM/simbad-biblio/otypes/Nebula in=/tmp/tmpcjjd7fal out=/var/www/hips-simbad/data/simbad-biblio/Nebula mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:50Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/Nebula hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/Nebula hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288482758 ID = CDS/P/DM/simbad-biblio/otypes/Other client_category = Ancillary/Simbad bibliography/By object types hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/otypes/Other hips_creator = CDS obs_title = Simbad heatmap - Other hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:52Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = 0.01793 28.15 hips_data_range = -1086 3257 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:52Z hipsgen_params = "title=Simbad heatmap - Other" "creator=CDS Simbad" "pixelCut=0.017935 28.153819 sqrt" id=ivo://CDS/P/DM/simbad-biblio/otypes/Other in=/tmp/tmpggfhna8c out=/var/www/hips-simbad/data/simbad-biblio/Other mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:52Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/Other hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/Other hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288482814 ID = CDS/P/DM/simbad-biblio/otypes/Radio client_category = Ancillary/Simbad bibliography/By object types hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/otypes/Radio hips_creator = CDS obs_title = Simbad heatmap - Radio hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:51Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -1.35E-4 2 hips_data_range = -5.294 15.88 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:51Z hipsgen_params = "title=Simbad heatmap - Radio" "creator=CDS Simbad" "pixelCut=-0.000135 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/otypes/Radio in=/tmp/tmp7ug5nbhc out=/var/www/hips-simbad/data/simbad-biblio/Radio mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:51Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/Radio hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/Radio hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288482942 ID = CDS/P/DM/simbad-biblio/otypes/Star client_category = Ancillary/Simbad bibliography/By object types hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/otypes/Star hips_creator = CDS obs_title = Simbad heatmap - Star hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:50Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = 0.2524 81.76 hips_data_range = -2066 6198 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:50Z hipsgen_params = "title=Simbad heatmap - Star" "creator=CDS Simbad" "pixelCut=0.252396 81.762224 sqrt" id=ivo://CDS/P/DM/simbad-biblio/otypes/Star in=/tmp/tmph5nijqlx out=/var/www/hips-simbad/data/simbad-biblio/Star mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:50Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/Star hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/Star hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288483002 ID = CDS/P/DM/simbad-biblio/otypes/UV client_category = Ancillary/Simbad bibliography/By object types hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/otypes/UV hips_creator = CDS obs_title = Simbad heatmap - UV hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:52Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -1.46E-4 2 hips_data_range = -9.012 27.02 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:52Z hipsgen_params = "title=Simbad heatmap - UV" "creator=CDS Simbad" "pixelCut=-0.000146 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/otypes/UV in=/tmp/tmp0csofnol out=/var/www/hips-simbad/data/simbad-biblio/UV mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:52Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/UV hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/UV hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288483054 ID = CDS/P/DM/simbad-biblio/otypes/X client_category = Ancillary/Simbad bibliography/By object types hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/otypes/X hips_creator = CDS obs_title = Simbad heatmap - X hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:51Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -0.001509 2 hips_data_range = -362.4 1087 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:51Z hipsgen_params = "title=Simbad heatmap - X" "creator=CDS Simbad" "pixelCut=-0.001509 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/otypes/X in=/tmp/tmpfwvor7pf out=/var/www/hips-simbad/data/simbad-biblio/X mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:51Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/X hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/X hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288483114 ID = CDS/P/DM/simbad-biblio/pub-dates/1850-1900 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1850-1900 hips_creator = CDS obs_title = Simbad heatmap - 1850-1900 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:52Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -4.6E-5 2 hips_data_range = -1.927 5.779 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:52Z hipsgen_params = "title=Simbad heatmap - 1850-1900" "creator=CDS Simbad" "pixelCut=-0.000046 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1850-1900 in=/tmp/tmpgu_eqy7e out=/var/www/hips-simbad/data/simbad-biblio/1850-1900 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:52Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1850-1900 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1850-1900 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288479626 ID = CDS/P/DM/simbad-biblio/pub-dates/1900-1910 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1900-1910 hips_creator = CDS obs_title = Simbad heatmap - 1900-1910 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:52Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -3.27E-4 2 hips_data_range = -51.66 155 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:52Z hipsgen_params = "title=Simbad heatmap - 1900-1910" "creator=CDS Simbad" "pixelCut=-0.000327 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1900-1910 in=/tmp/tmp9hr65lc1 out=/var/www/hips-simbad/data/simbad-biblio/1900-1910 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:52Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1900-1910 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1900-1910 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288479682 ID = CDS/P/DM/simbad-biblio/pub-dates/1910-1920 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1910-1920 hips_creator = CDS obs_title = Simbad heatmap - 1910-1920 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:53Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -9.3E-5 2 hips_data_range = -4.966 14.9 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:53Z hipsgen_params = "title=Simbad heatmap - 1910-1920" "creator=CDS Simbad" "pixelCut=-0.000093 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1910-1920 in=/tmp/tmpgyarms2p out=/var/www/hips-simbad/data/simbad-biblio/1910-1920 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:53Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1910-1920 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1910-1920 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288479734 ID = CDS/P/DM/simbad-biblio/pub-dates/1920-1930 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1920-1930 hips_creator = CDS obs_title = Simbad heatmap - 1920-1930 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:53Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -8.6E-5 2 hips_data_range = -6.973 20.92 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:53Z hipsgen_params = "title=Simbad heatmap - 1920-1930" "creator=CDS Simbad" "pixelCut=-0.000086 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1920-1930 in=/tmp/tmp3bb0ucv_ out=/var/www/hips-simbad/data/simbad-biblio/1920-1930 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:53Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1920-1930 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1920-1930 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288479786 ID = CDS/P/DM/simbad-biblio/pub-dates/1930-1940 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1930-1940 hips_creator = CDS obs_title = Simbad heatmap - 1930-1940 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:53Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -1.32E-4 2 hips_data_range = -18.94 56.83 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:53Z hipsgen_params = "title=Simbad heatmap - 1930-1940" "creator=CDS Simbad" "pixelCut=-0.000132 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1930-1940 in=/tmp/tmps4y3jd77 out=/var/www/hips-simbad/data/simbad-biblio/1930-1940 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:53Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1930-1940 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1930-1940 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288479838 ID = CDS/P/DM/simbad-biblio/pub-dates/1940-1945 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1940-1945 hips_creator = CDS obs_title = Simbad heatmap - 1940-1945 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:54Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -5.7E-5 2 hips_data_range = -4.872 14.61 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:53Z hipsgen_params = "title=Simbad heatmap - 1940-1945" "creator=CDS Simbad" "pixelCut=-0.000057 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1940-1945 in=/tmp/tmp0k5eaf2h out=/var/www/hips-simbad/data/simbad-biblio/1940-1945 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:53Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1940-1945 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1940-1945 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288479894 ID = CDS/P/DM/simbad-biblio/pub-dates/1945-1950 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1945-1950 hips_creator = CDS obs_title = Simbad heatmap - 1945-1950 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:54Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -7.4E-5 2 hips_data_range = -2.683 8.047 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:54Z hipsgen_params = "title=Simbad heatmap - 1945-1950" "creator=CDS Simbad" "pixelCut=-0.000074 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1945-1950 in=/tmp/tmpg84wi_za out=/var/www/hips-simbad/data/simbad-biblio/1945-1950 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:54Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1945-1950 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1945-1950 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288479958 ID = CDS/P/DM/simbad-biblio/pub-dates/1950-1955 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1950-1955 hips_creator = CDS obs_title = Simbad heatmap - 1950-1955 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:54Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -3.11E-4 2 hips_data_range = -21.57 64.69 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:54Z hipsgen_params = "title=Simbad heatmap - 1950-1955" "creator=CDS Simbad" "pixelCut=-0.000311 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1950-1955 in=/tmp/tmpo22tccn4 out=/var/www/hips-simbad/data/simbad-biblio/1950-1955 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:54Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1950-1955 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1950-1955 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288480026 ID = CDS/P/DM/simbad-biblio/pub-dates/1955-1960 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1955-1960 hips_creator = CDS obs_title = Simbad heatmap - 1955-1960 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:54Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -3.49E-4 2 hips_data_range = -14.76 44.26 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:54Z hipsgen_params = "title=Simbad heatmap - 1955-1960" "creator=CDS Simbad" "pixelCut=-0.000349 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1955-1960 in=/tmp/tmpq0k71l_x out=/var/www/hips-simbad/data/simbad-biblio/1955-1960 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:54Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1955-1960 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1955-1960 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288480086 ID = CDS/P/DM/simbad-biblio/pub-dates/1960-1965 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1960-1965 hips_creator = CDS obs_title = Simbad heatmap - 1960-1965 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:55Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -3.75E-4 2 hips_data_range = -19.37 58.11 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:55Z hipsgen_params = "title=Simbad heatmap - 1960-1965" "creator=CDS Simbad" "pixelCut=-0.000375 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1960-1965 in=/tmp/tmpoo1x1eho out=/var/www/hips-simbad/data/simbad-biblio/1960-1965 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:55Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1960-1965 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1960-1965 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288480138 ID = CDS/P/DM/simbad-biblio/pub-dates/1965-1970 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1965-1970 hips_creator = CDS obs_title = Simbad heatmap - 1965-1970 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:55Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -4.88E-4 2 hips_data_range = -17.61 52.81 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:55Z hipsgen_params = "title=Simbad heatmap - 1965-1970" "creator=CDS Simbad" "pixelCut=-0.000488 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1965-1970 in=/tmp/tmpqbth1q74 out=/var/www/hips-simbad/data/simbad-biblio/1965-1970 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:55Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1965-1970 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1965-1970 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288480190 ID = CDS/P/DM/simbad-biblio/pub-dates/1970-1975 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1970-1975 hips_creator = CDS obs_title = Simbad heatmap - 1970-1975 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:55Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -6.15E-4 2 hips_data_range = -16.25 48.73 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:55Z hipsgen_params = "title=Simbad heatmap - 1970-1975" "creator=CDS Simbad" "pixelCut=-0.000615 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1970-1975 in=/tmp/tmpcp01n1kz out=/var/www/hips-simbad/data/simbad-biblio/1970-1975 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:55Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1970-1975 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1970-1975 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288480242 ID = CDS/P/DM/simbad-biblio/pub-dates/1975-1980 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1975-1980 hips_creator = CDS obs_title = Simbad heatmap - 1975-1980 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:56Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -5.62E-4 2 hips_data_range = -67.22 201.6 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:55Z hipsgen_params = "title=Simbad heatmap - 1975-1980" "creator=CDS Simbad" "pixelCut=-0.000562 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1975-1980 in=/tmp/tmp8soiuxz9 out=/var/www/hips-simbad/data/simbad-biblio/1975-1980 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:55Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1975-1980 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1975-1980 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288480306 ID = CDS/P/DM/simbad-biblio/pub-dates/1980-1985 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1980-1985 hips_creator = CDS obs_title = Simbad heatmap - 1980-1985 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:56Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -9.2E-4 2.305 hips_data_range = -41.75 125.2 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:56Z hipsgen_params = "title=Simbad heatmap - 1980-1985" "creator=CDS Simbad" "pixelCut=-0.000920 2.304875 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1980-1985 in=/tmp/tmpxbg5v1lu out=/var/www/hips-simbad/data/simbad-biblio/1980-1985 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:56Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1980-1985 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1980-1985 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288480362 ID = CDS/P/DM/simbad-biblio/pub-dates/1985-1990 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1985-1990 hips_creator = CDS obs_title = Simbad heatmap - 1985-1990 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:56Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -0.001041 3.456 hips_data_range = -79.09 237.2 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:56Z hipsgen_params = "title=Simbad heatmap - 1985-1990" "creator=CDS Simbad" "pixelCut=-0.001041 3.455914 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1985-1990 in=/tmp/tmpcj4cx4ad out=/var/www/hips-simbad/data/simbad-biblio/1985-1990 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:56Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1985-1990 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1985-1990 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288480418 ID = CDS/P/DM/simbad-biblio/pub-dates/1991 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1991 hips_creator = CDS obs_title = Simbad heatmap - 1991 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:56Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -4.47E-4 2 hips_data_range = -19.13 57.38 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:56Z hipsgen_params = "title=Simbad heatmap - 1991" "creator=CDS Simbad" "pixelCut=-0.000447 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1991 in=/tmp/tmpkr2te4cc out=/var/www/hips-simbad/data/simbad-biblio/1991 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:56Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1991 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1991 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288480478 ID = CDS/P/DM/simbad-biblio/pub-dates/1992 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1992 hips_creator = CDS obs_title = Simbad heatmap - 1992 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:57Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -5.57E-4 2 hips_data_range = -22.02 66 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:57Z hipsgen_params = "title=Simbad heatmap - 1992" "creator=CDS Simbad" "pixelCut=-0.000557 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1992 in=/tmp/tmput4vlc2e out=/var/www/hips-simbad/data/simbad-biblio/1992 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:57Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1992 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1992 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288480654 ID = CDS/P/DM/simbad-biblio/pub-dates/1993 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1993 hips_creator = CDS obs_title = Simbad heatmap - 1993 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:57Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -1.2E-5 2 hips_data_range = -79.58 238.7 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:57Z hipsgen_params = "title=Simbad heatmap - 1993" "creator=CDS Simbad" "pixelCut=-0.000012 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1993 in=/tmp/tmpzypxgrpj out=/var/www/hips-simbad/data/simbad-biblio/1993 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:57Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1993 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1993 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288480786 ID = CDS/P/DM/simbad-biblio/pub-dates/1994 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1994 hips_creator = CDS obs_title = Simbad heatmap - 1994 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:57Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -6.86E-4 2 hips_data_range = -45.11 135.3 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:57Z hipsgen_params = "title=Simbad heatmap - 1994" "creator=CDS Simbad" "pixelCut=-0.000686 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1994 in=/tmp/tmp2jzuik2x out=/var/www/hips-simbad/data/simbad-biblio/1994 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:57Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1994 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1994 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288480838 ID = CDS/P/DM/simbad-biblio/pub-dates/1995 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1995 hips_creator = CDS obs_title = Simbad heatmap - 1995 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:58Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -4.51E-4 2 hips_data_range = -75.96 227.8 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:57Z hipsgen_params = "title=Simbad heatmap - 1995" "creator=CDS Simbad" "pixelCut=-0.000451 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1995 in=/tmp/tmps8b3ysch out=/var/www/hips-simbad/data/simbad-biblio/1995 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:57Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1995 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1995 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288480898 ID = CDS/P/DM/simbad-biblio/pub-dates/1996 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1996 hips_creator = CDS obs_title = Simbad heatmap - 1996 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:58Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -0.001119 2.156 hips_data_range = -72.28 216.8 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:58Z hipsgen_params = "title=Simbad heatmap - 1996" "creator=CDS Simbad" "pixelCut=-0.001119 2.156105 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1996 in=/tmp/tmpcifotf6t out=/var/www/hips-simbad/data/simbad-biblio/1996 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:58Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1996 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1996 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288480954 ID = CDS/P/DM/simbad-biblio/pub-dates/1997 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1997 hips_creator = CDS obs_title = Simbad heatmap - 1997 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:58Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -8.46E-4 2.063 hips_data_range = -86.36 259 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:58Z hipsgen_params = "title=Simbad heatmap - 1997" "creator=CDS Simbad" "pixelCut=-0.000846 2.062980 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1997 in=/tmp/tmpjrbbxgfw out=/var/www/hips-simbad/data/simbad-biblio/1997 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:58Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1997 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1997 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288481010 ID = CDS/P/DM/simbad-biblio/pub-dates/1998 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1998 hips_creator = CDS obs_title = Simbad heatmap - 1998 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:58Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -7.19E-4 2 hips_data_range = -108.9 326.7 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:58Z hipsgen_params = "title=Simbad heatmap - 1998" "creator=CDS Simbad" "pixelCut=-0.000719 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1998 in=/tmp/tmpfr1nrqmv out=/var/www/hips-simbad/data/simbad-biblio/1998 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:58Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1998 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1998 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288481066 ID = CDS/P/DM/simbad-biblio/pub-dates/1999 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/1999 hips_creator = CDS obs_title = Simbad heatmap - 1999 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:59Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -7.27E-4 2 hips_data_range = -50.53 151.6 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:59Z hipsgen_params = "title=Simbad heatmap - 1999" "creator=CDS Simbad" "pixelCut=-0.000727 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/1999 in=/tmp/tmphwk8m84k out=/var/www/hips-simbad/data/simbad-biblio/1999 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:59Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/1999 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/1999 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288481118 ID = CDS/P/DM/simbad-biblio/pub-dates/2000 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2000 hips_creator = CDS obs_title = Simbad heatmap - 2000 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:59Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -0.001147 2 hips_data_range = -103.6 310.9 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:59Z hipsgen_params = "title=Simbad heatmap - 2000" "creator=CDS Simbad" "pixelCut=-0.001147 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2000 in=/tmp/tmpg2w8hfht out=/var/www/hips-simbad/data/simbad-biblio/2000 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:59Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2000 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2000 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288481170 ID = CDS/P/DM/simbad-biblio/pub-dates/2001 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2001 hips_creator = CDS obs_title = Simbad heatmap - 2001 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T07:59Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -0.001362 3.033 hips_data_range = -84.54 253.6 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:59Z hipsgen_params = "title=Simbad heatmap - 2001" "creator=CDS Simbad" "pixelCut=-0.001362 3.032577 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2001 in=/tmp/tmpemryilmx out=/var/www/hips-simbad/data/simbad-biblio/2001 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:59Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2001 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2001 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288481230 ID = CDS/P/DM/simbad-biblio/pub-dates/2002 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2002 hips_creator = CDS obs_title = Simbad heatmap - 2002 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:00Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -0.001096 2 hips_data_range = -178.9 536.7 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T07:59Z hipsgen_params = "title=Simbad heatmap - 2002" "creator=CDS Simbad" "pixelCut=-0.001096 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2002 in=/tmp/tmpej96bbt0 out=/var/www/hips-simbad/data/simbad-biblio/2002 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T07:59Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2002 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2002 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288481282 ID = CDS/P/DM/simbad-biblio/pub-dates/2003 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2003 hips_creator = CDS obs_title = Simbad heatmap - 2003 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:00Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -1.7E-5 3.738 hips_data_range = -344.1 1032 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T08:00Z hipsgen_params = "title=Simbad heatmap - 2003" "creator=CDS Simbad" "pixelCut=-0.000017 3.738499 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2003 in=/tmp/tmpg524ypft out=/var/www/hips-simbad/data/simbad-biblio/2003 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T08:00Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2003 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2003 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288481338 ID = CDS/P/DM/simbad-biblio/pub-dates/2004 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2004 hips_creator = CDS obs_title = Simbad heatmap - 2004 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:00Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -9.76E-4 2.919 hips_data_range = -209.4 628 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T08:00Z hipsgen_params = "title=Simbad heatmap - 2004" "creator=CDS Simbad" "pixelCut=-0.000976 2.918503 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2004 in=/tmp/tmprbtor3wi out=/var/www/hips-simbad/data/simbad-biblio/2004 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T08:00Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2004 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2004 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288481390 ID = CDS/P/DM/simbad-biblio/pub-dates/2005 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. 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All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2006 hips_creator = CDS obs_title = Simbad heatmap - 2006 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:01Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -8.1E-4 2.106 hips_data_range = -425.5 1276 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T08:01Z hipsgen_params = "title=Simbad heatmap - 2006" "creator=CDS Simbad" "pixelCut=-0.000810 2.105847 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2006 in=/tmp/tmpv1ap8q4s out=/var/www/hips-simbad/data/simbad-biblio/2006 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T08:01Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2006 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2006 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288481494 ID = CDS/P/DM/simbad-biblio/pub-dates/2007 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2007 hips_creator = CDS obs_title = Simbad heatmap - 2007 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:01Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -7.98E-4 2 hips_data_range = -140.3 420.7 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T08:01Z hipsgen_params = "title=Simbad heatmap - 2007" "creator=CDS Simbad" "pixelCut=-0.000798 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2007 in=/tmp/tmpn457wft2 out=/var/www/hips-simbad/data/simbad-biblio/2007 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T08:01Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2007 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2007 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288481546 ID = CDS/P/DM/simbad-biblio/pub-dates/2008 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2008 hips_creator = CDS obs_title = Simbad heatmap - 2008 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:01Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -9.21E-4 2.845 hips_data_range = -164.8 494.3 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T08:01Z hipsgen_params = "title=Simbad heatmap - 2008" "creator=CDS Simbad" "pixelCut=-0.000921 2.845083 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2008 in=/tmp/tmppp9zthbf out=/var/www/hips-simbad/data/simbad-biblio/2008 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T08:01Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2008 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2008 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288481598 ID = CDS/P/DM/simbad-biblio/pub-dates/2009 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2009 hips_creator = CDS obs_title = Simbad heatmap - 2009 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:02Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -2.63E-4 3.996 hips_data_range = -199.2 597.4 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T08:01Z hipsgen_params = "title=Simbad heatmap - 2009" "creator=CDS Simbad" "pixelCut=-0.000263 3.996111 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2009 in=/tmp/tmp2m18srlp out=/var/www/hips-simbad/data/simbad-biblio/2009 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T08:01Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2009 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2009 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288481690 ID = CDS/P/DM/simbad-biblio/pub-dates/2010 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2010 hips_creator = CDS obs_title = Simbad heatmap - 2010 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:02Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -2.47E-4 4.353 hips_data_range = -219.4 658.3 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T08:02Z hipsgen_params = "title=Simbad heatmap - 2010" "creator=CDS Simbad" "pixelCut=-0.000247 4.352876 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2010 in=/tmp/tmpbcr3vw5s out=/var/www/hips-simbad/data/simbad-biblio/2010 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T08:02Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2010 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2010 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288481802 ID = CDS/P/DM/simbad-biblio/pub-dates/2011 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2011 hips_creator = CDS obs_title = Simbad heatmap - 2011 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:02Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -6.2E-5 6.14 hips_data_range = -359.6 1079 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T08:02Z hipsgen_params = "title=Simbad heatmap - 2011" "creator=CDS Simbad" "pixelCut=-0.000062 6.140479 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2011 in=/tmp/tmp67w8cjid out=/var/www/hips-simbad/data/simbad-biblio/2011 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T08:02Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2011 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2011 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288481858 ID = CDS/P/DM/simbad-biblio/pub-dates/2012 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2012 hips_creator = CDS obs_title = Simbad heatmap - 2012 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:02Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = 2.0E-6 2.933 hips_data_range = -246.6 739.9 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T08:02Z hipsgen_params = "title=Simbad heatmap - 2012" "creator=CDS Simbad" "pixelCut=0.000002 2.932784 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2012 in=/tmp/tmp8nql7750 out=/var/www/hips-simbad/data/simbad-biblio/2012 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T08:02Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2012 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2012 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288481914 ID = CDS/P/DM/simbad-biblio/pub-dates/2013 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2013 hips_creator = CDS obs_title = Simbad heatmap - 2013 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:03Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -5.13E-4 5.9 hips_data_range = -2132 6395 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T08:03Z hipsgen_params = "title=Simbad heatmap - 2013" "creator=CDS Simbad" "pixelCut=-0.000513 5.900180 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2013 in=/tmp/tmpo68tojd_ out=/var/www/hips-simbad/data/simbad-biblio/2013 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T08:03Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2013 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2013 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288481970 ID = CDS/P/DM/simbad-biblio/pub-dates/2014 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2014 hips_creator = CDS obs_title = Simbad heatmap - 2014 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:03Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -6.2E-5 5.551 hips_data_range = -949.1 2847 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T08:03Z hipsgen_params = "title=Simbad heatmap - 2014" "creator=CDS Simbad" "pixelCut=-0.000062 5.551417 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2014 in=/tmp/tmp5mdmd369 out=/var/www/hips-simbad/data/simbad-biblio/2014 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T08:03Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2014 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2014 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288482026 ID = CDS/P/DM/simbad-biblio/pub-dates/2015 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2015 hips_creator = CDS obs_title = Simbad heatmap - 2015 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:03Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -4.57E-4 8.632 hips_data_range = -802 2406 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T08:03Z hipsgen_params = "title=Simbad heatmap - 2015" "creator=CDS Simbad" "pixelCut=-0.000457 8.632473 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2015 in=/tmp/tmpa0l9mxoc out=/var/www/hips-simbad/data/simbad-biblio/2015 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T08:03Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2015 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2015 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288482078 ID = CDS/P/DM/simbad-biblio/pub-dates/2016 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2016 hips_creator = CDS obs_title = Simbad heatmap - 2016 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:04Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -3.5E-5 14.17 hips_data_range = -1179 3537 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T08:03Z hipsgen_params = "title=Simbad heatmap - 2016" "creator=CDS Simbad" "pixelCut=-0.000035 14.167781 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2016 in=/tmp/tmpm3vzca59 out=/var/www/hips-simbad/data/simbad-biblio/2016 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T08:03Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2016 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2016 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288482130 ID = CDS/P/DM/simbad-biblio/pub-dates/2017 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2017 hips_creator = CDS obs_title = Simbad heatmap - 2017 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:04Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -9.4E-5 5.891 hips_data_range = -1350 4050 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T08:04Z hipsgen_params = "title=Simbad heatmap - 2017" "creator=CDS Simbad" "pixelCut=-0.000094 5.891159 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2017 in=/tmp/tmp7ubi7h3v out=/var/www/hips-simbad/data/simbad-biblio/2017 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T08:04Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2017 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2017 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288482186 ID = CDS/P/DM/simbad-biblio/pub-dates/2018 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2018 hips_creator = CDS obs_title = Simbad heatmap - 2018 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:04Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = 0.01091 10.62 hips_data_range = -510.9 1533 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T08:04Z hipsgen_params = "title=Simbad heatmap - 2018" "creator=CDS Simbad" "pixelCut=0.010910 10.624367 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2018 in=/tmp/tmpr1dk8t0f out=/var/www/hips-simbad/data/simbad-biblio/2018 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T08:04Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2018 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2018 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288482246 ID = CDS/P/DM/simbad-biblio/pub-dates/2019 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2019 hips_creator = CDS obs_title = Simbad heatmap - 2019 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:04Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = 0.05744 5.57 hips_data_range = -350.8 1052 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T08:04Z hipsgen_params = "title=Simbad heatmap - 2019" "creator=CDS Simbad" "pixelCut=0.057436 5.569919 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2019 in=/tmp/tmp8sklyik6 out=/var/www/hips-simbad/data/simbad-biblio/2019 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T08:04Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2019 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2019 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288482306 ID = CDS/P/DM/simbad-biblio/pub-dates/2020 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2020 hips_creator = CDS obs_title = Simbad heatmap - 2020 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:05Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -1.32E-4 10.06 hips_data_range = -167.1 501.1 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T08:05Z hipsgen_params = "title=Simbad heatmap - 2020" "creator=CDS Simbad" "pixelCut=-0.000132 10.063485 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2020 in=/tmp/tmpxev6ivl5 out=/var/www/hips-simbad/data/simbad-biblio/2020 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T08:05Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2020 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2020 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288482362 ID = CDS/P/DM/simbad-biblio/pub-dates/2021 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2021 hips_creator = CDS obs_title = Simbad heatmap - 2021 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:05Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -1.4E-5 8.185 hips_data_range = -232.3 696.8 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T08:05Z hipsgen_params = "title=Simbad heatmap - 2021" "creator=CDS Simbad" "pixelCut=-0.000014 8.185436 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2021 in=/tmp/tmp4ytxr_4q out=/var/www/hips-simbad/data/simbad-biblio/2021 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T08:05Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2021 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2021 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288482414 ID = CDS/P/DM/simbad-biblio/pub-dates/2022 client_category = Ancillary/Simbad bibliography/By publication dates hips_copyright = © Université de Strasbourg - CNRS. All rights reserved obs_copyright = © Université de Strasbourg - CNRS. All rights reserved hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/DM/simbad-biblio/pub-dates/2022 hips_creator = CDS obs_title = Simbad heatmap - 2022 hips_builder = Aladin/HipsGen v12.032 hips_version = 1.4 hips_release_date = 2023-01-30T08:05Z hips_frame = equatorial hips_order = 3 hips_tile_width = 64 hips_status = public master unclonable hips_tile_format = fits png hips_pixel_bitpix = -64 hips_pixel_cut = -0.001042 2 hips_data_range = -71.67 215 hips_pixel_scale = 0.1145 dataproduct_type = image hipsgen_date = 2023-01-30T08:05Z hipsgen_params = "title=Simbad heatmap - 2022" "creator=CDS Simbad" "pixelCut=-0.001042 2.000000 sqrt" id=ivo://CDS/P/DM/simbad-biblio/pub-dates/2022 in=/tmp/tmp_1mfw_35 out=/var/www/hips-simbad/data/simbad-biblio/2022 mode=OVERWRITE MAPTILES PNG hips_creation_date = 2023-01-30T08:05Z hips_service_url = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/2022 hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/2022 hips_status_1 = public mirror unclonable moc_type = smoc moc_sky_fraction = 1 moc_order = 7 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288482466 ID = CDS/P/DM/vizMine hips_initial_fov = 330 hips_initial_ra = 266.4168333 hips_initial_dec = -29.0078055 creator_did = ivo://CDS/P/DM/vizMine hips_creator = Boch T. (CDS) obs_title = vizMine: density map for all VizieR tables obs_collection = VizieR obs_description = This HiPS is a density maps of the positions of all rows available in the VizieR database client_category = Ancillary/VizieR vizMine hips_builder = Aladin/HipsGen v10.138 hips_version = 1.4 hips_release_date = 2019-11-08T07:58Z hips_frame = equatorial hips_order = 3 hips_order_min = 0 hips_tile_width = 256 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_bitpix = 32 hips_pixel_cut = 0 9000 hips_data_range = -332295 996917 hips_pixel_scale = 0.02863 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 284289 hipsgen_date = 2019-11-08T07:30Z hipsgen_params = in=/home/boch/FootprintService/generation-scripts/vizMine_2048.hpx out=/var/www/ancillary/vizier/vizMine creator_did=ivo://CDS/P/DM/vizMine "-hips_creator=T. Boch (CDS)" "-obs_title=vizMine: density map for all VizieR tables" "-hips_pixel_cut=0 9000 log" hips_creation_date = 2019-11-08T07:30Z hipsgen_date_1 = 2019-11-08T07:49Z hipsgen_params_1 = in=/home/boch/FootprintService/generation-scripts/vizMine_2048.hpx out=/var/www/ancillary/vizier/vizMine creator_did=ivo://CDS/P/DM/vizMine "-hips_creator=T. Boch (CDS)" "-obs_title=vizMine: density map for all VizieR tables" "-hips_pixel_cut=0 9000 log" hipsgen_date_2 = 2019-11-08T07:58Z hipsgen_params_2 = in=/home/boch/FootprintService/generation-scripts/vizMine_2048.hpx out=/var/www/ancillary/vizier/vizMine creator_did=ivo://CDS/P/DM/vizMine "-hips_creator=T. Boch (CDS)" "-obs_title=vizMine: density map for all VizieR tables" "-hips_pixel_cut=0 9000 log" hips_service_url = https://alasky.cds.unistra.fr/ancillary/vizier/vizMine hips_service_url_1 = https://alaskybis.cds.unistra.fr/ancillary/vizier/vizMine hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 7 obs_initial_ra = 266.4168333 obs_initial_dec = -29.0078055 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288498838 ID = CDS/P/DSS2/NIR hips_doi = 10.26093/cds/aladin/3hh0-7dk creator_did = ivo://CDS/P/DSS2/NIR obs_collection = DSS2 NIR (XI+IS) obs_title = DSS2 NIR (XI+IS) obs_description = The Catalogs and Surveys Group of the Space Telescope Science Institute has digitized the photographic Sky survey plates from the Palomar and UK Schmidt telescopes to produce the "Digitized Sky Survey"(DSS). Each plate covers 6.5 x 6.5 degrees of the sky and have been digitized using a modified PDS microdensitometer. The DSS NIT HiPS is a combination of DSS2-XI and DSS2-IS. DSS2-XI north is the digitalization of the POSS-II N (1987-2002 - filter: IV-N +RG9) from Caltech, DSS2-IS south is the digitalization of the SERC-IS (1990-2002 - filter: IV-N +RG175). The all-sky HEALPix resampling has been done by the CDS with the help of CADC. obs_ack = The Digitized Sky Surveys were produced at the Space Telescope Science Institute under U.S. Government grant NAG W-2166. The images of these surveys are based on photographic data obtained using the Oschin Schmidt Telescope on Palomar Mountain and the UK Schmidt Telescope. The plates were processed into the present compressed digital form with the permission of these institutions. The National Geographic Society - Palomar Observatory Sky Atlas (POSS-I) was made by the California Institute of Technology with grants from the National Geographic Society. The Second Palomar Observatory Sky Survey (POSS-II) was made by the California Institute of Technology with funds from the National Science Foundation, the National Geographic Society, the Sloan Foundation, the Samuel Oschin Foundation, and the Eastman Kodak Corporation. The Oschin Schmidt Telescope is operated by the California Institute of Technology and Palomar Observatory. The UK Schmidt Telescope was operated by the Royal Observatory Edinburgh, with funding from the UK Science and Engineering Research Council (later the UK Particle Physics and Astronomy Research Council), until 1988 June, and thereafter by the Anglo-Australian Observatory. The blue plates of the southern Sky Atlas and its Equatorial Extension (together known as the SERC-J), as well as the Equatorial Red (ER), and the Second Epoch [red] Survey (SES) were all taken with the UK Schmidt. Supplemental funding for sky-survey work at the ST ScI is provided by the European Southern Observatory. prov_progenitor = STScI bib_reference = 1996ASPC..101...88L bib_reference_url = http://cdsads.u-strasbg.fr/abs/1996ASPC..101...88L obs_copyright = Digitized Sky Survey - STScI/NASA, Healpixed by CDS obs_copyright_url = http://archive.stsci.edu/dss/copyright.html client_category = Image/Optical/DSS client_sort_key = 03-01-03a t_min = 46796 t_max = 52620 em_min = 7E-7 em_max = 9.5E-7 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-20T15:03Z hips_creator = Fernique P. (CDS) hips_frame = equatorial hips_order = 9 hips_tile_width = 512 hips_status = public master clonableOnce hips_hierarchy = mean hips_pixel_scale = 2.236E-4 dataproduct_type = image moc_sky_fraction = 0.9955 hips_creation_date = 2015-09-08T12:14Z hips_tile_format = jpeg fits hips_pixel_bitpix = 16 data_pixel_bitpix = 16 hips_pixel_cut = 1249 10940 hips_data_range = -11612 34834 hips_initial_ra = 200.0641577 hips_initial_dec = -62.0757716 hips_initial_fov = 30.0 s_pixel_scale = 2.798E-4 obs_regime = Optical hips_copyright = CNRS/Unistra hips_order_min = 0 hips_estsize = 2328304001 hipsgen_date = 2019-05-20T15:03Z hipsgen_params = out=/asd-volumes/sc1-asd-volume6/DSS/DSS2-NIR UPDATE hips_service_url = https://alasky.cds.unistra.fr/DSS/DSS2-NIR hips_progenitor_url = https://alasky.cds.unistra.fr/DSS/DSS2-NIR/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/DSS/DSS2-NIR hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 41 moc_time_range = 1 moc_order = 9 obs_initial_ra = 200.0641577 obs_initial_dec = -62.0757716 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288455126 ID = CDS/P/DSS2/blue hips_doi = 10.26093/cds/aladin/2szd-bms creator_did = ivo://CDS/P/DSS2/blue obs_collection = DSS2 Blue (XJ+S) obs_title = DSS2 Blue (XJ+S) obs_description = The Catalogs and Surveys Group of the Space Telescope Science Institute has digitized the photographic Sky survey plates from the Palomar and UK Schmidt telescopes to produce the "Digitized Sky Survey"(DSS). Each plate covers 6.5 x 6.5 degrees of the sky and have been\ndigitized using a modified PDS microdensitometer. The DSS blue HiPS is a combination of DSS2-XJ and DSS2-S. DSS2-XJ north is the digitalization of the POSS-II J (1987-1998 - 0.491um) from Caltech,DSS2-S south is the digitalization of the SERC-J (1975-1987 - 0.468um) and SERC-EJ (1979-1988 - 0.468um) from ROE.The all-sky HEALPix resampling has been done by the CDS with the help of CADC. obs_copyright = Digitized Sky Survey - STScI/NASA, Healpixed by CDS obs_copyright_url = http://archive.stsci.edu/dss/copyright.html client_category = Image/Optical/DSS client_sort_key = 03-01-03 hips_release_date = 2019-06-17T07:58Z hips_builder = Aladin/HipsGen v10.125 hips_creator = Fernique P. (CDS) hips_version = 1.4 hips_order = 9 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = jpeg fits dataproduct_type = image hips_pixel_cut = 4286 19959 hips_data_range = -4736 29668 client_application = AladinLite client_application = AladinDesktop moc_access_url = http://alasky.u-strasbg.fr/DSS/DSS2-blue-XJ-S/Moc.fits hips_progenitor_url = https://alasky.cds.unistra.fr/DSS/DSS2-blue-XJ-S/HpxFinder hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = The Digitized Sky Surveys were produced at the Space Telescope Science Institute under U.S. Government grant NAG W-2166. The images of these surveys are based on photographic data obtained using the Oschin Schmidt Telescope on Palomar Mountain and the UK Schmidt Telescope. The plates were processed into the present compressed digital form with the permission of these institutions. The National Geographic Society - Palomar Observatory Sky Atlas (POSS-I) was made by the California Institute of Technology with grants from the National Geographic Society. The Second Palomar Observatory Sky Survey (POSS-II) was made by the California Institute of Technology with funds from the National Science Foundation, the National Geographic Society, the Sloan Foundation, the Samuel Oschin Foundation, and the Eastman Kodak Corporation. The Oschin Schmidt Telescope is operated by the California Institute of Technology and Palomar Observatory. The UK Schmidt Telescope was operated by the Royal Observatory Edinburgh, with funding from the UK Science and Engineering Research Council (later the UK Particle Physics and Astronomy Research Council), until 1988 June, and thereafter by the Anglo-Australian Observatory. The blue plates of the southern Sky Atlas and its Equatorial Extension (together known as the SERC-J), as well as the Equatorial Red (ER), and the Second Epoch [red] Survey (SES) were all taken with the UK Schmidt. Supplemental funding for sky-survey work at the ST ScI is provided by the European Southern Observatory. prov_progenitor = STScI bib_reference = 1996ASPC..101...88L bib_reference_url = http://cdsads.u-strasbg.fr/abs/1996ASPC..101...88L t_min = 42413 t_max = 50814 obs_regime = Optical em_min = 4.68e-7 em_max = 4.91e-7 hips_creation_date = 2015-02-07T11:42Z hips_pixel_scale = 2.236E-4 hips_initial_fov = 23.0 hips_initial_ra = 271.0198457 hips_initial_dec = -24.3603897 hips_order_min = 0 hips_pixel_bitpix = 16 moc_sky_fraction = 0.9972 hips_estsize = 2331148605 hipsgen_date = 2019-06-17T07:58Z hipsgen_params = out=/asd-volumes/sc1-asd-volume6/DSS/DSS2-blue-XJ-S UPDATE hips_service_url = https://alasky.cds.unistra.fr/DSS/DSS2-blue-XJ-S hips_service_url_1 = https://alaskybis.cds.unistra.fr/DSS/DSS2-blue-XJ-S hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 41 moc_time_range = 1 moc_order = 9 obs_initial_ra = 271.0198457 obs_initial_dec = -24.3603897 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288414390 ID = CDS/P/DSS2/color hips_doi = 10.26093/cds/aladin/ht9n-7r creator_did = ivo://CDS/P/DSS2/color obs_collection = DSS colored obs_title = DSS colored obs_description = Color composition generated by CDS. This HiPS survey is based on 2 others HiPS surveys, respectively DSS2-red and DSS2-blue HiPS, both of them directly generated from original scanned plates downloaded from STScI site. The red component has been built from POSS-II F, AAO-SES,SR and SERC-ER plates. The blue component has been build from POSS-II J and SERC-J,EJ. The green component is based on the mean of other components. Three missing plates from red survey (253, 260, 359) has been replaced by pixels from the DSSColor STScI jpeg survey. The 11 missing blue plates (mainly in galactic plane) have not been replaced (only red component). obs_copyright = Digitized Sky Survey - STScI/NASA, Colored & Healpixed by CDS obs_copyright_url = http://archive.stsci.edu/dss/copyright.html client_category = Image/Optical/DSS client_sort_key = 03-00 hips_builder = Aladin/HipsGen v10.123 hips_creation_date = 2010-05-01T19:05Z hips_release_date = 2019-05-07T10:55Z hips_creator = Oberto A. (CDS) , Fernique P. (CDS) hips_version = 1.4 hips_order = 9 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = jpeg dataproduct_type = image client_application = AladinLite client_application = AladinDesktop moc_access_url = http://alasky.u-strasbg.fr/DSS/DSSColor/Moc.fits hips_status = public master clonableOnce hips_rgb_red = DSS2Merged [1488.0 8488.8125 14666.0 Linear] hips_rgb_blue = DSS2-blue-XJ-S [4286.0 12122.5 19959.0 Linear] hips_hierarchy = median hips_pixel_scale = 2.236E-4 hips_initial_ra = 085.30251 hips_initial_dec = -02.25468 hips_initial_fov = 2 moc_sky_fraction = 1 hips_copyright = CNRS/Unistra obs_ack = The Digitized Sky Surveys were produced at the Space Telescope Science Institute under U.S. Government grant NAG W-2166. The images of these surveys are based on photographic data obtained using the Oschin Schmidt Telescope on Palomar Mountain and the UK Schmidt Telescope. The plates were processed into the present compressed digital form with the permission of these institutions. The National Geographic Society - Palomar Observatory Sky Atlas (POSS-I) was made by the California Institute of Technology with grants from the National Geographic Society. The Second Palomar Observatory Sky Survey (POSS-II) was made by the California Institute of Technology with funds from the National Science Foundation, the National Geographic Society, the Sloan Foundation, the Samuel Oschin Foundation, and the Eastman Kodak Corporation. The Oschin Schmidt Telescope is operated by the California Institute of Technology and Palomar Observatory. The UK Schmidt Telescope was operated by the Royal Observatory Edinburgh, with funding from the UK Science and Engineering Research Council (later the UK Particle Physics and Astronomy Research Council), until 1988 June, and thereafter by the Anglo-Australian Observatory. The blue plates of the southern Sky Atlas and its Equatorial Extension (together known as the SERC-J), as well as the Equatorial Red (ER), and the Second Epoch [red] Survey (SES) were all taken with the UK Schmidt. Supplemental funding for sky-survey work at the ST ScI is provided by the European Southern Observatory. prov_progenitor = STScI bib_reference = 1996ASPC..101...88L bib_reference_url = http://cdsads.u-strasbg.fr/abs/1996ASPC..101...88L t_min = 42413 t_max = 51179 obs_regime = Optical em_min = 4e-7 em_max = 6e-7 hips_order_min = 0 dataproduct_subtype = color hips_estsize = 37580398 hipsgen_date = 2019-05-07T10:55Z hipsgen_params = out=/asd-volumes/sc1-asd-volume8/DSS/DSSColor UPDATE hips_service_url = https://alasky.cds.unistra.fr/DSS/DSSColor hips_service_url_1 = https://alaskybis.cds.unistra.fr/DSS/DSSColor hips_status_1 = public mirror clonableOnce hips_service_url_2 = https://casda.csiro.au/hips/DSS2/color hips_status_2 = public mirror unclonable hips_service_url_3 = https://irsa.ipac.caltech.edu/data/hips/CDS/DSS2/color hips_status_3 = public mirror unclonable hips_service_url_4 = https://healpix.ias.u-psud.fr/CDS_P_DSS2_color hips_status_4 = public mirror unclonable hips_service_url_5 = http://skies.esac.esa.int/DSSColor hips_status_5 = public mirror unclonable moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 9 obs_initial_ra = 085.30251 obs_initial_dec = -02.25468 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1729584775740 ID = CDS/P/DSS2/red hips_doi = 10.26093/cds/aladin/wenz-vg creator_did = ivo://CDS/P/DSS2/red obs_collection = DSS2 Red (F+R) obs_title = DSS2 Red (F+R) obs_description = The Catalogs and Surveys Group of the Space Telescope Science Institute has digitized the photographic Sky survey plates from the Palomar and UK Schmidt telescopes to produce the "Digitized Sky Survey" (DSS). Each plate covers 6.5 x 6.5 degrees of the sky and have been digitized using a modified PDS microdensitometer.\nDSS2F north is the digitalization of the POSS2/UKSTU Red survey (0.658um)\nDSS2R south is the digitalization of the AAO Red survey (0.64um)\nThe all-sky HEALPix resampling has been done by the CDS obs_copyright = Digitized Sky Survey - STScI/NASA, Healpixed by CDS obs_copyright_url = http://archive.stsci.edu/dss/copyright.html client_category = Image/Optical/DSS client_sort_key = 03-01-02 hips_creation_date = 2012-07-13T14:03Z hips_release_date = 2019-05-07T10:59Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Boch T. (CDS) hips_version = 1.4 hips_order = 9 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = jpeg fits hips_pixel_cut = 1000 10000 dataproduct_type = image client_application = AladinLite client_application = AladinDesktop moc_access_url = http://alasky.u-strasbg.fr/DSS/DSS2Merged/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = The Digitized Sky Surveys were produced at the Space Telescope Science Institute under U.S. Government grant NAG W-2166. The images of these surveys are based on photographic data obtained using the Oschin Schmidt Telescope on Palomar Mountain and the UK Schmidt Telescope. The plates were processed into the present compressed digital form with the permission of these institutions. The National Geographic Society - Palomar Observatory Sky Atlas (POSS-I) was made by the California Institute of Technology with grants from the National Geographic Society. The Second Palomar Observatory Sky Survey (POSS-II) was made by the California Institute of Technology with funds from the National Science Foundation, the National Geographic Society, the Sloan Foundation, the Samuel Oschin Foundation, and the Eastman Kodak Corporation. The Oschin Schmidt Telescope is operated by the California Institute of Technology and Palomar Observatory. The UK Schmidt Telescope was operated by the Royal Observatory Edinburgh, with funding from the UK Science and Engineering Research Council (later the UK Particle Physics and Astronomy Research Council), until 1988 June, and thereafter by the Anglo-Australian Observatory. The blue plates of the southern Sky Atlas and its Equatorial Extension (together known as the SERC-J), as well as the Equatorial Red (ER), and the Second Epoch [red] Survey (SES) were all taken with the UK Schmidt. Supplemental funding for sky-survey work at the ST ScI is provided by the European Southern Observatory. prov_progenitor = STScI bib_reference = 1996ASPC..101...88L bib_reference_url = http://cdsads.u-strasbg.fr/abs/1996ASPC..101...88L t_min = 45700 t_max = 51179 obs_regime = Optical em_min = 6.4e-7 em_max = 6.58e-7 hips_pixel_scale = 2.236E-4 hips_initial_fov = 33.0 hips_initial_ra = 82.9368880 hips_initial_dec = -3.3581890 hips_order_min = 0 hips_pixel_bitpix = 16 moc_sky_fraction = 1 hips_estsize = 2301246266 hipsgen_date = 2019-05-07T10:59Z hipsgen_params = out=/asd-volumes/sc1-asd-volume8/DSS/DSS2Merged UPDATE hips_service_url = https://alasky.cds.unistra.fr/DSS/DSS2Merged hips_service_url_1 = https://alaskybis.cds.unistra.fr/DSS/DSS2Merged hips_status_1 = public mirror clonableOnce hips_service_url_2 = https://irsa.ipac.caltech.edu/data/hips/CDS/DSS2/red hips_status_2 = public mirror unclonable moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 9 obs_initial_ra = 82.9368880 obs_initial_dec = -3.3581890 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288897892 ID = CDS/P/Dione/Cassini-PIA12577 client_category = Solar system/Saturn/Dione hips_initial_fov = 180 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/Dione/Cassini-PIA12577 hips_overlay = mean hips_hierarchy = median hips_creator = Fernique P. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = Dione Cassini PIA12577 obs_description = This global map of Saturn's moon Dione was created using images taken during flybys by NASA's Cassini spacecraft. Images from NASA's Voyager mission fill the gaps in Cassini's coverage. The map is a simple cylindrical (equidistant) projection and has a scale of 153 meters (500 feet) per pixel at the equator. The resolution of the map is 64 pixels per degree. The mean radius of Dione used for projection of this map is 563 kilometers (350 miles). The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate in Washington. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. obs_ack = NASA/JPL/Space Science Institute prov_progenitor = JPL/PhotoJournal prov_progenitor_url = https://photojournal.jpl.nasa.gov/catalog/PIA12577 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T07:06Z hips_frame = dione hips_body = dione hips_order = 3 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg hips_pixel_scale = 0.01431 s_pixel_scale = 0.01562 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 18357 hipsgen_date = 2018-01-24T13:47Z hipsgen_params = "hhh=Dione/Dione.jpg 23040x11520 11520x11520" partitioning=false -maxthread=10 in=Dione creator_did=CDS/P/Dione/Cassini-PIA12577 -f color=jpg INDEX TILES hips_creation_date = 2018-01-24T13:47Z hips_order_min = 0 dataproduct_subtype = color hipsgen_date_1 = 2019-05-21T07:06Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume6/Planets/CDS_P_Dione_Cassini-PIA12577 UPDATE hips_service_url = https://alasky.cds.unistra.fr/Planets/CDS_P_Dione_Cassini-PIA12577 hips_service_url_1 = https://alaskybis.cds.unistra.fr/Planets/CDS_P_Dione_Cassini-PIA12577 hips_status_1 = public mirror clonableOnce client_application = AladinDesktopBeta>=10.040 AladinDesktop>=11.125 moc_type = smoc moc_order = 3 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288467626 ID = CDS/P/EGRET/Dif/100-150 hips_doi = 10.26093/cds/aladin/3k8t-1gp creator_did = ivo://CDS/P/EGRET/Dif/100-150 obs_collection = Diffuse Gamma-ray EGRET maps - 100-150MeV obs_title = EGRET Dif 100-150MeV obs_description = This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000. bib_reference = 2005ApJ...621..291C obs_copyright_url = ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html client_category = Image/Gamma-ray/EGRET/Diffuse client_sort_key = 00-02-01-04 hips_release_date = 2019-05-05T06:00Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_width = 128 hips_tile_format = jpeg fits dataproduct_type = image hips_pixel_cut = 1.731E-6 6.218E-5 moc_access_url = http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_100-150/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = This research has made use of data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory's High Energy Astrophysics Division prov_progenitor = NASA/HEASARC bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2005ApJ...621..291C obs_copyright = Compton Gamma Ray Observatory (CGRO) t_min = 48361 t_max = 48943 obs_regime = Gamma-ray em_min = 8.2656e-15 em_max = 1.2398e-14 hips_creation_date = 2014-06-05T11:13Z hips_hierarchy = mean hips_pixel_scale = 0.01431 hips_initial_fov = 120 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 1112337 hipsgen_date = 2019-05-05T06:00Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/EGRET/EGRET-dif/EGRET_dif_100-150 UPDATE hips_service_url = https://alasky.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_100-150 hips_service_url_1 = https://alaskybis.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_100-150 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288414574 ID = CDS/P/EGRET/Dif/1000-2000 hips_doi = 10.26093/cds/aladin/3535-cdg creator_did = ivo://CDS/P/EGRET/Dif/1000-2000 obs_collection = Diffuse Gamma-ray EGRET maps - 1000-2000MeV obs_title = EGRET Dif 1000-2000MeV obs_description = This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000. bib_reference = 2005ApJ...621..291C obs_copyright_url = ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html client_category = Image/Gamma-ray/EGRET/Diffuse client_sort_key = 00-02-01-08 hips_release_date = 2019-05-05T06:00Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_width = 128 hips_tile_format = jpeg fits dataproduct_type = image hips_pixel_cut = 1.731E-6 6.218E-5 moc_access_url = http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_1000-2000/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = This research has made use of data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory's High Energy Astrophysics Division prov_progenitor = NASA/HEASARC bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2005ApJ...621..291C obs_copyright = Compton Gamma Ray Observatory (CGRO) t_min = 48361 t_max = 48943 obs_regime = Gamma-ray em_min = 6.1992e-16 em_max = 1.2398e-15 hips_creation_date = 2014-06-05T11:18Z hips_hierarchy = mean hips_pixel_scale = 0.01431 hips_initial_fov = 120 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 1112337 hipsgen_date = 2019-05-05T06:00Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/EGRET/EGRET-dif/EGRET_dif_1000-2000 UPDATE hips_service_url = https://alasky.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_1000-2000 hips_service_url_1 = https://alaskybis.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_1000-2000 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288414630 ID = CDS/P/EGRET/Dif/150-300 hips_doi = 10.26093/cds/aladin/34b7-dwe creator_did = ivo://CDS/P/EGRET/Dif/150-300 obs_collection = Diffuse Gamma-ray EGRET maps - 150-300MeV obs_title = EGRET Dif 150-300MeV obs_description = This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000. bib_reference = 2005ApJ...621..291C obs_copyright_url = ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html client_category = Image/Gamma-ray/EGRET/Diffuse client_sort_key = 00-02-01-05 hips_release_date = 2019-05-05T06:01Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_width = 128 hips_tile_format = jpeg fits dataproduct_type = image hips_pixel_cut = 1.731E-6 6.218E-5 moc_access_url = http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_150-300/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = This research has made use of data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory's High Energy Astrophysics Division prov_progenitor = NASA/HEASARC bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2005ApJ...621..291C obs_copyright = Compton Gamma Ray Observatory (CGRO) t_min = 48361 t_max = 48943 obs_regime = Gamma-ray em_min = 4.1328e-15 em_max = 8.2656e-15 hips_creation_date = 2014-06-05T11:14Z hips_hierarchy = mean hips_pixel_scale = 0.01431 hips_initial_fov = 120 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 1112337 hipsgen_date = 2019-05-05T06:01Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/EGRET/EGRET-dif/EGRET_dif_150-300 UPDATE hips_service_url = https://alasky.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_150-300 hips_service_url_1 = https://alaskybis.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_150-300 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288414682 ID = CDS/P/EGRET/Dif/2000-4000 hips_doi = 10.26093/cds/aladin/3bd9-mn9 creator_did = ivo://CDS/P/EGRET/Dif/2000-4000 obs_collection = Diffuse Gamma-ray EGRET maps - 2000-4000MeV obs_title = EGRET Dif 2000-4000MeV obs_description = This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000. bib_reference = 2005ApJ...621..291C obs_copyright_url = ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html client_category = Image/Gamma-ray/EGRET/Diffuse client_sort_key = 00-02-01-09 hips_release_date = 2019-05-05T06:01Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_width = 128 hips_tile_format = jpeg fits dataproduct_type = image hips_pixel_cut = 1.731E-6 6.218E-5 moc_access_url = http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_2000-4000/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = This research has made use of data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory's High Energy Astrophysics Division prov_progenitor = NASA/HEASARC bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2005ApJ...621..291C obs_copyright = Compton Gamma Ray Observatory (CGRO) t_min = 48361 t_max = 48943 obs_regime = Gamma-ray em_min = 3.0996e-16 em_max = 6.1992e-16 hips_creation_date = 2014-06-05T11:19Z hips_hierarchy = mean hips_pixel_scale = 0.01431 hips_initial_fov = 120 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 1112337 hipsgen_date = 2019-05-05T06:01Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/EGRET/EGRET-dif/EGRET_dif_2000-4000 UPDATE hips_service_url = https://alasky.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_2000-4000 hips_service_url_1 = https://alaskybis.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_2000-4000 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288414734 ID = CDS/P/EGRET/Dif/30-50 hips_doi = 10.26093/cds/aladin/2nbf-ypm creator_did = ivo://CDS/P/EGRET/Dif/30-50 obs_collection = Diffuse Gamma-ray EGRET maps - 30-50MeV obs_title = EGRET Dif 30-50MeV obs_description = This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000. bib_reference = 2005ApJ...621..291C obs_copyright_url = ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html client_category = Image/Gamma-ray/EGRET/Diffuse client_sort_key = 00-02-01-01 hips_release_date = 2019-05-05T06:01Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_width = 128 hips_tile_format = jpeg fits dataproduct_type = image hips_pixel_cut = 1.731E-6 6.218E-5 moc_access_url = http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_30-50/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = This research has made use of data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory's High Energy Astrophysics Division prov_progenitor = NASA/HEASARC bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2005ApJ...621..291C obs_copyright = Compton Gamma Ray Observatory (CGRO) t_min = 48361 t_max = 48943 obs_regime = Gamma-ray em_min = 2.4797e-14 em_max = 4.1328e-14 hips_creation_date = 2014-06-05T11:10Z hips_hierarchy = mean hips_pixel_scale = 0.01431 hips_initial_fov = 120 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 1112337 hipsgen_date = 2019-05-05T06:01Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/EGRET/EGRET-dif/EGRET_dif_30-50 UPDATE hips_service_url = https://alasky.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_30-50 hips_service_url_1 = https://alaskybis.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_30-50 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288414794 ID = CDS/P/EGRET/Dif/300-500 hips_doi = 10.26093/cds/aladin/5prj-x6 creator_did = ivo://CDS/P/EGRET/Dif/300-500 obs_collection = Diffuse Gamma-ray EGRET maps - 300-500MeV obs_title = EGRET Dif 300-500MeV obs_description = This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000. bib_reference = 2005ApJ...621..291C obs_copyright_url = ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html client_category = Image/Gamma-ray/EGRET/Diffuse client_sort_key = 00-02-01-06 hips_release_date = 2019-05-05T06:01Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_width = 128 hips_tile_format = jpeg fits dataproduct_type = image hips_pixel_cut = 1.731E-6 6.218E-5 moc_access_url = http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_300-500/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = This research has made use of data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory's High Energy Astrophysics Division prov_progenitor = NASA/HEASARC bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2005ApJ...621..291C obs_copyright = Compton Gamma Ray Observatory (CGRO) t_min = 48361 t_max = 48943 obs_regime = Gamma-ray em_min = 2.4797e-15 em_max = 4.1328e-15 hips_creation_date = 2014-06-05T11:16Z hips_hierarchy = mean hips_pixel_scale = 0.01431 hips_initial_fov = 120 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 1112337 hipsgen_date = 2019-05-05T06:01Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/EGRET/EGRET-dif/EGRET_dif_300-500 UPDATE hips_service_url = https://alasky.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_300-500 hips_service_url_1 = https://alaskybis.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_300-500 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288414854 ID = CDS/P/EGRET/Dif/4000-10000 hips_doi = 10.26093/cds/aladin/2ffk-vw8 creator_did = ivo://CDS/P/EGRET/Dif/4000-10000 obs_collection = Diffuse Gamma-ray EGRET maps - 4000-10000MeV obs_title = EGRET Dif 4000-10000MeV obs_description = This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000. bib_reference = 2005ApJ...621..291C obs_copyright_url = ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html client_category = Image/Gamma-ray/EGRET/Diffuse client_sort_key = 00-02-01-10 hips_release_date = 2019-05-05T06:02Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_width = 128 hips_tile_format = jpeg fits dataproduct_type = image hips_pixel_cut = 1.731E-6 6.218E-5 moc_access_url = http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_4000-10000/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = This research has made use of data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory's High Energy Astrophysics Division prov_progenitor = NASA/HEASARC bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2005ApJ...621..291C obs_copyright = Compton Gamma Ray Observatory (CGRO) t_min = 48361 t_max = 48943 obs_regime = Gamma-ray em_min = 1.2398e-16 em_max = 3.0996e-16 hips_creation_date = 2014-06-05T11:19Z hips_hierarchy = mean hips_pixel_scale = 0.01431 hips_initial_fov = 120 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 1112337 hipsgen_date = 2019-05-05T06:02Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/EGRET/EGRET-dif/EGRET_dif_4000-10000 UPDATE hips_service_url = https://alasky.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_4000-10000 hips_service_url_1 = https://alaskybis.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_4000-10000 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288414922 ID = CDS/P/EGRET/Dif/50-70 hips_doi = 10.26093/cds/aladin/bw2v-fp creator_did = ivo://CDS/P/EGRET/Dif/50-70 obs_collection = Diffuse Gamma-ray EGRET maps - 50-70MeV obs_title = EGRET Dif 50-70MeV obs_description = This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000. bib_reference = 2005ApJ...621..291C obs_copyright_url = ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html client_category = Image/Gamma-ray/EGRET/Diffuse client_sort_key = 00-02-01-02 hips_release_date = 2019-05-05T06:02Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_width = 128 hips_tile_format = jpeg fits dataproduct_type = image hips_pixel_cut = 1.731E-6 6.218E-5 moc_access_url = http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_50-70/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = This research has made use of data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory's High Energy Astrophysics Division prov_progenitor = NASA/HEASARC bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2005ApJ...621..291C obs_copyright = Compton Gamma Ray Observatory (CGRO) t_min = 48361 t_max = 48943 obs_regime = Gamma-ray em_min = 1.7712e-14 em_max = 2.4797e-14 hips_creation_date = 2014-06-05T11:09Z hips_hierarchy = mean hips_pixel_scale = 0.01431 hips_initial_fov = 120 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 1112337 hipsgen_date = 2019-05-05T06:02Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/EGRET/EGRET-dif/EGRET_dif_50-70 UPDATE hips_service_url = https://alasky.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_50-70 hips_service_url_1 = https://alaskybis.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_50-70 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288414978 ID = CDS/P/EGRET/Dif/500-1000 hips_doi = 10.26093/cds/aladin/216g-av7 creator_did = ivo://CDS/P/EGRET/Dif/500-1000 obs_collection = Diffuse Gamma-ray EGRET maps - 500-1000MeV obs_title = EGRET Dif 500-1000MeV obs_description = This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000. bib_reference = 2005ApJ...621..291C obs_copyright_url = ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html client_category = Image/Gamma-ray/EGRET/Diffuse client_sort_key = 00-02-01-07 hips_release_date = 2019-05-05T06:02Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_width = 128 hips_tile_format = jpeg fits dataproduct_type = image hips_pixel_cut = 1.731E-6 6.218E-5 moc_access_url = http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_500-1000/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = This research has made use of data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory's High Energy Astrophysics Division prov_progenitor = NASA/HEASARC bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2005ApJ...621..291C obs_copyright = Compton Gamma Ray Observatory (CGRO) t_min = 48361 t_max = 48943 obs_regime = Gamma-ray em_min = 1.2398e-15 em_max = 2.4797e-15 hips_creation_date = 2014-06-05T11:17Z hips_hierarchy = mean hips_pixel_scale = 0.01431 hips_initial_fov = 120 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 1112337 hipsgen_date = 2019-05-05T06:02Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/EGRET/EGRET-dif/EGRET_dif_500-1000 UPDATE hips_service_url = https://alasky.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_500-1000 hips_service_url_1 = https://alaskybis.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_500-1000 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288415034 ID = CDS/P/EGRET/Dif/70-100 hips_doi = 10.26093/cds/aladin/3mnf-56w creator_did = ivo://CDS/P/EGRET/Dif/70-100 obs_collection = Diffuse Gamma-ray EGRET maps - 70-100MeV obs_title = EGRET Dif 70-100MeV obs_description = This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000. bib_reference = 2005ApJ...621..291C obs_copyright_url = ftp://legacy.gsfc.nasa.gov/compton/data/egret/diffuse_maps/README.fitsmaps.html client_category = Image/Gamma-ray/EGRET/Diffuse client_sort_key = 00-02-01-03 hips_release_date = 2019-05-05T06:03Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_width = 128 hips_tile_format = jpeg fits dataproduct_type = image hips_pixel_cut = 1.731E-6 6.218E-5 moc_access_url = http://alasky.u-strasbg.fr/EGRET/EGRET-dif/EGRET_dif_70-100/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = This research has made use of data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory's High Energy Astrophysics Division prov_progenitor = NASA/HEASARC bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2005ApJ...621..291C obs_copyright = Compton Gamma Ray Observatory (CGRO) t_min = 48361 t_max = 48943 obs_regime = Gamma-ray em_min = 1.2398e-14 em_max = 1.7712e-14 hips_creation_date = 2014-06-05T11:12Z hips_hierarchy = mean hips_pixel_scale = 0.01431 hips_initial_fov = 120 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 1112337 hipsgen_date = 2019-05-05T06:03Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/EGRET/EGRET-dif/EGRET_dif_70-100 UPDATE hips_service_url = https://alasky.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_70-100 hips_service_url_1 = https://alaskybis.cds.unistra.fr/EGRET/EGRET-dif/EGRET_dif_70-100 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288415090 ID = CDS/P/EGRET/inf100 hips_doi = 10.26093/cds/aladin/35cp-apx creator_did = ivo://CDS/P/EGRET/inf100 obs_collection = Gamma-ray EGRET maps - inf 100MeV obs_title = EGRET inf 100MeV obs_description = This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000. bib_reference = 2005ApJ...621..291C obs_copyright = Distributed by SkyView/HEASARC - HEALPixed by CDS obs_copyright = Compton Gamma Ray Observatory (CGRO) client_category = Image/Gamma-ray/EGRET client_sort_key = 00-02-00a hips_release_date = 2019-05-05T06:03Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_format = jpeg fits dataproduct_type = image hips_pixel_cut = 0 3.588E-4 hips_data_range = -2.037E-4 6.112E-4 moc_access_url = http://alasky.u-strasbg.fr/EGRET/EGRET-inf100/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = This research has made use of data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory's High Energy Astrophysics Division prov_progenitor = NASA/HEASARC bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2005ApJ...621..291C t_min = 48361 t_max = 48943 obs_regime = Gamma-ray em_min = 1.2398e-14 em_max = 4.1328e-14 hips_creation_date = 2014-06-05T16:54Z hips_tile_width = 512 hips_hierarchy = mean hips_pixel_scale = 0.01431 hips_initial_fov = 120 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 1112337 hipsgen_date = 2019-05-05T06:03Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/EGRET/EGRET-inf100 UPDATE hips_service_url = https://alasky.cds.unistra.fr/EGRET/EGRET-inf100 hips_service_url_1 = https://alaskybis.cds.unistra.fr/EGRET/EGRET-inf100 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288415146 ID = CDS/P/EGRET/sup100 hips_doi = 10.26093/cds/aladin/5c99-fg creator_did = ivo://CDS/P/EGRET/sup100 obs_collection = Gamma-ray EGRET maps - sup 100MeV obs_title = EGRET sup 100MeV obs_description = This data presents all-sky maps of diffuse gamma radiation in energy ranges between 100 MeV to 150 MeV, based on data collected by the EGRET instrument on the Compton Gamma Ray Observatory. EGRET detected gamma rays in the energy range from 30 MeV to over 30 GeV, with an energy resolution of 20-25% over most of that range. The instrument is described in Hughes et al. (1980), Kanbach (1988, 1989), Thompson et. al (1993) and Esposito et al. (1998). The work described here started with standard EGRET all-sky maps (ftp://cossc.gsfc.nasa.gov/compton/data/egret/high_level/combined_data) of photon counts, instrument exposure, and gamma-ray intensity, binned in 0.5 degree pixels, in both Galactic and equatorial coordinates. The energy ranges in MeV are: (narrow ranges) 30-50, 50-70, 70-100, 100-150, 150-300, 300-500, 500-1000, 1000-2000, 2000-4000, 4000-10000; (broader ranges) 30-100, 100-300, 300-1000; (integral ranges) >100, >300, >1000. bib_reference = 2005ApJ...621..291C obs_copyright = Distributed by SkyView/HEASARC - HEALPixed by CDS obs_copyright = Compton Gamma Ray Observatory (CGRO) client_category = Image/Gamma-ray/EGRET client_sort_key = 00-02-00b hips_release_date = 2019-05-05T06:04Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_format = jpeg fits dataproduct_type = image hips_pixel_cut = 0 1.508E-4 hips_data_range = -8.375E-5 2.512E-4 moc_access_url = http://alasky.u-strasbg.fr/EGRET/EGRET-sup100/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = This research has made use of data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory's High Energy Astrophysics Division prov_progenitor = NASA/HEASARC bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2005ApJ...621..291C t_min = 48361 t_max = 48943 obs_regime = Gamma-ray em_min = 1.2398e-16 em_max = 1.2398e-14 hips_creation_date = 2014-06-05T17:00Z hips_tile_width = 512 hips_hierarchy = mean hips_pixel_scale = 0.01431 hips_initial_fov = 120 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 1112337 hipsgen_date = 2019-05-05T06:04Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/EGRET/EGRET-sup100 UPDATE hips_service_url = https://alasky.cds.unistra.fr/EGRET/EGRET-sup100 hips_service_url_1 = https://alaskybis.cds.unistra.fr/EGRET/EGRET-sup100 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288415202 ID = CDS/P/ESO/EPO hips_doi = 10.26093/cds/aladin/2jgn-ywn hips_frame = equatorial hips_order = 12 hips_initial_fov = 0.2 hips_initial_ra = 49.9210259 hips_initial_dec = -19.4111631 creator_did = ivo://CDS/P/ESO/EPO hips_overlay = mean hips_hierarchy = median client_category = Outreach/ESO hips_creator = Boch T. (CDS) hips_copyright = CNRS/Unistra obs_title = ESO EPO images obs_collection = ESO obs_description = ESO Outreach images. Hipsilized by CDS obs_copyright = European Southern Observatory obs_copyright_url = https://www.eso.org/public/unitedkingdom/copyright/ hips_builder = Aladin/HipsGen v11.071 hips_version = 1.4 hips_release_date = 2022-08-17T10:29Z hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png hips_pixel_scale = 6.989E-6 s_pixel_scale = 9.540E-12 dataproduct_type = image dataproduct_subtype = color moc_sky_fraction = 0.03754 hips_estsize = 4340404428 hipsgen_date = 2022-08-17T10:29Z hipsgen_params = in=data creator_did=CDS/P/ESO/EPO maxThread=32 hips_order=14 mode=keeptile tiles hips_service_url = https://alasky.cds.unistra.fr/ESO-outreach/CDS_P_ESO_EPO hips_progenitor_url = https://alasky.cds.unistra.fr/ESO-outreach/CDS_P_ESO_EPO/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/ESO-outreach/CDS_P_ESO_EPO hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 14 obs_initial_ra = 49.9210259 obs_initial_dec = -19.4111631 obs_initial_fov = 0.003578631678976464 TIMESTAMP = 1721288492218 ID = CDS/P/Earth/BlueMarble client_category = Solar system/Earth hips_initial_fov = 180 hips_initial_ra = 7.76910551354468 hips_initial_dec = 48.58284624496147 creator_did = ivo://CDS/P/Earth/BlueMarble hips_overlay = mean hips_hierarchy = median hips_creator = Fernique P. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = Blue Marble Next Generation w/ Topography and Bathymetry obs_description = Blue Marble: Next Generation offers greater spatial detail of the surface and spans a longer data collection period than the original. The original Blue Marble was a composite of four months of MODIS observations with a spatial resolution (level of detail) of 1 square kilometer per pixel. Blue Marble: Next Generation offers a years worth of monthly composites at a spatial resolution of 500 meters. These monthly images reveal seasonal changes to the land surface: the green-up and dying-back of vegetation in temperate regions such as North America and Europe, dry and wet seasons in the tropics, and advancing and retreating Northern Hemisphere snow cover. From a computer processing standpoint, the major improvement is the development of a new technique for allowing the computer to automatically recognize and remove cloud-contaminated or otherwise bad data - a process that was previously done manually. Credit: Blue Marble: Next Generation was produced by Reto Stockli, NASA Earth Observatory (NASA Goddard Space Flight Center) obs_ack = Blue Marble: Next Generation was produced by Reto Stockli, NASA Earth Observatory (NASA Goddard Space Flight Center) prov_progenitor = NASA's Earth Observatory obs_copyright_url = https://earthobservatory.nasa.gov/Features/BlueMarble/ hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T06:51Z hips_frame = earth hips_body = earth hips_order = 5 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg hips_pixel_scale = 0.003579 s_pixel_scale = 0.004167 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 293604 hipsgen_date = 2018-01-21T16:49Z hipsgen_params = "hhh=Earth/Earth.jpg 86400x43200 21600x21600" partitioning=10800 -maxthread=10 in=Earth creator_did=CDS/P/Earth/BlueMarble -f color=jpg INDEX TILES hips_creation_date = 2018-01-21T16:50Z hips_order_min = 0 hipsgen_date_1 = 2019-05-21T06:48Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume6/Planets/CDS_P_Earth_BlueMarble UPDATE dataproduct_subtype = color hipsgen_date_2 = 2019-05-21T06:51Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/Planets/CDS_P_Earth_BlueMarble UPDATE hips_service_url = https://alasky.cds.unistra.fr/Planets/CDS_P_Earth_BlueMarble hips_service_url_1 = https://alaskybis.cds.unistra.fr/Planets/CDS_P_Earth_BlueMarble hips_status_1 = public mirror clonableOnce client_application = AladinDesktopBeta>=10.040 AladinDesktop>=11.125 moc_type = smoc moc_order = 5 obs_initial_ra = 7.76910551354468 obs_initial_dec = 48.58284624496147 obs_initial_fov = 1.8322594196359496 TIMESTAMP = 1721288465590 ID = CDS/P/Earth/DEM/elevation hips_doi = 10.26093/cds/aladin/2pkb-1hy creator_did = ivo://CDS/P/Earth/DEM/elevation hips_creator = Boch T. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = Earth elevation obs_collection = Earth DEM obs_description = This HiPS provides elevation data for the whole earth. Ground elevation data originate from viewfinderpanoramas.org (resolution: 3 arcseconds). It has been complemented with bathymetry data from www.gebco.net (resolution: 15 arcseconds). FITS tiles values provide elevation in meters at the given location. PNG tiles have been built using the mby color map (http://soliton.vm.bytemark.co.uk/pub/cpt-city/mby/index.html) with min cut=-10000m and max cut=7000m. obs_ack = Jonathan de Ferranti (https://viewfinderpanoramas.org/) - GEBCO (https://www.gebco.net/) prov_progenitor = Viewfinder panoramas (https://viewfinderpanoramas.org/Coverage%20map%20viewfinderpanoramas_org3.htm) and GEBCO_2023 Grid (ice surface elevation) (https://www.gebco.net/data_and_products/gridded_bathymetry_data/) o_unit = m o_ucd = pos.bodyrc.alt hips_builder = Aladin/HipsGen v12.104 + Python scripts hips_version = 1.4 hips_release_date = 2024-03-21T15:00Z hips_frame = earth hips_body = earth hips_order = 8 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = -7000 7000 hips_pixel_bitpix = -32 hips_initial_ra = 8.01 hips_initial_dec = 48.7 hips_initial_fov = 180 hips_pixel_scale = 4.473E-4 s_pixel_scale = 8.333E-4 dataproduct_type = image moc_sky_fraction = 1 hipsgen_date = 2023-11-08T10:49Z hips_sampling = bilinear hips_overlay = overlayMean mergeOverwrite treeMedian hips_service_url = https://alasky.cds.unistra.fr/Planets/CDS_P_Earth_DEM_elevation hips_service_url_1 = https://alaskybis.cds.unistra.fr/Planets/CDS_P_Earth_DEM_elevation hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 8 obs_initial_ra = 8.01 obs_initial_dec = 48.7 obs_initial_fov = 0.2290324274544937 TIMESTAMP = 1721288498054 ID = CDS/P/Earth/DEM/elevation+hillshading hips_doi = 10.26093/cds/aladin/1bp4-ate creator_did = ivo://CDS/P/Earth/DEM/elevation+hillshading client_category = Solar system/Earth hips_creator = Boch T. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = Earth elevation + hillshading obs_collection = Earth DEM obs_description = This HiPS combines elevation data from CDS/P/Earth/DEM/elevation and hillshading from CDS/P/Earth/DEM/hillshading obs_ack = Jonathan de Ferranti (https://viewfinderpanoramas.org/) - GEBCO (https://www.gebco.net/) prov_progenitor = Viewfinder panoramas (https://viewfinderpanoramas.org/Coverage%20map%20viewfinderpanoramas_org3.htm) and GEBCO_2023 Grid (ice surface elevation) (https://www.gebco.net/data_and_products/gridded_bathymetry_data/) o_unit = m o_ucd = pos.bodyrc.alt hips_builder = Aladin/HipsGen v12.104 + Python scripts hips_version = 1.4 hips_release_date = 2024-03-21T15:00Z hips_frame = earth hips_body = earth hips_order = 8 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png hips_pixel_bitpix = -32 hips_initial_ra = 8.01 hips_initial_dec = 48.7 hips_initial_fov = 180 hips_pixel_scale = 4.473E-4 s_pixel_scale = 8.333E-4 dataproduct_type = image moc_sky_fraction = 1 hipsgen_date = 2023-11-08T10:49Z hips_sampling = bilinear hips_overlay = overlayMean mergeOverwrite treeMedian dataproduct_subtype = color client_link = CDS/P/Earth/DEM/elevation elevation data only client_link = CDS/P/Earth/DEM/hillshading Hillshading only hips_service_url = https://alasky.cds.unistra.fr/Planets/CDS_P_Earth_DEM_elevation+hillshading hips_service_url_1 = https://alaskybis.cds.unistra.fr/Planets/CDS_P_Earth_DEM_elevation+hillshading hips_status_1 = public mirror clonableOnce client_application = AladinDesktopBeta>=10.040 AladinDesktop>=11.125 moc_type = smoc moc_order = 8 obs_initial_ra = 8.01 obs_initial_dec = 48.7 obs_initial_fov = 0.2290324274544937 TIMESTAMP = 1721288497998 ID = CDS/P/Earth/DEM/hillshading hips_doi = 10.26093/cds/aladin/k63e-69 creator_did = ivo://CDS/P/Earth/DEM/hillshading hips_creator = Boch T. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = Hillshading derived from earth elevation obs_collection = Earth DEM obs_description = Earth hillshading map derived from HiPS CDS/P/Earth/DEM/elevation. Hill shade has been computed from EarthPy hillshade function (https://earthpy.readthedocs.io/en/latest/api/earthpy.spatial.html#earthpy.spatial.hillshade ), using the default values of azimuth=30 deg, altitude=30 deg. obs_ack = Jonathan de Ferranti (https://viewfinderpanoramas.org/) - GEBCO (https://www.gebco.net/) prov_progenitor = Viewfinder panoramas (https://viewfinderpanoramas.org/Coverage%20map%20viewfinderpanoramas_org3.htm) and GEBCO_2023 Grid (ice surface elevation) (https://www.gebco.net/data_and_products/gridded_bathymetry_data/) hips_builder = Aladin/HipsGen v12.104 + Python scripts hips_version = 1.4 hips_release_date = 2024-03-21T15:00Z hips_frame = earth hips_body = earth hips_order = 8 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg fits hips_pixel_cut = 0 255 hips_pixel_bitpix = -32 hips_initial_ra = 8.01 hips_initial_dec = 48.7 hips_initial_fov = 180 hips_pixel_scale = 4.473E-4 s_pixel_scale = 8.333E-4 dataproduct_type = image moc_sky_fraction = 1 hipsgen_date = 2023-11-08T10:49Z hips_sampling = bilinear hips_overlay = overlayMean mergeOverwrite treeMedian hips_service_url = https://alasky.cds.unistra.fr/Planets/CDS_P_Earth_DEM_hillshading hips_service_url_1 = https://alaskybis.cds.unistra.fr/Planets/CDS_P_Earth_DEM_hillshading hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 8 obs_initial_ra = 8.01 obs_initial_dec = 48.7 obs_initial_fov = 0.2290324274544937 TIMESTAMP = 1721288498110 ID = CDS/P/Enceladus/Cassini-110m client_category = Solar system/Saturn/Enceladus hips_initial_fov = 180 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/Enceladus/Cassini-110m hips_overlay = mean hips_hierarchy = median hips_creator = Fernique P. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = Enceladus Cassini 110m (PIA 12564) obs_description = The Cassini Equinox Mission is a joint United States and European endeavor. The imaging team consists of scientists from the US, England, France, and Germany. The imaging operations center and team lead (Dr. C. Porco) are based at the Space Science Institute in Boulder, Colo. obs_ack = Cassini Team, Jet Propulsion Laboratory, Space Science Institute prov_progenitor = USGS Astrogeology Science Center prov_progenitor_url = https://planetarymaps.usgs.gov/mosaic/Enceladus_Cassini_mosaic_global_110m.tif t_min = 55105 t_max = 55165 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T07:06Z hips_frame = enceladus hips_body = enceladus hips_order = 3 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg hips_pixel_scale = 0.01431 s_pixel_scale = 0.025 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 18357 hipsgen_date = 2018-01-24T11:45Z hipsgen_params = "hhh=Enceladus/Enceladus.jpg 14401x7201 7201x7201" partitioning=false -maxthread=10 in=Enceladus creator_did=CDS/P/Enceladus/Cassini-110m -f color=jpg INDEX TILES hips_creation_date = 2018-01-24T11:45Z hips_order_min = 0 dataproduct_subtype = color hipsgen_date_1 = 2019-05-21T07:06Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume6/Planets/CDS_P_Enceladus_Cassini-110m UPDATE hips_service_url = https://alasky.cds.unistra.fr/Planets/CDS_P_Enceladus_Cassini-110m hips_service_url_1 = https://alaskybis.cds.unistra.fr/Planets/CDS_P_Enceladus_Cassini-110m hips_status_1 = public mirror clonableOnce client_application = AladinDesktopBeta>=10.040 AladinDesktop>=11.125 moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288467694 ID = CDS/P/Euclid/ERO/FirstImages hips_doi = 10.26093/cds/aladin/46gm-jp creator_did = ivo://CDS/P/Euclid/ERO/FirstImages hips_creator = Boch T. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = Euclid Early Release Observations (ERO) First Images obs_collection = Euclid obs_description = This HiPS is made of the five first images in the frame of Euclid ERO (Early Release Observations). Color composition made from VIS (0.53-0.92um wide-band), and near-infrared Y and H bands. Astrometry was added by CDS using astrometry.net software. obs_ack = These images correspond to the following proposals selected by the Euclid ERO programme committee : A first glance at free-floating baby Jupiters with Euclid - Lead scientist: E. Martín (Instituto de Astrofísica de Canarias); Euclid view of Milky Way globular clusters - Lead scientist: D. Massari (INAF-OAS Bologna); A Euclid showcase of nearby galaxies - Lead Scientist: L. Hunt (INAF-AO Arcetri, Firenze); The Perseus cluster of galaxies - Lead scientist: J.-C. Cuillandre (CEA, AIM, Université Paris-Saclay) prov_progenitor = https://www.esa.int/Science_Exploration/Space_Science/Euclid/Euclid_s_first_images_the_dazzling_edge_of_darkness obs_copyright = ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi; CC BY-SA 3.0 IGO obs_regime = Optical em_min = 5.3e-7 em_max = 2.02e-6 hips_builder = Aladin/HipsGen v12.104 hips_version = 1.4 hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 49.6864965 hips_initial_dec = 41.5852518 hips_initial_fov = 0.68335 hips_pixel_scale = 5.591E-5 s_pixel_scale = 8.333E-5 dataproduct_type = image moc_sky_fraction = 6.457E-5 hipsgen_date = 2023-11-07T13:30Z hipsgen_params = in=definitive-data out=hips id=CDS/P/Euclid/ERO/FirstImages hips_overlay = overlayMean mergeOverwriteTile treeMedian hips_release_date = 2023-11-07T15:31Z hips_tile_format = png hips_creation_date = 2023-11-07T15:31Z hips_estsize = 2088078 hips_nb_tiles = 4576 dataproduct_subtype = color hips_check_code = png:2806193857 client_category = Image/Optical/Euclid ERO hips_service_url = https://alasky.cds.unistra.fr/Euclid/ERO/FirstImages hips_progenitor_url = https://alasky.cds.unistra.fr/Euclid/ERO/FirstImages/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/Euclid/ERO/FirstImages hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 11 obs_initial_ra = 49.6864965 obs_initial_dec = 41.5852518 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288496314 ID = CDS/P/Euclid/ERO/NISP.H hips_doi = 10.26093/cds/aladin/32mq-2vf creator_did = ivo://CDS/P/Euclid/ERO/NISP.H hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = Euclid ERO NISP.H obs_collection = Euclid ERO obs_description = The ERO programme is an initiative of ESA and the Euclid Science Team: it includes one day of observations, taken before the start of the nominal survey, to showcase the capabilities of the ESA Euclid mission.Seventeen targets, from galaxy clusters, nearby galaxies, globular clusters, to star-forming regions, have been observed and analyzed. Details on selected ERO projects are available at https://www.cosmos.esa.int/web/euclid/ero-public-release obs_ack = This work has made use of the Early Release Observations (ERO) data from the Euclid mission of the European Space Agency (ESA), 2024, https://doi.org/10.57780/esa-qmocze3 prov_progenitor = https://euclid.esac.esa.int/dr/ero/ bib_reference_url = https://www.euclid-ec.org/science/publications/ obs_copyright_url = https://www.cosmos.esa.int/web/euclid/ero-credits obs_regime = Infrared em_min = 1.497170e-6 em_max = 2.056814e-6 client_category = Image/Infrared/Euclid ERO hips_builder = Aladin/HipsGen v12.119 + Montage hips_version = 1.4 hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 dataproduct_type = image hips_status = public master clonableOnce hips_initial_ra = 86.6908333 hips_initial_dec = 0.07916667 hips_initial_fov = 1.2 hips_pixel_scale = 2.795E-5 s_pixel_scale = 8.333E-5 hipsgen_date = 2024-05-23T18:29Z hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwriteTile treeMean hips_release_date = 2024-05-27T12:39Z hips_tile_format = png fits hips_pixel_cut = 139 2067 hips_data_range = -55410 166587 moc_sky_fraction = 2.718E-4 hips_creation_date = 2024-05-23T18:33Z hips_service_url = https://alasky.cds.unistra.fr/Euclid/ERO/CDS_P_Euclid_ERO_NISP.H hips_service_url_1 = https://alaskybis.cds.unistra.fr/Euclid/ERO/CDS_P_Euclid_ERO_NISP.H hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 12 obs_initial_ra = 86.6908333 obs_initial_dec = 0.07916667 obs_initial_fov = 0.014314526715905856 TIMESTAMP = 1721288496238 ID = CDS/P/Euclid/ERO/NISP.J hips_doi = 10.26093/cds/aladin/nmbt-j3 creator_did = ivo://CDS/P/Euclid/ERO/NISP.J hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = Euclid ERO NISP.J obs_collection = Euclid ERO obs_description = The ERO programme is an initiative of ESA and the Euclid Science Team: it includes one day of observations, taken before the start of the nominal survey, to showcase the capabilities of the ESA Euclid mission.Seventeen targets, from galaxy clusters, nearby galaxies, globular clusters, to star-forming regions, have been observed and analyzed. Details on selected ERO projects are available at https://www.cosmos.esa.int/web/euclid/ero-public-release obs_ack = This work has made use of the Early Release Observations (ERO) data from the Euclid mission of the European Space Agency (ESA), 2024, https://doi.org/10.57780/esa-qmocze3 prov_progenitor = https://euclid.esac.esa.int/dr/ero/ bib_reference_url = https://www.euclid-ec.org/science/publications/ obs_copyright_url = https://www.cosmos.esa.int/web/euclid/ero-credits obs_regime = Infrared em_min = 1.152258e-6 em_max = 1.595197e-6 client_category = Image/Infrared/Euclid ERO hips_builder = Aladin/HipsGen v12.119 + Montage hips_version = 1.4 hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 86.6908333 hips_initial_dec = 0.07916667 hips_initial_fov = 1.2 hips_pixel_scale = 2.795E-5 s_pixel_scale = 2.777E-5 dataproduct_type = image hipsgen_date = 2024-05-23T14:21Z hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwrite treeMean hips_release_date = 2024-05-27T12:41Z hips_tile_format = png fits hips_pixel_cut = 86 1126 hips_data_range = -4956 14919 moc_sky_fraction = 2.721E-4 hips_creation_date = 2024-05-23T16:12Z hips_service_url = https://alasky.cds.unistra.fr/Euclid/ERO/CDS_P_Euclid_ERO_NISP.J hips_service_url_1 = https://alaskybis.cds.unistra.fr/Euclid/ERO/CDS_P_Euclid_ERO_NISP.J hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 12 obs_initial_ra = 86.6908333 obs_initial_dec = 0.07916667 obs_initial_fov = 0.014314526715905856 TIMESTAMP = 1721288496174 ID = CDS/P/Euclid/ERO/NISP.Y hips_doi = 10.26093/cds/aladin/2qzq-awx creator_did = ivo://CDS/P/Euclid/ERO/NISP.Y hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = Euclid ERO NISP.Y obs_collection = Euclid ERO obs_description = The ERO programme is an initiative of ESA and the Euclid Science Team: it includes one day of observations, taken before the start of the nominal survey, to showcase the capabilities of the ESA Euclid mission.Seventeen targets, from galaxy clusters, nearby galaxies, globular clusters, to star-forming regions, have been observed and analyzed. Details on selected ERO projects are available at https://www.cosmos.esa.int/web/euclid/ero-public-release obs_ack = This work has made use of the Early Release Observations (ERO) data from the Euclid mission of the European Space Agency (ESA), 2024, https://doi.org/10.57780/esa-qmocze3 prov_progenitor = https://euclid.esac.esa.int/dr/ero/ bib_reference_url = https://www.euclid-ec.org/science/publications/ obs_copyright_url = https://www.cosmos.esa.int/web/euclid/ero-credits obs_regime = Infrared em_min = 0.938152e-6 em_max = 1.243544e-6 client_category = Image/Infrared/Euclid ERO hips_builder = Aladin/HipsGen v12.119 + Montage hips_version = 1.4 hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 86.6908333 hips_initial_dec = 0.07916667 hips_initial_fov = 1.2 hips_pixel_scale = 2.795E-5 s_pixel_scale = 8.333E-5 dataproduct_type = image hipsgen_date = 2024-05-23T13:22Z hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwriteTile treeMean hips_release_date = 2024-05-27T12:42Z hips_tile_format = png fits hips_pixel_cut = 163.6 1718 hips_data_range = -69736 209628 moc_sky_fraction = 2.718E-4 hips_creation_date = 2024-05-23T13:25Z hips_service_url = https://alasky.cds.unistra.fr/Euclid/ERO/CDS_P_Euclid_ERO_NISP.Y hips_service_url_1 = https://alaskybis.cds.unistra.fr/Euclid/ERO/CDS_P_Euclid_ERO_NISP.Y hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 12 obs_initial_ra = 86.6908333 obs_initial_dec = 0.07916667 obs_initial_fov = 0.014314526715905856 TIMESTAMP = 1721288496118 ID = CDS/P/Euclid/ERO/VIS hips_doi = 10.26093/cds/aladin/bfw5-7z creator_did = ivo://CDS/P/Euclid/ERO/VIS hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = Euclid ERO VIS obs_collection = Euclid ERO obs_description = The ERO programme is an initiative of ESA and the Euclid Science Team: it includes one day of observations, taken before the start of the nominal survey, to showcase the capabilities of the ESA Euclid mission.Seventeen targets, from galaxy clusters, nearby galaxies, globular clusters, to star-forming regions, have been observed and analyzed. Details on selected ERO projects are available at https://www.cosmos.esa.int/web/euclid/ero-public-release obs_ack = This work has made use of the Early Release Observations (ERO) data from the Euclid mission of the European Space Agency (ESA), 2024, https://doi.org/10.57780/esa-qmocze3 prov_progenitor = https://euclid.esac.esa.int/dr/ero/ bib_reference_url = https://www.euclid-ec.org/science/publications/ obs_copyright_url = https://www.cosmos.esa.int/web/euclid/ero-credits obs_regime = Optical em_min = 4.97077e-7 em_max = 9.31759e-7 client_category = Image/Optical/Euclid ERO hips_builder = Aladin/HipsGen v12.119 + Montage hips_version = 1.4 hips_frame = equatorial hips_order = 13 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 86.6908333 hips_initial_dec = 0.07916667 hips_initial_fov = 1.2 hips_pixel_scale = 1.397E-5 s_pixel_scale = 2.777E-5 dataproduct_type = image hipsgen_date = 2024-05-23T13:05Z hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwrite treeMean hips_release_date = 2024-05-27T13:51Z hips_tile_format = png fits hips_pixel_cut = 19.06 59.99 hips_data_range = -4956 14919 moc_sky_fraction = 2.644E-4 hips_creation_date = 2024-05-23T14:33Z hips_service_url = https://alasky.cds.unistra.fr/Euclid/ERO/CDS_P_Euclid_ERO_VIS hips_service_url_1 = https://alaskybis.cds.unistra.fr/Euclid/ERO/CDS_P_Euclid_ERO_VIS hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 13 obs_initial_ra = 86.6908333 obs_initial_dec = 0.07916667 obs_initial_fov = 0.007157263357952928 TIMESTAMP = 1721288496058 ID = CDS/P/Euclid/ERO/color hips_doi = 10.26093/cds/aladin/1byc-byf creator_did = ivo://CDS/P/Euclid/ERO/color hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = Euclid ERO color (filters H, Y, VIS) obs_collection = Euclid ERO obs_description = The ERO programme is an initiative of ESA and the Euclid Science Team: it includes one day of observations, taken before the start of the nominal survey, to showcase the capabilities of the ESA Euclid mission.Seventeen targets, from galaxy clusters, nearby galaxies, globular clusters, to star-forming regions, have been observed and analyzed. Details on selected ERO projects are available at https://www.cosmos.esa.int/web/euclid/ero-public-release . This HiPS has been built by CDS from HiPS CDS/P/Euclid/ERO/NISP.H, CDS/P/Euclid/ERO/NISP.Y and CDS/P/Euclid/ERO/VIS obs_ack = This work has made use of the Early Release Observations (ERO) data from the Euclid mission of the European Space Agency (ESA), 2024, https://doi.org/10.57780/esa-qmocze3 prov_progenitor = https://euclid.esac.esa.int/dr/ero/ bib_reference_url = https://www.euclid-ec.org/science/publications/ obs_copyright_url = https://www.cosmos.esa.int/web/euclid/ero-credits obs_regime = Infrared em_min = 4.97077e-7 em_max = 2.056814e-6 client_category = Image/Infrared/Euclid ERO hips_builder = Aladin/HipsGen v12.119 and Montage hips_version = 1.4 hips_frame = equatorial hips_order = 12 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 86.6908333 hips_initial_dec = 0.07916667 hips_initial_fov = 1.2 hips_pixel_scale = 2.795E-5 s_pixel_scale = 2.777E-5 dataproduct_type = image hipsgen_date = 2024-05-23T14:21Z hips_pixel_bitpix = 0 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwrite treeMean hips_release_date = 2024-05-28T07:14Z hips_tile_format = png hips_pixel_cut = 19.06 59.99 hips_data_range = -4956 14919 moc_sky_fraction = 2.712E-4 hips_creation_date = 2024-05-23T16:12Z dataproduct_subtype = color hips_service_url = https://alasky.cds.unistra.fr/Euclid/ERO/CDS_P_Euclid_ERO_color hips_service_url_1 = https://alaskybis.cds.unistra.fr/Euclid/ERO/CDS_P_Euclid_ERO_color hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 12 obs_initial_ra = 86.6908333 obs_initial_dec = 0.07916667 obs_initial_fov = 0.014314526715905856 TIMESTAMP = 1721288495994 ID = CDS/P/Europa/Voyager-GalileoSSI-500m client_category = Solar system/Jupiter/Europa hips_initial_fov = 180 hips_initial_ra = 0 hips_initial_dec = 0 creator_did = ivo://CDS/P/Europa/Voyager-GalileoSSI-500m hips_overlay = mean hips_hierarchy = median hips_creator = Fernique P. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = Europa Voyager-GalileoSSI-500m obs_description = This global map base of Europa utilizes the best image quality and moderate resolution coverage supplied by the Galileo SSI (Solid-State Imaging) instrument and Voyager 1 and 2. The image processing was performed at the USGS Astrogeology Science Center using the Integrated Software for Imagers and Spectrometers (ISIS2) system. The image data was selected on the basis of overall image quality, reasonable input resolution (from 20 km/pixel for gap fill to as high as 200 meters/pixel), and availability of moderate viewing and sun angles for topography. The map projections are based on a sphere having a radius of 1,562.09 kilometers. prov_progenitor = Planetary Data System, from USGS Astrogeology Science Center prov_progenitor_url = https://astrogeology.usgs.gov/search/map/Europa/Voyager-Galileo/Europa_Voyager_GalileoSSI_global_mosaic_500m bib_reference_url = http://pubs.usgs.gov/imap/i2757/ obs_copyright = Public domain hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T07:03Z hips_frame = europa hips_body = europa hips_order = 3 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg hips_pixel_scale = 0.01431 s_pixel_scale = 0.01834 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 18357 hipsgen_date = 2018-01-17T16:23Z hipsgen_params = -maxthread=10 in=Europa creator_did=CDS/P/Europa/Europa-Voyager-GalilieaSSI-500m -f color=jpg INDEX TILES hips_creation_date = 2018-01-17T16:23Z hipsgen_date_1 = 2018-01-21T12:47Z hipsgen_params_1 = "hhh=Europa/Europa.jpg 19631x9816 9816x9816" partitioning=9816 -maxthread=10 in=Europa creator_did=CDS/P/Europa/Voyager-GalileoSSI-500m -f color=jpg INDEX TILES hips_order_min = 0 dataproduct_subtype = color hipsgen_date_2 = 2019-05-21T07:03Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/Planets/CDS_P_Europa_Voyager-GalileoSSI-500m UPDATE hips_service_url = https://alasky.cds.unistra.fr/Planets/CDS_P_Europa_Voyager-GalileoSSI-500m hips_service_url_1 = https://alaskybis.cds.unistra.fr/Planets/CDS_P_Europa_Voyager-GalileoSSI-500m hips_status_1 = public mirror clonableOnce client_application = AladinDesktopBeta>=10.040 AladinDesktop>=11.125 moc_type = smoc moc_order = 3 obs_initial_ra = 0 obs_initial_dec = 0 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288466926 ID = CDS/P/FDS/DR1/color hips_doi = 10.26093/cds/aladin/2pt5-dgy creator_did = ivo://CDS/P/FDS/DR1/color hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = Fornax Deep Survey (FDS) color obs_collection = Fornax Deep Survey (FDS) obs_description = This FDS color HiPS has been built from bands i' (red channel), r? (green) and g' (blue) bands.\n The Fornax Deep Survey (FDS) Survey is an imaging survey in 4 bands,using the wide-field imager OmegaCAM mounted on the VST in the SDSS u', g', r', and i'-bands of about 30 degrees² covering the Fornax Galaxy Cluster and the infalling Fornax A Group down to a surface brightness limit of ~28 mag/arcsec² (1-sigma surface brightness over a 1 arcsecond² area). FDS is a joint project that used the VST-GTO time of NOVA (previously called FOCUS - PI: R. F. Peletier) and INAF (as part of VEGAS - PIs: M. Capaccioli and E. Iodice). obs_ack = Based on data obtained from the ESO Science Archive Facility with DOI(s): https://doi.eso.org/10.18727/archive/23 . The FDS data were produced by the FDS collaboration. prov_progenitor = ESO Science Archive ( https://archive.eso.org/scienceportal/home?publ_date=2020-08-26 ) bib_reference = 10.48550/arXiv.2008.12633 bib_reference_url = https://doi.org/10.48550/arXiv.2008.12633 obs_copyright = All data in the ESO archive retain ESO's copyright, and are distributed according to the terms of the Creative Commons Attribution 4.0 International license (CC BY 4.0). obs_copyright_url = http://archive.eso.org/cms/eso-data-access-policy.html client_category = Image/Optical/FDS obs_regime = Optical em_min = 3.91271e-7 em_max = 8.74145e-7 hips_builder = Aladin/HipsGen v12.060 hips_version = 1.4 hips_frame = equatorial hips_order = 12 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 50.6941250 hips_initial_dec = -36.8862186 hips_initial_fov = 2.1 hips_pixel_scale = 0.229 s_pixel_scale = 5.555E-5 dataproduct_type = image dataproduct_subtype = color hips_release_date = 2023-07-31T09:05Z hips_tile_format = png moc_sky_fraction = 6.587E-4 hips_creation_date = 2023-07-31T08:47Z hips_service_url = https://alasky.cds.unistra.fr/FDS/CDS_P_FDS_DR1_color hips_service_url_1 = https://alaskybis.cds.unistra.fr/FDS/CDS_P_FDS_DR1_color hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 12 obs_initial_ra = 50.6941250 obs_initial_dec = -36.8862186 obs_initial_fov = 0.014314526715905856 TIMESTAMP = 1721288495482 ID = CDS/P/FDS/DR1/g hips_doi = 10.26093/cds/aladin/20c2-y44 creator_did = ivo://CDS/P/FDS/DR1/g hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = Fornax Deep Survey (FDS) g' band obs_collection = Fornax Deep Survey (FDS) obs_description = The Fornax Deep Survey (FDS) Survey is an imaging survey in 4 bands,using the wide-field imager OmegaCAM mounted on the VST in the SDSS u', g', r', and i'-bands of about 30 degrees² covering the Fornax Galaxy Cluster and the infalling Fornax A Group down to a surface brightness limit of ~28 mag/arcsec² (1-sigma surface brightness over a 1 arcsecond² area). FDS is a joint project that used the VST-GTO time of NOVA (previously called FOCUS - PI: R. F. Peletier) and INAF (as part of VEGAS - PIs: M. Capaccioli and E. Iodice). obs_ack = Based on data obtained from the ESO Science Archive Facility with DOI(s): https://doi.eso.org/10.18727/archive/23 . The FDS data were produced by the FDS collaboration. prov_progenitor = ESO Science Archive ( https://archive.eso.org/scienceportal/home?publ_date=2020-08-26 ) bib_reference = 10.48550/arXiv.2008.12633 bib_reference_url = https://doi.org/10.48550/arXiv.2008.12633 obs_copyright = All data in the ESO archive retain ESO's copyright, and are distributed according to the terms of the Creative Commons Attribution 4.0 International license (CC BY 4.0). obs_copyright_url = http://archive.eso.org/cms/eso-data-access-policy.html client_category = Image/Optical/FDS t_min = 55865.311074 t_max = 57717.197638 obs_regime = Optical em_min = 3.91271e-7 em_max = 5.57293e-7 hips_builder = Aladin/HipsGen v12.060 hips_version = 1.4 hips_frame = equatorial hips_order = 12 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 50.6941250 hips_initial_dec = -36.8862186 hips_initial_fov = 2.1 hips_pixel_scale = 2.795E-5 s_pixel_scale = 5.555E-5 dataproduct_type = image hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwriteTile treeMean hips_release_date = 2023-08-03T11:07Z hips_tile_format = png fits hips_pixel_cut = -3.0E-12 2.0E-10 hips_data_range = -6.591E-9 1.976E-8 moc_sky_fraction = 6.788E-4 hipsgen_date = 2023-07-31T08:47Z hipsgen_params = cache=./tmp in=data/g id=CDS/P/FDS/DR1/g out=./hips/CDS_P_FDS_DR1_g TILES hips_creation_date = 2023-07-31T08:47Z hipsgen_date_1 = 2023-07-31T09:05Z hipsgen_params_1 = cache=./tmp in=data/g id=CDS/P/FDS/DR1/g out=./hips/CDS_P_FDS_DR1_g "pixelCut=-3e-12 2e-10 log" mode=median PNG -clean hipsgen_date_2 = 2023-08-03T07:31Z hipsgen_params_2 = cache=./tmp in=data/g id=CDS/P/FDS/DR1/g out=./hips/CDS_P_FDS_DR1_g "pixelCut=-3e-12 2e-10 log" mode=median PNG hipsgen_date_3 = 2023-08-03T11:07Z hipsgen_params_3 = cache=./tmp in=data/g id=CDS/P/FDS/DR1/g out=./hips/CDS_P_FDS_DR1_g "pixelCut=-3e-12 2e-10 log" mode=mean PNG hips_service_url = https://alasky.cds.unistra.fr/FDS/CDS_P_FDS_DR1_g hips_progenitor_url = https://alasky.cds.unistra.fr/FDS/CDS_P_FDS_DR1_g/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/FDS/CDS_P_FDS_DR1_g hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 12 obs_initial_ra = 50.6941250 obs_initial_dec = -36.8862186 obs_initial_fov = 0.014314526715905856 TIMESTAMP = 1721288495538 ID = CDS/P/FDS/DR1/i hips_doi = 10.26093/cds/aladin/1kqj-nc3 creator_did = ivo://CDS/P/FDS/DR1/i hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = Fornax Deep Survey (FDS) i' band obs_collection = Fornax Deep Survey (FDS) obs_description = The Fornax Deep Survey (FDS) Survey is an imaging survey in 4 bands,using the wide-field imager OmegaCAM mounted on the VST in the SDSS u', g', r', and i'-bands of about 30 degrees² covering the Fornax Galaxy Cluster and the infalling Fornax A Group down to a surface brightness limit of ~28 mag/arcsec² (1-sigma surface brightness over a 1 arcsecond² area). FDS is a joint project that used the VST-GTO time of NOVA (previously called FOCUS - PI: R. F. Peletier) and INAF (as part of VEGAS - PIs: M. Capaccioli and E. Iodice). obs_ack = Based on data obtained from the ESO Science Archive Facility with DOI(s): https://doi.eso.org/10.18727/archive/23 . The FDS data were produced by the FDS collaboration. prov_progenitor = ESO Science Archive ( https://archive.eso.org/scienceportal/home?publ_date=2020-08-26 ) bib_reference = 10.48550/arXiv.2008.12633 bib_reference_url = https://doi.org/10.48550/arXiv.2008.12633 obs_copyright = All data in the ESO archive retain ESO's copyright, and are distributed according to the terms of the Creative Commons Attribution 4.0 International license (CC BY 4.0). obs_copyright_url = http://archive.eso.org/cms/eso-data-access-policy.html client_category = Image/Optical/FDS t_min = 56974.22476186 t_max = 58084.251340278 obs_regime = Optical em_min = 6.58008e-7 em_max = 8.74145e-7 hips_builder = Aladin/HipsGen v12.060 hips_version = 1.4 hips_frame = equatorial hips_order = 12 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 50.6941250 hips_initial_dec = -36.8862186 hips_initial_fov = 2.1 hips_pixel_scale = 2.795E-5 s_pixel_scale = 5.555E-5 dataproduct_type = image hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwrite treeMean hips_release_date = 2023-08-03T13:06Z hips_tile_format = png fits hips_pixel_cut = -8.0E-12 6.0E-10 hips_data_range = -1.331E-8 3.987E-8 moc_sky_fraction = 6.587E-4 hipsgen_date = 2023-07-31T11:03Z hipsgen_params = cache=./tmp in=data/i id=CDS/P/FDS/DR1/i out=./hips/CDS_P_FDS_DR1_i TILES hips_creation_date = 2023-07-31T11:03Z hipsgen_date_1 = 2023-07-31T13:53Z hipsgen_params_1 = cache=./tmp in=data/i id=CDS/P/FDS/DR1/i out=./hips/CDS_P_FDS_DR1_i TILES hipsgen_date_2 = 2023-08-03T13:06Z hipsgen_params_2 = cache=./tmp in=data/i id=CDS/P/FDS/DR1/i out=./hips/CDS_P_FDS_DR1_i "pixelCut=-8e-12 6e-10 log" mode=mean PNG hips_service_url = https://alasky.cds.unistra.fr/FDS/CDS_P_FDS_DR1_i hips_progenitor_url = https://alasky.cds.unistra.fr/FDS/CDS_P_FDS_DR1_i/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/FDS/CDS_P_FDS_DR1_i hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 12 obs_initial_ra = 50.6941250 obs_initial_dec = -36.8862186 obs_initial_fov = 0.014314526715905856 TIMESTAMP = 1721288495650 ID = CDS/P/FDS/DR1/r hips_doi = 10.26093/cds/aladin/3phs-73f creator_did = ivo://CDS/P/FDS/DR1/r hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = Fornax Deep Survey (FDS) r' band obs_collection = Fornax Deep Survey (FDS) obs_description = The Fornax Deep Survey (FDS) Survey is an imaging survey in 4 bands,using the wide-field imager OmegaCAM mounted on the VST in the SDSS u', g', r', and i'-bands of about 30 degrees² covering the Fornax Galaxy Cluster and the infalling Fornax A Group down to a surface brightness limit of ~28 mag/arcsec² (1-sigma surface brightness over a 1 arcsecond² area). FDS is a joint project that used the VST-GTO time of NOVA (previously called FOCUS - PI: R. F. Peletier) and INAF (as part of VEGAS - PIs: M. Capaccioli and E. Iodice). obs_ack = Based on data obtained from the ESO Science Archive Facility with DOI(s): https://doi.eso.org/10.18727/archive/23 . The FDS data were produced by the FDS collaboration. prov_progenitor = ESO Science Archive ( https://archive.eso.org/scienceportal/home?publ_date=2020-08-26 ) bib_reference = 10.48550/arXiv.2008.12633 bib_reference_url = https://doi.org/10.48550/arXiv.2008.12633 obs_copyright = All data in the ESO archive retain ESO's copyright, and are distributed according to the terms of the Creative Commons Attribution 4.0 International license (CC BY 4.0). obs_copyright_url = http://archive.eso.org/cms/eso-data-access-policy.html client_category = Image/Optical/FDS t_min = 55864.281561031 t_max = 57718.048615268 obs_regime = Optical em_min = 5.40542e-7 em_max = 7.24473e-7 hips_builder = Aladin/HipsGen v12.060 hips_version = 1.4 hips_frame = equatorial hips_order = 12 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 50.6941250 hips_initial_dec = -36.8862186 hips_initial_fov = 2.1 hips_pixel_scale = 2.795E-5 s_pixel_scale = 5.555E-5 dataproduct_type = image hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwriteTile treeMean hips_release_date = 2023-08-03T08:52Z hips_tile_format = png fits hips_pixel_cut = -8.0E-12 5.0E-10 hips_data_range = -3.014E-9 9.018E-9 moc_sky_fraction = 6.745E-4 hipsgen_date = 2023-07-31T11:09Z hipsgen_params = cache=./tmp in=data/r id=CDS/P/FDS/DR1/r out=./hips/CDS_P_FDS_DR1_r TILES hips_creation_date = 2023-07-31T11:09Z hipsgen_date_1 = 2023-08-03T08:52Z hipsgen_params_1 = cache=./tmp in=data/r id=CDS/P/FDS/DR1/r out=./hips/CDS_P_FDS_DR1_r "pixelCut=-8e-12 5e-10 log" mode=mean PNG hips_service_url = https://alasky.cds.unistra.fr/FDS/CDS_P_FDS_DR1_r hips_progenitor_url = https://alasky.cds.unistra.fr/FDS/CDS_P_FDS_DR1_r/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/FDS/CDS_P_FDS_DR1_r hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 12 obs_initial_ra = 50.6941250 obs_initial_dec = -36.8862186 obs_initial_fov = 0.014314526715905856 TIMESTAMP = 1721288495590 ID = CDS/P/FDS/DR1/u hips_doi = 10.26093/cds/aladin/1sqg-2ec creator_did = ivo://CDS/P/FDS/DR1/u hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = Fornax Deep Survey (FDS) u' band obs_collection = Fornax Deep Survey (FDS) obs_description = The Fornax Deep Survey (FDS) Survey is an imaging survey in 4 bands,using the wide-field imager OmegaCAM mounted on the VST in the SDSS u', g', r', and i'-bands of about 30 degrees² covering the Fornax Galaxy Cluster and the infalling Fornax A Group down to a surface brightness limit of ~28 mag/arcsec² (1-sigma surface brightness over a 1 arcsecond² area). FDS is a joint project that used the VST-GTO time of NOVA (previously called FOCUS - PI: R. F. Peletier) and INAF (as part of VEGAS - PIs: M. Capaccioli and E. Iodice). obs_ack = Based on data obtained from the ESO Science Archive Facility with DOI(s): https://doi.eso.org/10.18727/archive/23 . The FDS data were produced by the FDS collaboration. prov_progenitor = ESO Science Archive ( https://archive.eso.org/scienceportal/home?publ_date=2020-08-26 ) bib_reference = 10.48550/arXiv.2008.12633 bib_reference_url = https://doi.org/10.48550/arXiv.2008.12633 obs_copyright = All data in the ESO archive retain ESO's copyright, and are distributed according to the terms of the Creative Commons Attribution 4.0 International license (CC BY 4.0). obs_copyright_url = http://archive.eso.org/cms/eso-data-access-policy.html client_category = Image/Optical/FDS t_min = 56598.217182819 t_max = 58085.355686761 obs_regime = Optical em_min = 3.20744e-7 em_max = 4.00294e-7 hips_builder = Aladin/HipsGen v12.060 hips_version = 1.4 hips_frame = equatorial hips_order = 12 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 53.3980220 hips_initial_dec = -36.1509186 hips_initial_fov = 2.1 hips_pixel_scale = 2.795E-5 s_pixel_scale = 5.555E-5 dataproduct_type = image hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwriteTile treeMean hips_release_date = 2023-08-03T13:46Z hips_tile_format = png fits hips_pixel_cut = -4.0E-13 1.0E-10 hips_data_range = -1.420E-9 4.224E-9 moc_sky_fraction = 5.318E-4 hipsgen_date = 2023-07-31T11:53Z hipsgen_params = cache=./tmp in=data/u id=CDS/P/FDS/DR1/u out=./hips/CDS_P_FDS_DR1_u TILES hips_creation_date = 2023-07-31T11:53Z hipsgen_date_1 = 2023-08-03T13:46Z hipsgen_params_1 = cache=./tmp in=data/u id=CDS/P/FDS/DR1/u out=./hips/CDS_P_FDS_DR1_u "pixelCut=-4e-13 1e-10 log" mode=mean PNG hips_service_url = https://alasky.cds.unistra.fr/FDS/CDS_P_FDS_DR1_u hips_progenitor_url = https://alasky.cds.unistra.fr/FDS/CDS_P_FDS_DR1_u/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/FDS/CDS_P_FDS_DR1_u hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 12 obs_initial_ra = 53.3980220 obs_initial_dec = -36.1509186 obs_initial_fov = 0.014314526715905856 TIMESTAMP = 1721288495702 ID = CDS/P/Fermi/3 hips_doi = 10.26093/cds/aladin/3q2w-3mk creator_did = ivo://CDS/P/Fermi/3 obs_collection = Fermi3 300-1000MeV obs_title = Fermi 300-1000MeV HEALPix survey obs_description = Launched on June 11, 2008, the Fermi Gamma-ray Space Telescope observes the cosmos using the highest-energy form of light. This survey sums all data observed by the Fermi mission up to week 396. This version of the Fermi survey are intensity maps where the summed counts maps are divided by the exposure for each pixel. We anticipate using the HEASARC's Hera capabilities to update this survey on a roughly quarterly basis. Data is broken into 5 energy bands : 30-100 MeV Band 1, 100-300 MeV Band 2, 300-1000 MeV Band 3, 1-3 GeV Band 4 , 3-300 GeV Band 5. The SkyView data are based upon a Cartesian projection of the counts divided by the exposure maps. In the Cartesian projection pixels near the pole have a much smaller area than pixels on the equator, so these pixels have smaller integrated flux. When creating large scale images in other projections users may wish to make sure to compensate for this effect the flux conserving clip-resampling option. obs_copyright = Distributed by SkyView/HEASARC - HEALPixed by CDS client_category = Image/Gamma-ray client_sort_key = 00-01-04 hips_creation_date = 2013-06-28T08:03Z hips_release_date = 2019-05-05T06:04Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Boch T. (CDS) hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_format = jpeg fits dataproduct_type = image moc_access_url = http://alasky.u-strasbg.fr/Fermi/300-1000MeV/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = This research has made use of data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory's High Energy Astrophysics Division prov_progenitor = NASA/HEASARC bib_reference = 2009ApJ...697.1071A bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2009ApJ...697.1071A obs_copyright_url = http://skyview.gsfc.nasa.gov/current/cgi/survey.pl t_min = 54628 t_max = 56291 obs_regime = Gamma-ray em_min = 1.2398e-15 em_max = 4.1328e-15 hips_tile_width = 512 hips_pixel_scale = 0.01431 hips_initial_fov = 150.0 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 1112337 hipsgen_date = 2019-05-05T06:04Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/Fermi/300-1000MeV UPDATE hips_service_url = https://alasky.cds.unistra.fr/Fermi/300-1000MeV hips_service_url_1 = https://alaskybis.cds.unistra.fr/Fermi/300-1000MeV hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288415254 ID = CDS/P/Fermi/4 hips_doi = 10.26093/cds/aladin/1r4n-6sg creator_did = ivo://CDS/P/Fermi/4 obs_collection = Fermi4 1-3GeV obs_title = Fermi 1-3GeV HEALPix survey. obs_description = Launched on June 11, 2008, the Fermi Gamma-ray Space Telescope observes the cosmos using the highest-energy form of light. This survey sums all data observed by the Fermi mission up to week 396. This version of the Fermi survey are intensity maps where the summed counts maps are divided by the exposure for each pixel. We anticipate using the HEASARC's Hera capabilities to update this survey on a roughly quarterly basis. Data is broken into 5 energy bands : 30-100 MeV Band 1, 100-300 MeV Band 2, 300-1000 MeV Band 3, 1-3 GeV Band 4 , 3-300 GeV Band 5. The SkyView data are based upon a Cartesian projection of the counts divided by the exposure maps. In the Cartesian projection pixels near the pole have a much smaller area than pixels on the equator, so these pixels have smaller integrated flux. When creating large scale images in other projections users may wish to make sure to compensate for this effect the flux conserving clip-resampling option. obs_copyright = Distributed by SkyView/HEASARC - HEALPixed by CDS client_category = Image/Gamma-ray client_sort_key = 00-01-03 hips_creation_date = 2013-06-28T08:28Z hips_release_date = 2019-05-05T06:05Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Boch T. (CDS) hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_format = jpeg fits dataproduct_type = image moc_access_url = http://alasky.u-strasbg.fr/Fermi/1-3GeV/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = This research has made use of data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory's High Energy Astrophysics Division prov_progenitor = NASA/HEASARC bib_reference = 2009ApJ...697.1071A bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2009ApJ...697.1071A obs_copyright_url = http://skyview.gsfc.nasa.gov/current/cgi/survey.pl t_min = 54628 t_max = 56291 obs_regime = Gamma-ray em_min = 4.1328e-16 em_max = 1.2398e-15 hips_tile_width = 512 hips_pixel_scale = 0.01431 hips_initial_fov = 150.0 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 1112337 hipsgen_date = 2019-05-05T06:05Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/Fermi/1-3GeV UPDATE hips_service_url = https://alasky.cds.unistra.fr/Fermi/1-3GeV hips_service_url_1 = https://alaskybis.cds.unistra.fr/Fermi/1-3GeV hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288415310 ID = CDS/P/Fermi/5 hips_doi = 10.26093/cds/aladin/3mva-x6 creator_did = ivo://CDS/P/Fermi/5 obs_collection = Fermi5 3-300GeV obs_title = Fermi 3-300GeV HEALPix survey obs_description = Launched on June 11, 2008, the Fermi Gamma-ray Space Telescope observes the cosmos using the highest-energy form of light. This survey sums all data observed by the Fermi mission up to week 396. This version of the Fermi survey are intensity maps where the summed counts maps are divided by the exposure for each pixel. We anticipate using the HEASARC's Hera capabilities to update this survey on a roughly quarterly basis. Data is broken into 5 energy bands : 30-100 MeV Band 1, 100-300 MeV Band 2, 300-1000 MeV Band 3, 1-3 GeV Band 4 , 3-300 GeV Band 5. The SkyView data are based upon a Cartesian projection of the counts divided by the exposure maps. In the Cartesian projection pixels near the pole have a much smaller area than pixels on the equator, so these pixels have smaller integrated flux. When creating large scale images in other projections users may wish to make sure to compensate for this effect the flux conserving clip-resampling option. obs_copyright = Distributed by SkyView/HEASARC - HEALPixed by CDS client_category = Image/Gamma-ray client_sort_key = 00-01-02 hips_creation_date = 2013-06-28T09:09Z hips_release_date = 2019-05-05T06:05Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Boch T. (CDS) hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_format = jpeg fits dataproduct_type = image moc_access_url = http://alasky.u-strasbg.fr/Fermi/3-300GeV/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = This research has made use of data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory's High Energy Astrophysics Division prov_progenitor = NASA/HEASARC bib_reference = 2009ApJ...697.1071A bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2009ApJ...697.1071A obs_copyright_url = http://skyview.gsfc.nasa.gov/current/cgi/survey.pl t_min = 54628 t_max = 56291 obs_regime = Gamma-ray em_min = 4.1328e-18 em_max = 4.1328e-16 hips_tile_width = 512 hips_pixel_scale = 0.01431 hips_initial_fov = 150.0 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 1112337 hipsgen_date = 2019-05-05T06:05Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/Fermi/3-300GeV UPDATE hips_service_url = https://alasky.cds.unistra.fr/Fermi/3-300GeV hips_service_url_1 = https://alaskybis.cds.unistra.fr/Fermi/3-300GeV hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288415366 ID = CDS/P/Fermi/color hips_doi = 10.26093/cds/aladin/276y-1xd creator_did = ivo://CDS/P/Fermi/color obs_collection = Fermi color obs_title = Fermi Color HEALPix survey obs_description = Launched on June 11, 2008, the Fermi Gamma-ray Space Telescope observes the cosmos using the highest-energy form of light. This survey sums all data observed by the Fermi mission up to week 396. This version of the Fermi survey are intensity maps where the summed counts maps are divided by the exposure for each pixel. We anticipate using the HEASARC's Hera capabilities to update this survey on a roughly quarterly basis. Data is broken into 5 energy bands : 30-100 MeV Band 1, 100-300 MeV Band 2, 300-1000 MeV Band 3, 1-3 GeV Band 4 , 3-300 GeV Band 5. The SkyView data are based upon a Cartesian projection of the counts divided by the exposure maps. In the Cartesian projection pixels near the pole have a much smaller area than pixels on the equator, so these pixels have smaller integrated flux. When creating large scale images in other projections users may wish to make sure to compensate for this effect the flux conserving clip-resampling option. obs_copyright = Distributed by SkyView/HEASARC - HEALPixed by CDS client_category = Image/Gamma-ray client_sort_key = 00-01-01 hips_creation_date = 2013-06-28T11:09Z hips_release_date = 2019-05-05T06:06Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Boch T. (CDS) hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_format = jpeg dataproduct_type = image hips_rgb_red = 300-1000MeVALLSKY~1 [0.0 10.0 20.0 Sqrt] hips_rgb_green = 1-3GeVALLSKY~1 [0.0 5.0 10.0 Sqrt] hips_rgb_blue = 3-300GeVALLSKY [0.0 2.0 4.0 Sqrt] client_application = AladinLite client_application = AladinDesktop moc_access_url = http://alasky.u-strasbg.fr/Fermi/Color/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = This research has made use of data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory's High Energy Astrophysics Division prov_progenitor = NASA/HEASARC bib_reference = 2009ApJ...697.1071A bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2009ApJ...697.1071A obs_copyright_url = http://skyview.gsfc.nasa.gov/current/cgi/survey.pl t_min = 54628 t_max = 56291 obs_regime = Gamma-ray em_min = 4.1328e-18 em_max = 4.1328e-15 hips_tile_width = 512 hips_pixel_scale = 0.01431 hips_initial_fov = 150.0 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_order_min = 0 dataproduct_subtype = color moc_sky_fraction = 1 hips_estsize = 9182 hipsgen_date = 2019-05-05T06:06Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/Fermi/Color UPDATE hips_service_url = https://alasky.cds.unistra.fr/Fermi/Color hips_service_url_1 = https://alaskybis.cds.unistra.fr/Fermi/Color hips_status_1 = public mirror clonableOnce hips_service_url_2 = https://healpix.ias.u-psud.fr/CDS_P_Fermi_color hips_status_2 = public mirror unclonable hips_service_url_3 = http://skies.esac.esa.int/FermiColor hips_status_3 = public mirror unclonable moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1729584619409 ID = CDS/P/Finkbeiner hips_doi = 10.26093/cds/aladin/3a4t-avb creator_did = ivo://CDS/P/Finkbeiner obs_collection = Finkbeiner Halpha obs_title = Finkbeiner Halpha composite survey obs_description = D. Finkbeiner has assembled a full sky Halpha map using data from several surveys: the Wisconsin H-Alpha Mapper (WHAM), the Virginia Tech Spectral-Line Survey (VTSS), and the Southern H-Alpha Sky Survey Atlas (SHASSA). The composite map can be used to provide limits on free-free foreground emission. obs_copyright = Composite map by Douglas Finkbeiner (2004). client_category = Image/Gas-lines/Halpha client_sort_key = 06-01 hips_creation_date = 2010-12-14T01:07Z hips_release_date = 2019-05-05T06:07Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 3 hips_frame = galactic hips_tile_width = 128 hips_tile_format = jpeg fits hips_pixel_cut = -10 800 dataproduct_type = image client_application = AladinLite client_application = AladinDesktop moc_access_url = http://alasky.u-strasbg.fr/FinkbeinerHalpha/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = All of these data products are available to the public on the World Wide Web prov_progenitor = The data can be found as an on line material in the reference 2003ApJS..146..407F bib_reference = 2003ApJS..146..407F bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2003ApJS..146..407F t_min = 50753 t_max = 51818 obs_regime = Optical em_min = 48E-8 em_max = 73E-8 hips_pixel_scale = 0.01431 hips_initial_fov = 150.0 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 1112337 hipsgen_date = 2019-05-05T06:07Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/FinkbeinerHalpha UPDATE hips_service_url = https://alasky.cds.unistra.fr/FinkbeinerHalpha hips_service_url_1 = https://alaskybis.cds.unistra.fr/FinkbeinerHalpha hips_status_1 = public mirror clonableOnce hips_service_url_2 = http://skies.esac.esa.int/FinkbeinerHa hips_status_2 = public mirror unclonable moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288732541 ID = CDS/P/GALACTICNUCLEUS/DR1/H hips_doi = 10.26093/cds/aladin/f9cc-d0 creator_did = ivo://CDS/P/GALACTICNUCLEUS/DR1/H hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = GALACTICNUCLEUS DR1 H obs_collection = GALACTICNUCLEUS obs_description = The GALACTICNUCLEUS (GNS) survey is a single-epoch catalog of the Galactic Centre in the near-infrared bands JHKs. The observations were optimised for the Galactic Center: high angular resolution (0.2") to overcome extreme crowding and high dynamic range to minimise saturation issues. The data were acquired with the HAWK-I intrument at the ESO VLT unit telescope 4. The catalogue covers an area of ~0.3 square degrees (~6000 square pc) distributed across seven regions that correspond to the nuclear stellar disc (NSD), the inner Galactic Bulge and the transition region between them. obs_ack = Based on data obtained from the ESO Science Archive Facility with DOI(s): https://doi.org/10.18727/archive/9 . prov_progenitor = ESO Science Archive ( https://archive.eso.org/scienceportal/home?data_collection=195.B-0283 ) bib_reference = 10.1051/0004-6361/201936263 bib_reference_url = https://doi.org/10.1051/0004-6361/201936263 obs_copyright = All data in the ESO archive retain ESO's copyright, and are distributed according to the terms of the Creative Commons Attribution 4.0 International license (CC BY 4.0). obs_copyright_url = http://archive.eso.org/cms/eso-data-access-policy.html t_min = 57836.0 t_max = 58589.0 obs_regime = Infrared em_min = 1.443053e-6 em_max = 1.807710e-6 hips_builder = Aladin/HipsGen v12.132 hips_version = 1.4 hips_frame = equatorial hips_order = 13 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 266.415009 hips_initial_dec = -29.0061110 hips_initial_fov = 1.5 hips_pixel_scale = 1.397E-5 s_pixel_scale = 1.476E-5 dataproduct_type = image hipsgen_date = 2024-04-22T09:11Z hipsgen_params = in=data/H out=./hips/ id=CDS/P/GALACTICNUCLEUS/DR1/H exptime=EXPTIME TILES hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwriteTile treeMean hips_release_date = 2024-04-22T09:12Z hips_tile_format = png fits hips_pixel_cut = -37.67 6724 hips_data_range = -39326 106449 hips_data_minmax = -303894 254787 moc_sky_fraction = 8.023E-6 hips_service_url = https://alasky.cds.unistra.fr/GALACTICNUCLEUS/CDS_P_GALACTICNUCLEUS_DR1_H hips_service_url_1 = https://alaskybis.cds.unistra.fr/GALACTICNUCLEUS/CDS_P_GALACTICNUCLEUS_DR1_H hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 13 obs_initial_ra = 266.415009 obs_initial_dec = -29.0061110 obs_initial_fov = 0.007157263357952928 TIMESTAMP = 1721288498614 ID = CDS/P/GALACTICNUCLEUS/DR1/J hips_doi = 10.26093/cds/aladin/3r9g-m4c creator_did = ivo://CDS/P/GALACTICNUCLEUS/DR1/J hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = GALACTICNUCLEUS DR1 J obs_collection = GALACTICNUCLEUS obs_description = The GALACTICNUCLEUS (GNS) survey is a single-epoch catalog of the Galactic Centre in the near-infrared bands JHKs. The observations were optimised for the Galactic Center: high angular resolution (0.2") to overcome extreme crowding and high dynamic range to minimise saturation issues. The data were acquired with the HAWK-I intrument at the ESO VLT unit telescope 4. The catalogue covers an area of ~0.3 square degrees (~6000 square pc) distributed across seven regions that correspond to the nuclear stellar disc (NSD), the inner Galactic Bulge and the transition region between them. obs_ack = Based on data obtained from the ESO Science Archive Facility with DOI(s): https://doi.org/10.18727/archive/9 . prov_progenitor = ESO Science Archive ( https://archive.eso.org/scienceportal/home?data_collection=195.B-0283 ) bib_reference = 10.1051/0004-6361/201936263 bib_reference_url = https://doi.org/10.1051/0004-6361/201936263 obs_copyright = All data in the ESO archive retain ESO's copyright, and are distributed according to the terms of the Creative Commons Attribution 4.0 International license (CC BY 4.0). obs_copyright_url = http://archive.eso.org/cms/eso-data-access-policy.html t_min = 57836.0 t_max = 58595.0 obs_regime = Infrared em_min = 1.158165e-6 em_max = 1.360190e-6 hips_builder = Aladin/HipsGen v12.132 hips_version = 1.4 hips_frame = equatorial hips_order = 13 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 266.415009 hips_initial_dec = -29.0061110 hips_initial_fov = 1.5 hips_pixel_scale = 1.397E-5 s_pixel_scale = 1.477E-5 dataproduct_type = image hipsgen_date = 2024-04-22T09:10Z hipsgen_params = in=data/J out=./hips/ id=CDS/P/GALACTICNUCLEUS/DR1/J exptime=EXPTIME TILES hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwriteTile treeMean hips_release_date = 2024-04-22T09:11Z hips_tile_format = png fits hips_pixel_cut = -24.3 1047 hips_data_range = -5440 14819 hips_data_minmax = -57430 90620 moc_sky_fraction = 8.172E-6 hips_service_url = https://alasky.cds.unistra.fr/GALACTICNUCLEUS/CDS_P_GALACTICNUCLEUS_DR1_J hips_service_url_1 = https://alaskybis.cds.unistra.fr/GALACTICNUCLEUS/CDS_P_GALACTICNUCLEUS_DR1_J hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 13 obs_initial_ra = 266.415009 obs_initial_dec = -29.0061110 obs_initial_fov = 0.007157263357952928 TIMESTAMP = 1721288498558 ID = CDS/P/GALACTICNUCLEUS/DR1/Ks hips_doi = 10.26093/cds/aladin/3keq-a8h creator_did = ivo://CDS/P/GALACTICNUCLEUS/DR1/Ks hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = GALACTICNUCLEUS DR1 Ks obs_collection = GALACTICNUCLEUS obs_description = The GALACTICNUCLEUS (GNS) survey is a single-epoch catalog of the Galactic Centre in the near-infrared bands JHKs. The observations were optimised for the Galactic Center: high angular resolution (0.2") to overcome extreme crowding and high dynamic range to minimise saturation issues. The data were acquired with the HAWK-I intrument at the ESO VLT unit telescope 4. The catalogue covers an area of ~0.3 square degrees (~6000 square pc) distributed across seven regions that correspond to the nuclear stellar disc (NSD), the inner Galactic Bulge and the transition region between them. obs_ack = Based on data obtained from the ESO Science Archive Facility with DOI(s): https://doi.org/10.18727/archive/9 . prov_progenitor = ESO Science Archive ( https://archive.eso.org/scienceportal/home?data_collection=195.B-0283 ) bib_reference = 10.1051/0004-6361/201936263 bib_reference_url = https://doi.org/10.1051/0004-6361/201936263 obs_copyright = All data in the ESO archive retain ESO's copyright, and are distributed according to the terms of the Creative Commons Attribution 4.0 International license (CC BY 4.0). obs_copyright_url = http://archive.eso.org/cms/eso-data-access-policy.html t_min = 57836.0 t_max = 58589.0 obs_regime = Infrared em_min = 1.936971e-6 em_max = 2.372430e-6 hips_builder = Aladin/HipsGen v12.132 hips_version = 1.4 hips_frame = equatorial hips_order = 13 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 266.415009 hips_initial_dec = -29.0061110 hips_initial_fov = 1.5 hips_pixel_scale = 1.397E-5 s_pixel_scale = 1.477E-5 dataproduct_type = image hipsgen_date = 2024-04-22T09:13Z hipsgen_params = in=data/Ks out=./hips/ id=CDS/P/GALACTICNUCLEUS/DR1/Ks exptime=EXPTIME TILES hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwriteTile treeMean hips_release_date = 2024-04-22T09:14Z hips_tile_format = png fits hips_pixel_cut = -5.691 10571 hips_data_range = -32584 85862 hips_data_minmax = -107289 220226 moc_sky_fraction = 8.200E-6 hips_service_url = https://alasky.cds.unistra.fr/GALACTICNUCLEUS/CDS_P_GALACTICNUCLEUS_DR1_Ks hips_service_url_1 = https://alaskybis.cds.unistra.fr/GALACTICNUCLEUS/CDS_P_GALACTICNUCLEUS_DR1_Ks hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 13 obs_initial_ra = 266.415009 obs_initial_dec = -29.0061110 obs_initial_fov = 0.007157263357952928 TIMESTAMP = 1721288498670 ID = CDS/P/GALACTICNUCLEUS/DR1/color hips_doi = 10.26093/cds/aladin/1e6b-x9x hips_initial_ra = 266.415009 hips_initial_dec = -29.0061110 hips_initial_fov = 1.5 creator_did = ivo://CDS/P/GALACTICNUCLEUS/DR1/color hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = GALACTICNUCLEUS DR1 color (from bands Ks, H, J) obs_collection = GALACTICNUCLEUS obs_description = The GALACTICNUCLEUS (GNS) survey is a single-epoch catalog of the Galactic Centre in the near-infrared bands JHKs. The observations were optimised for the Galactic Center: high angular resolution (0.2") to overcome extreme crowding and high dynamic range to minimise saturation issues. The data were acquired with the HAWK-I intrument at the ESO VLT unit telescope 4. The catalogue covers an area of ~0.3 square degrees (~6000 square pc) distributed across seven regions that correspond to the nuclear stellar disc (NSD), the inner Galactic Bulge and the transition region between them. obs_ack = Based on data obtained from the ESO Science Archive Facility with DOI(s): https://doi.org/10.18727/archive/9 . prov_progenitor = ESO Science Archive ( https://archive.eso.org/scienceportal/home?data_collection=195.B-0283 ) bib_reference = 10.1051/0004-6361/201936263 bib_reference_url = https://doi.org/10.1051/0004-6361/201936263 obs_copyright = All data in the ESO archive retain ESO's copyright, and are distributed according to the terms of the Creative Commons Attribution 4.0 International license (CC BY 4.0). obs_copyright_url = http://archive.eso.org/cms/eso-data-access-policy.html t_min = 57836.0 t_max = 58595.0 obs_regime = Infrared em_min = 1.158165e-6 em_max = 2.372430e-6 hips_builder = Aladin/HipsGen v12.132 hips_version = 1.4 hips_release_date = 2024-04-22T12:25Z hips_frame = equatorial hips_order = 13 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_pixel_scale = 0.229 dataproduct_type = image hips_creation_date = 2024-04-11T12:38Z hips_overlay = overlayMean mergeOverwriteTile treeMedian hips_tile_format = png moc_sky_fraction = 7.994E-6 dataproduct_subtype = color hips_service_url = https://alasky.cds.unistra.fr/GALACTICNUCLEUS/CDS_P_GALACTICNUCLEUS_DR1_color hips_service_url_1 = https://alaskybis.cds.unistra.fr/GALACTICNUCLEUS/CDS_P_GALACTICNUCLEUS_DR1_color hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 13 obs_initial_ra = 266.415009 obs_initial_dec = -29.0061110 obs_initial_fov = 0.007157263357952928 TIMESTAMP = 1721288498722 ID = CDS/P/GALEXGR6/AIS/FUV hips_doi = 10.26093/cds/aladin/366y-ayp creator_did = ivo://CDS/P/GALEXGR6/AIS/FUV obs_collection = GALEX Allsky Imaging Survey (AIS) FUV obs_title = GALEX GR6 AIS (until March 2014)- Far UV obs_description = From its launch into low-Earth orbit on April 28, 2003 the GALEX NUV camera operated almost continuously. The Project suspended operations of the FUV camera following an electrical overcurrent in May 2009. GALEX data products include a series of all sky surveys and deep sky surveys in the imaging mode, and partial surveys in the near and far UV spectroscopic modes. The principal imaging studies are the Nearby Galaxy Survey (NGS), Deep (DIS), Medium (MIS), and All Sky Imaging Surveys (AIS). The GALEX GR6 direct imaging data release are to be delivered to MAST between April and June 2010. The grism data release will occur shortly thereafter. The most notable changes between GR6 and GR4/5 include changes to the bandmerged source catalog (-mcat.fits). The Project has removed 26 columns which are either redundant or of questionable quality. These include the "BEST" and "ISOCOR" fluxes and magnitudes. The Project has also added 53 columns, mostly FUV measurements using the NUV source position. Significant updates and improvements have been made to the calibrations used for the GR6 data reductions. obs_copyright_url = http://galex.stsci.edu/GR6/ prov_progenitor = STScI (NASA) client_category = Deprecated/HiPS/CDS/UV/GALEX client_sort_key = 02-01-03 hips_creation_date = 2014-04-18T18:04Z hips_release_date = 2019-05-05T06:11Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Fernique P. (CDS) hips_version = 1.4 hips_order = 8 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png fits dataproduct_type = image hips_pixel_cut = 0 0.003 moc_access_url = http://alasky.u-strasbg.fr/GALEX/GR6-03-2014/AIS-FD/Moc.fits hips_progenitor_url = https://alasky.cds.unistra.fr/GALEX/GR6-03-2014/AIS-FD/HpxFinder hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = We acknowledge the contribution of the JHU Sloan Digital Sky Survey group to the development of this site. Many of its features were inspired by the look and feel of the SkyServer. A special thanks goes to Tamas Budavari for his help with the SDSS-GALEX matching and to Wil O'Mullane for his help with the CASJobs site setup and configuration. We also acknowledge Randy Thompson (MAST) for providing IDL IUEDAC routines and Mark Siebert for providing IDL routines to generate tile JPEG images. bib_reference = 2014AdSpR..53..900B bib_reference_url = http://cdsads.u-strasbg.fr/abs/2014AdSpR..53..900B obs_copyright = Material credited to STScI on this site was created, authored, and/or prepared for NASA under Contract NAS5-26555. Unless otherwise specifically stated, no claim to copyright is being asserted by STScI and it may be freely used as in the public domain in accordance with NASA's contract. t_min = 55287 t_max = 55348 obs_regime = UV em_min = 1.344e-7 em_max = 1.786e-7 hips_pixel_scale = 4.473E-4 hips_initial_fov = 45.0 hips_initial_ra = 210.43262500 hips_initial_dec = 11.01900000 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 0.6821 hips_estsize = 862829722 hipsgen_date = 2019-05-05T06:11Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/GALEX/GR6-03-2014/AIS-FD UPDATE hips_service_url = https://alasky.cds.unistra.fr/GALEX/GR6-03-2014/AIS-FD hips_service_url_1 = https://alaskybis.cds.unistra.fr/GALEX/GR6-03-2014/AIS-FD hips_status_1 = public mirror clonableOnce hips_service_url_2 = https://irsa.ipac.caltech.edu/data/hips/CDS/GALEX/GR6-03-2014/AIS-FD hips_status_2 = public mirror unclonable moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 8 obs_initial_ra = 210.43262500 obs_initial_dec = 11.01900000 obs_initial_fov = 0.2290324274544937 TIMESTAMP = 1721288579930 ID = CDS/P/GALEXGR6/AIS/NUV hips_doi = 10.26093/cds/aladin/317r-yke creator_did = ivo://CDS/P/GALEXGR6/AIS/NUV obs_collection = GALEX Allsky Imaging Survey (AIS) NUV obs_title = GALEX GR6 AIS (until March 2014)- NEAR UV obs_description = From its launch into low-Earth orbit on April 28, 2003 the GALEX NUV camera operated almost continuously. The Project suspended operations of the FUV camera following an electrical overcurrent in May 2009. GALEX data products include a series of all sky surveys and deep sky surveys in the imaging mode, and partial surveys in the near and far UV spectroscopic modes. The principal imaging studies are the Nearby Galaxy Survey (NGS), Deep (DIS), Medium (MIS), and All Sky Imaging Surveys (AIS). The GALEX GR6 direct imaging data release are to be delivered to MAST between April and June 2010. The grism data release will occur shortly thereafter. The most notable changes between GR6 and GR4/5 include changes to the bandmerged source catalog (-mcat.fits). The Project has removed 26 columns which are either redundant or of questionable quality. These include the "BEST" and "ISOCOR" fluxes and magnitudes. The Project has also added 53 columns, mostly FUV measurements using the NUV source position. Significant updates and improvements have been made to the calibrations used for the GR6 data reductions. obs_copyright_url = http://galex.stsci.edu/GR6/ prov_progenitor = STScI (NASA) client_category = Deprecated/HiPS/CDS/UV/GALEX client_sort_key = 02-01-02 hips_creation_date = 2014-05-02T21:02Z hips_release_date = 2019-05-05T06:21Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Fernique P. (CDS) hips_version = 1.4 hips_order = 8 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png fits dataproduct_type = image hips_pixel_cut = -0.001 0.05 moc_access_url = http://alasky.u-strasbg.fr/GALEX/GR6-03-2014/AIS-ND/Moc.fits hips_progenitor_url = https://alasky.cds.unistra.fr/GALEX/GR6-03-2014/AIS-ND/HpxFinder hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = We acknowledge the contribution of the JHU Sloan Digital Sky Survey group to the development of this site. Many of its features were inspired by the look and feel of the SkyServer. A special thanks goes to Tamas Budavari for his help with the SDSS-GALEX matching and to Wil O'Mullane for his help with the CASJobs site setup and configuration. We also acknowledge Randy Thompson (MAST) for providing IDL IUEDAC routines and Mark Siebert for providing IDL routines to generate tile JPEG images. bib_reference = 2014AdSpR..53..900B bib_reference_url = http://cdsads.u-strasbg.fr/abs/2014AdSpR..53..900B obs_copyright = Material credited to STScI on this site was created, authored, and/or prepared for NASA under Contract NAS5-26555. Unless otherwise specifically stated, no claim to copyright is being asserted by STScI and it may be freely used as in the public domain in accordance with NASA's contract. t_min = 55287 t_max = 55348 obs_regime = UV em_min = 1.771e-7 em_max = 2.831e-7 hips_pixel_scale = 4.473E-4 hips_initial_fov = 45.0 hips_initial_ra = 210.43262500 hips_initial_dec = 11.01900000 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 0.7961 hips_estsize = 1008605641 hipsgen_date = 2019-05-05T06:21Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/GALEX/GR6-03-2014/AIS-ND UPDATE hips_service_url = https://alasky.cds.unistra.fr/GALEX/GR6-03-2014/AIS-ND hips_service_url_1 = https://alaskybis.cds.unistra.fr/GALEX/GR6-03-2014/AIS-ND hips_status_1 = public mirror clonableOnce hips_service_url_2 = https://irsa.ipac.caltech.edu/data/hips/CDS/GALEX/GR6-03-2014/AIS-ND hips_status_2 = public mirror unclonable moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 8 obs_initial_ra = 210.43262500 obs_initial_dec = 11.01900000 obs_initial_fov = 0.2290324274544937 TIMESTAMP = 1721288581222 ID = CDS/P/GALEXGR6/AIS/color hips_doi = 10.26093/cds/aladin/3cj5-yp6 creator_did = ivo://CDS/P/GALEXGR6/AIS/color obs_collection = GALEX Allsky Imaging Survey (AIS) colored obs_title = GALEX GR6 AIS (until March 2014)- Color composition obs_description = From its launch into low-Earth orbit on April 28, 2003 the GALEX NUV camera operated almost continuously. The Project suspended operations of the FUV camera following an electrical overcurrent in May 2009. GALEX data products include a series of all sky surveys and deep sky surveys in the imaging mode, and partial surveys in the near and far UV spectroscopic modes. The principal imaging studies are the Nearby Galaxy Survey (NGS), Deep (DIS), Medium (MIS), and All Sky Imaging Surveys (AIS). The GALEX GR6 direct imaging data release are to be delivered to MAST between April and June 2010. The grism data release will occur shortly thereafter. The most notable changes between GR6 and GR4/5 include changes to the bandmerged source catalog (-mcat.fits). The Project has removed 26 columns which are either redundant or of questionable quality. These include the "BEST" and "ISOCOR" fluxes and magnitudes. The Project has also added 53 columns, mostly FUV measurements using the NUV source position. Significant updates and improvements have been made to the calibrations used for the GR6 data reductions. obs_copyright_url = http://galex.stsci.edu/GR6/ prov_progenitor = STScI (NASA) client_category = Deprecated/HiPS/CDS/UV/GALEX client_sort_key = 02-01-01 hips_creation_date = 2014-06-13T14:41Z hips_release_date = 2019-05-05T06:28Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Fernique P. (CDS) hips_version = 1.4 hips_order = 8 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png jpeg dataproduct_type = image hips_rgb_red = AIS-NDHiPS [9.908E-4 0.149936878125 0.2943 Sqrt] hips_rgb_blue = AIS-FDHiPS [0.0 0.02466879665851593 0.04933759331703186 Sqrt] client_application = AladinLite client_application = AladinDesktop moc_access_url = http://alasky.u-strasbg.fr/GALEX/GR6-03-2014/AIS-Color/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = We acknowledge the contribution of the JHU Sloan Digital Sky Survey group to the development of this site. Many of its features were inspired by the look and feel of the SkyServer. A special thanks goes to Tamas Budavari for his help with the SDSS-GALEX matching and to Wil O'Mullane for his help with the CASJobs site setup and configuration. We also acknowledge Randy Thompson (MAST) for providing IDL IUEDAC routines and Mark Siebert for providing IDL routines to generate tile JPEG images. bib_reference = 2014AdSpR..53..900B bib_reference_url = http://cdsads.u-strasbg.fr/abs/2014AdSpR..53..900B obs_copyright = Material credited to STScI on this site was created, authored, and/or prepared for NASA under Contract NAS5-26555. Unless otherwise specifically stated, no claim to copyright is being asserted by STScI and it may be freely used as in the public domain in accordance with NASA's contract. t_min = 55287 t_max = 55348 obs_regime = UV em_min = 1.344e-7 em_max = 2.831e-7 hips_pixel_scale = 4.473E-4 hips_initial_fov = 45.0 hips_initial_ra = 210.43262500 hips_initial_dec = 11.01900000 hips_order_min = 0 dataproduct_subtype = color moc_sky_fraction = 0.7979 hips_estsize = 23487751 hipsgen_date = 2019-05-05T06:28Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/GALEX/GR6-03-2014/AIS-Color UPDATE hips_service_url = https://alasky.cds.unistra.fr/GALEX/GR6-03-2014/AIS-Color hips_service_url_1 = https://alaskybis.cds.unistra.fr/GALEX/GR6-03-2014/AIS-Color hips_status_1 = public mirror clonableOnce hips_service_url_2 = https://irsa.ipac.caltech.edu/data/hips/CDS/GALEX/GR6-03-2014/AIS-Color hips_status_2 = public mirror unclonable hips_service_url_3 = https://healpix.ias.u-psud.fr/CDS_P_GALEXGR6_AIS_color hips_status_3 = public mirror unclonable moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 8 obs_initial_ra = 210.43262500 obs_initial_dec = 11.01900000 obs_initial_fov = 0.2290324274544937 TIMESTAMP = 1729584783740 ID = CDS/P/GALEXGR6_7/FUV hips_doi = 10.26093/cds/aladin/27bp-2en hips_initial_fov = 45.0 hips_initial_ra = 210.43262500 hips_initial_dec = 11.01900000 creator_did = ivo://CDS/P/GALEXGR6_7/FUV hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra obs_title = GALEXGR6_7 FUV obs_collection = GALEX FUV obs_description = The Galaxy Evolution Explorer (GALEX) satellite is a NASA mission led by the California Institute of Technology to investigate how star formation in galaxies evolved from the early Universe up to the present. GALEX uses microchannel plate detectors to obtain direct images in the near-UV (NUV) and far-UV (FUV) and a grism to disperse light for low resolution spectroscopy. From its launch into low-Earth orbit on April 28, 2003 the GALEX NUV camera operated almost continuously. The Project suspended operations of the FUV camera following an electrical overcurrent in May 2009. GALEX data products include a series of all sky surveys and deep sky surveys in the imaging mode, and partial surveys in the near and far UV spectroscopic modes. The principal imaging studies are the Nearby Galaxy Survey (NGS), Deep (DIS), Medium (MIS), and All Sky Imaging Surveys (AIS). During the course of the mission, the GALEX team have released data to the public through MAST at discrete times. The last complete release was the GR6 (late 2010 through mid 2011 for imaging supplements and the grism survey). A final release of GALEX data arrived in late 2012 at MAST. These included a number of redelivered GR6 data (additional visits and associated coadds from 2003 onwards), along with new tiles within GR7, which span approximately from Jan. 2010 through Feb. 2012 obs_ack = We acknowledge the contribution of the JHU Sloan Digital Sky Survey group to the development of this site. Many of its features were inspired by the look and feel of the SkyServer. A special thanks goes to Tamas Budavari for his help with the SDSS-GALEX matching and to Wil O'Mullane for his help with the CASJobs site setup and configuration. We also acknowledge Randy Thompson (MAST) for providing IDL IUEDAC routines and Mark Siebert for providing IDL routines to generate tile JPEG images. prov_progenitor = STScI (NASA) bib_reference = 2017ApJS..230...24B bib_reference_url = https://iopscience.iop.org/article/10.3847/1538-4365/aa7053 client_category = Image/UV/GALEX obs_copyright = STScI (NASA) obs_copyright_url = https://www.stsci.edu/copyright t_min = 52757.4858796 t_max = 56471.4858796 obs_regime = UV em_min = 1.344e-7 em_max = 1.786e-7 hips_builder = Aladin/HipsGen v11.101 hips_version = 1.4 hips_release_date = 2022-03-15T23:01Z hips_frame = equatorial hips_bunit = (1/2.04142)MJy/sr hips_order = 9 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_bitpix = -32 hips_pixel_scale = 2.236E-4 dataproduct_type = image moc_sky_fraction = 0.6721 hips_estsize = 3112454074 hipsgen_date = 2022-02-12T00:05Z hipsgen_params = out=CDS_P_GALEXGR6_7_FUV_int creator_did=CDS/P/GALEXGR6_7/FUV hips_frame=equatorial TREE hips_creation_date = 2022-02-12T00:05Z hips_pixel_cut = 0 0.007 hipsgen_date_1 = 2022-03-15T03:37Z hipsgen_params_1 = out=CDS_P_GALEXGR6_7_FUV_int creator_did=CDS/P/GALEXGR6_7/FUV "hips_pixel_cut=0 0.007 sqrt" PNG hipsgen_date_2 = 2022-03-15T12:16Z hipsgen_params_2 = out=CDS_P_GALEXGR6_7_FUV_int creator_did=CDS/P/GALEXGR6_7/FUV -f "hips_pixel_cut=0 0.007 sqrt" method=MEAN PNG hips_service_url = https://alasky.cds.unistra.fr/GALEX/GALEXGR6_7_FUV hips_service_url_1 = https://alaskybis.cds.unistra.fr/GALEX/GALEXGR6_7_FUV hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 9 obs_initial_ra = 210.43262500 obs_initial_dec = 11.01900000 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1725343189732 ID = CDS/P/GALEXGR6_7/NUV hips_doi = 10.26093/cds/aladin/20ag-p3d hips_initial_fov = 45.0 hips_initial_ra = 210.43262500 hips_initial_dec = 11.01900000 creator_did = ivo://CDS/P/GALEXGR6_7/NUV hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra obs_title = GALEXGR6_7 NUV obs_collection = GALEX NUV obs_description = The Galaxy Evolution Explorer (GALEX) satellite is a NASA mission led by the California Institute of Technology to investigate how star formation in galaxies evolved from the early Universe up to the present. GALEX uses microchannel plate detectors to obtain direct images in the near-UV (NUV) and far-UV (FUV) and a grism to disperse light for low resolution spectroscopy. From its launch into low-Earth orbit on April 28, 2003 the GALEX NUV camera operated almost continuously. The Project suspended operations of the FUV camera following an electrical overcurrent in May 2009. GALEX data products include a series of all sky surveys and deep sky surveys in the imaging mode, and partial surveys in the near and far UV spectroscopic modes. The principal imaging studies are the Nearby Galaxy Survey (NGS), Deep (DIS), Medium (MIS), and All Sky Imaging Surveys (AIS). During the course of the mission, the GALEX team have released data to the public through MAST at discrete times. The last complete release was the GR6 (late 2010 through mid 2011 for imaging supplements and the grism survey). A final release of GALEX data arrived in late 2012 at MAST. These included a number of redelivered GR6 data (additional visits and associated coadds from 2003 onwards), along with new tiles within GR7, which span approximately from Jan. 2010 through Feb. 2012 obs_ack = We acknowledge the contribution of the JHU Sloan Digital Sky Survey group to the development of this site. Many of its features were inspired by the look and feel of the SkyServer. A special thanks goes to Tamas Budavari for his help with the SDSS-GALEX matching and to Wil O'Mullane for his help with the CASJobs site setup and configuration. We also acknowledge Randy Thompson (MAST) for providing IDL IUEDAC routines and Mark Siebert for providing IDL routines to generate tile JPEG images. prov_progenitor = STScI (NASA) bib_reference = 2017ApJS..230...24B bib_reference_url = https://iopscience.iop.org/article/10.3847/1538-4365/aa7053 client_category = Image/UV/GALEX obs_copyright = STScI (NASA) obs_copyright_url = https://www.stsci.edu/copyright t_min = 52757.4858796 t_max = 56471.4858796 obs_regime = UV em_min = 1.771e-7 em_max = 2.831e-7 hips_builder = Aladin/HipsGen v11.101 hips_version = 1.4 hips_release_date = 2022-03-17T03:25Z hips_frame = equatorial hips_bunit = (1/0.723778)MJy/sr hips_order = 9 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_bitpix = -32 hips_pixel_scale = 2.236E-4 dataproduct_type = image moc_sky_fraction = 0.788 hips_estsize = 3649325330 hipsgen_date = 2022-02-12T01:43Z hipsgen_params = out=CDS_P_GALEXGR6_7_NUV_int creator_did=CDS/P/GALEXGR6_7/NUV hips_frame=equatorial TREE hips_creation_date = 2022-02-12T01:43Z hipsgen_date_1 = 2022-03-16T13:27Z hipsgen_params_1 = out=CDS_P_GALEXGR6_7_NUV_int creator_did=CDS/P/GALEXGR6_7/NUV -f "hips_pixel_cut=0.001 0.1 sqrt" method=MEAN PNG hips_pixel_cut = 0.001 0.1 hips_service_url = https://alasky.cds.unistra.fr/GALEX/GALEXGR6_7_NUV hips_service_url_1 = https://alaskybis.cds.unistra.fr/GALEX/GALEXGR6_7_NUV hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 9 obs_initial_ra = 210.43262500 obs_initial_dec = 11.01900000 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1725343189828 ID = CDS/P/GALEXGR6_7/color hips_doi = 10.26093/cds/aladin/kpza-hn hips_initial_fov = 45.0 hips_initial_ra = 210.43262500 hips_initial_dec = 11.01900000 creator_did = ivo://CDS/P/GALEXGR6_7/color hips_creator = Buga M. (CDS) , Boch T. (CDS) hips_copyright = CNRS/Unistra obs_title = GALEX GR6/7 - Color composition obs_collection = GALEX obs_description = The Galaxy Evolution Explorer (GALEX) satellite is a NASA mission led by the California Institute of Technology to investigate how star formation in galaxies evolved from the early Universe up to the present. GALEX uses microchannel plate detectors to obtain direct images in the near-UV (NUV) and far-UV (FUV) and a grism to disperse light for low resolution spectroscopy. From its launch into low-Earth orbit on April 28, 2003 the GALEX NUV camera operated almost continuously. The Project suspended operations of the FUV camera following an electrical overcurrent in May 2009. GALEX data products include a series of all sky surveys and deep sky surveys in the imaging mode, and partial surveys in the near and far UV spectroscopic modes. The principal imaging studies are the Nearby Galaxy Survey (NGS), Deep (DIS), Medium (MIS), and All Sky Imaging Surveys (AIS). During the course of the mission, the GALEX team have released data to the public through MAST at discrete times. The last complete release was the GR6 (late 2010 through mid 2011 for imaging supplements and the grism survey). A final release of GALEX data arrived in late 2012 at MAST. These included a number of redelivered GR6 data (additional visits and associated coadds from 2003 onwards), along with new tiles within GR7, which span approximately from Jan. 2010 through Feb. 2012 obs_ack = We acknowledge the contribution of the JHU Sloan Digital Sky Survey group to the development of this site. Many of its features were inspired by the look and feel of the SkyServer. A special thanks goes to Tamas Budavari for his help with the SDSS-GALEX matching and to Wil O'Mullane for his help with the CASJobs site setup and configuration. We also acknowledge Randy Thompson (MAST) for providing IDL IUEDAC routines and Mark Siebert for providing IDL routines to generate tile JPEG images. prov_progenitor = STScI (NASA) bib_reference = 2017ApJS..230...24B bib_reference_url = https://iopscience.iop.org/article/10.3847/1538-4365/aa7053 client_category = Image/UV/GALEX obs_copyright = STScI (NASA) obs_copyright_url = https://www.stsci.edu/copyright t_min = 52757.4858796 t_max = 56471.4858796 obs_regime = UV em_min = 1.344e-7 em_max = 2.831e-7 hips_version = 1.4 hips_release_date = 2022-03-30T19:35Z hips_frame = equatorial hips_order = 9 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_pixel_scale = 2.236E-4 dataproduct_type = image hips_rgb_red = GALEXGR6_7 NUV [lupton min=0 scale=8 Q=20.0] hips_rgb_blue = GALEXGR6_7 FUV [lupton min=0 scale=32 Q=20.0] moc_sky_fraction = 0.7897 hips_estsize = 89031588 hipsgen_date = 2022-03-19T15:24Z hipsgen_params = inRed=/data-local-zfs/buga/Galex_DR6-7/all/NV/CDS_P_GALEXGR6_7_NUV_int inBlue=/data-local-zfs/buga/Galex_DR6-7/all/FV/CDS_P_GALEXGR6_7_FUV_int out=CDS_P_GALEXGR6_7_Color_int creator_did=CDS/P/GALEXGR6_7/Color color=png RGB hips_creation_date = 2022-03-19T15:24Z hips_hierarchy = mean hips_tile_format = png hipsgen_date_1 = 2022-03-21T19:01Z hipsgen_params_1 = inRed=/data-local-zfs/buga/Galex_DR6-7/all/NV/CDS_P_GALEXGR6_7_NUV_int inBlue=/data-local-zfs/buga/Galex_DR6-7/all/FV/CDS_P_GALEXGR6_7_FUV_int out=CDS_P_GALEXGR6_7_Color_int creator_did=CDS/P/GALEXGR6_7/Color -f "cmBlue=0 0.007 sqrt" "cmRed=0.001 0.1 sqrt" method=MEAN color=png RGB hipsgen_date_2 = 2022-03-25T21:02Z hipsgen_params_2 = inRed=/data-local-zfs/buga/Galex_DR6-7/all/NV/CDS_P_GALEXGR6_7_NUV_int inBlue=/data-local-zfs/buga/Galex_DR6-7/all/FV/CDS_P_GALEXGR6_7_FUV_int out=CDS_P_GALEXGR6_7_Color_int creator_did=CDS/P/GALEXGR6_7/Color "cmBlue=0 0.007" "cmRed=0.001 0.1" method=MEAN -f color=png RGB hipsgen_date_3 = 2022-03-29T17:42Z hipsgen_params_3 = inRed=/data-local-zfs/buga/Galex_DR6-7/all/NV/CDS_P_GALEXGR6_7_NUV_int inBlue=/data-local-zfs/buga/Galex_DR6-7/all/FV/CDS_P_GALEXGR6_7_FUV_int out=CDS_P_GALEXGR6_7_Color_int creator_did=CDS/P/GALEXGR6_7/Color -f luptonQ=20 luptonS=8/11/32 luptonM=0/0/0 method=MEAN color=png RGB dataproduct_subtype = color client_application = AladinLite client_application = AladinDesktop hips_service_url = https://alasky.cds.unistra.fr/GALEX/GALEXGR6_7_color hips_service_url_1 = https://alaskybis.cds.unistra.fr/GALEX/GALEXGR6_7_color hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 9 obs_initial_ra = 210.43262500 obs_initial_dec = 11.01900000 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288415650 ID = CDS/P/GalaxyCounts/2MPZ/0001-001 creator_did = ivo://CDS/P/GalaxyCounts/2MPZ/0001-001 client_category = Ancillary/GalaxyCounts/2MPZ obs_collection = LIGO/Virgo probability maps (0.001 < z < 0.01, 40 to 80 Mpc) obs_title = LIGO (0.001 < z < 0.01, 40 to 80 Mpc) obs_description = The initial discovery of LIGO on 14 September 2015 was the in-spiral merger and ring-down of the black hole binary at a distance of about 500 Mpc or a redshift of about 0.1. The search for electromagnetic counterparts for the in-spiral of binary black holes is impeded by poor initial source localizations and a lack of a compelling model for the counterpart; therefore, rapid electromagnetic follow-up is required to understand the astrophysical context of these sources. Because astrophysical sources of gravitational radiation are likely to reside in galaxies, it would make sense to search rst in regions where the LIGO-Virgo probability is large and where the density of galaxies is large as well. Under the Bayesian prior assumption that the probability of a gravitational-wave event from a given region of space is proportional to the density of galaxies within the probed volume, one can calculate an improved localization of the position of the source simply by multiplying the LIGO-Virgo skymap by the density of galaxies in the range of redshifts. We propose using the 2-MASS Photometric Redshift Galaxy Catalogue for this purpose and demonstrate that using it can dramatically reduce the search region for electromagnetic counterparts. obs_ack = The software and galaxy maps used in this paper is available at http://ubc-astrophysics.github.io . We used the VizieR Service, the NASA ADS service, the Super-COSMOS Science Archive, the NASA/IPAC Infrared Science Archive, the HEALPy libraries and arXiv.org. hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra prov_progenitor = UBC-Astrophysics bib_reference_url = https://ui.adsabs.harvard.edu/abs/2016MNRAS.462.1085A/abstract obs_copyright = UBC-Astrophysics obs_copyright_url = http://copyright.ubc.ca/guidelines-and-resources/faq/ t_min = 50600 t_max = 51941 obs_regime = Infrared hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T06:36Z hips_frame = equatorial hips_order = 3 hips_tile_width = 32 hips_master_url = http://alasky.unistra.fr/pub/arxiv.1602.07710v1/HIPS_0001_001/ hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_bitpix = -32 hips_pixel_cut = -3.735E-7 0.1841 hips_data_range = -0.1577 0.4732 hips_pixel_scale = 0.229 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 6566 hipsgen_date = 2016-10-21T14:47Z hipsgen_params = in=2MPZ.gz_0.001_0.01_smoothed.fits out=HIPS_0001_001 ivorn=ivo://CDS/P/LIGO/0001 "Publisher=M.Buga [CDS]" hips_creation_date = 2016-10-21T14:47Z hipsgen_date_1 = 2016-10-21T14:47Z hipsgen_params_1 = in=2MPZ.gz_0.001_0.01_smoothed.fits out=HIPS_0001_001 ivorn=ivo://CDS/P/LIGO/0001 "Publisher=M.Buga [CDS]" hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 bib_reference = 2016MNRAS.462.1085A hips_order_min = 0 hipsgen_date_2 = 2019-05-21T06:36Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/pub/arxiv.1602.07710v1/HIPS_0001_001 UPDATE hips_service_url = https://alasky.cds.unistra.fr/pub/arxiv.1602.07710v1/HIPS_0001_001 hips_service_url_1 = https://alaskybis.cds.unistra.fr/pub/arxiv.1602.07710v1/HIPS_0001_001 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 8 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.2290324274544937 TIMESTAMP = 1721288464706 ID = CDS/P/GalaxyCounts/2MPZ/001-002 creator_did = ivo://CDS/P/GalaxyCounts/2MPZ/001-002 client_category = Ancillary/GalaxyCounts/2MPZ obs_collection = LIGO/Virgo probability maps (0.01 < z < 0.02, 40 to 80 Mpc) obs_title = LIGO (0.01 < z < 0.02, 40 to 80 Mpc) obs_description = The initial discovery of LIGO on 14 September 2015 was the in-spiral merger and ring-down of the black hole binary at a distance of about 500 Mpc or a redshift of about 0.1. The search for electromagnetic counterparts for the in-spiral of binary black holes is impeded by poor initial source localizations and a lack of a compelling model for the counterpart; therefore, rapid electromagnetic follow-up is required to understand the astrophysical context of these sources. Because astrophysical sources of gravitational radiation are likely to reside in galaxies, it would make sense to search rst in regions where the LIGO-Virgo probability is large and where the density of galaxies is large as well. Under the Bayesian prior assumption that the probability of a gravitational-wave event from a given region of space is proportional to the density of galaxies within the probed volume, one can calculate an improved localization of the position of the source simply by multiplying the LIGO-Virgo skymap by the density of galaxies in the range of redshifts. We propose using the 2-MASS Photometric Redshift Galaxy Catalogue for this purpose and demonstrate that using it can dramatically reduce the search region for electromagnetic counterparts. obs_ack = The software and galaxy maps used in this paper is available at http://ubc-astrophysics.github.io . We used the VizieR Service, the NASA ADS service, the Super-COSMOS Science Archive, the NASA/IPAC Infrared Science Archive, the HEALPy libraries and arXiv.org. hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra prov_progenitor = UBC-Astrophysics bib_reference_url = https://ui.adsabs.harvard.edu/abs/2016MNRAS.462.1085A/abstract obs_copyright = UBC-Astrophysics obs_copyright_url = http://copyright.ubc.ca/guidelines-and-resources/faq/ t_min = 50600 t_max = 51941 obs_regime = Infrared hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T06:36Z hips_frame = equatorial hips_order = 3 hips_tile_width = 32 hips_master_url = http://alasky.unistra.fr/pub/arxiv.1602.07710v1/HIPS_001_002/ hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_bitpix = -32 hips_pixel_cut = -8.864E-7 0.2865 hips_data_range = -0.2589 0.7766 hips_pixel_scale = 0.229 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 6566 hipsgen_date = 2016-10-21T14:49Z hipsgen_params = in=2MPZ.gz_0.01_0.02_smoothed.fits out=HIPS_001_002 ivorn=ivo://CDS/P/LIGO/001 "Publisher=M.Buga [CDS]" hips_creation_date = 2016-10-21T14:49Z hipsgen_date_1 = 2016-10-21T14:49Z hipsgen_params_1 = in=2MPZ.gz_0.01_0.02_smoothed.fits out=HIPS_001_002 ivorn=ivo://CDS/P/LIGO/001 "Publisher=M.Buga [CDS]" hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 bib_reference = 2016MNRAS.462.1085A hips_order_min = 0 hipsgen_date_2 = 2019-05-21T06:36Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/pub/arxiv.1602.07710v1/HIPS_001_002 UPDATE hips_service_url = https://alasky.cds.unistra.fr/pub/arxiv.1602.07710v1/HIPS_001_002 hips_service_url_1 = https://alaskybis.cds.unistra.fr/pub/arxiv.1602.07710v1/HIPS_001_002 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 8 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.2290324274544937 TIMESTAMP = 1721288464782 ID = CDS/P/GalaxyCounts/2MPZ/002-003 creator_did = ivo://CDS/P/GalaxyCounts/2MPZ/002-003 client_category = Ancillary/GalaxyCounts/2MPZ obs_collection = LIGO/Virgo probability maps (0.02 < z < 0.03, 40 to 80 Mpc) obs_title = LIGO (0.02 < z < 0.03, 40 to 80 Mpc) obs_description = The initial discovery of LIGO on 14 September 2015 was the in-spiral merger and ring-down of the black hole binary at a distance of about 500 Mpc or a redshift of about 0.1. The search for electromagnetic counterparts for the in-spiral of binary black holes is impeded by poor initial source localizations and a lack of a compelling model for the counterpart; therefore, rapid electromagnetic follow-up is required to understand the astrophysical context of these sources. Because astrophysical sources of gravitational radiation are likely to reside in galaxies, it would make sense to search rst in regions where the LIGO-Virgo probability is large and where the density of galaxies is large as well. Under the Bayesian prior assumption that the probability of a gravitational-wave event from a given region of space is proportional to the density of galaxies within the probed volume, one can calculate an improved localization of the position of the source simply by multiplying the LIGO-Virgo skymap by the density of galaxies in the range of redshifts. We propose using the 2-MASS Photometric Redshift Galaxy Catalogue for this purpose and demonstrate that using it can dramatically reduce the search region for electromagnetic counterparts. obs_ack = The software and galaxy maps used in this paper is available at http://ubc-astrophysics.github.io . We used the VizieR Service, the NASA ADS service, the Super-COSMOS Science Archive, the NASA/IPAC Infrared Science Archive, the HEALPy libraries and arXiv.org. hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra prov_progenitor = UBC-Astrophysics bib_reference_url = https://ui.adsabs.harvard.edu/abs/2016MNRAS.462.1085A/abstract obs_copyright = UBC-Astrophysics obs_copyright_url = http://copyright.ubc.ca/guidelines-and-resources/faq/ t_min = 50600 t_max = 51941 obs_regime = Infrared hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T06:36Z hips_frame = equatorial hips_order = 3 hips_tile_width = 32 hips_master_url = http://alasky.unistra.fr/pub/arxiv.1602.07710v1/HIPS_002_003/ hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_bitpix = -32 hips_pixel_cut = -8.387E-7 0.3839 hips_data_range = -0.371 1.113 hips_pixel_scale = 0.229 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 6566 hipsgen_date = 2016-10-21T14:49Z hipsgen_params = in=2MPZ.gz_0.02_0.03_smoothed.fits out=HIPS_002_003 ivorn=ivo://CDS/P/LIGO/002 "Publisher=M.Buga [CDS]" hips_creation_date = 2016-10-21T14:49Z hipsgen_date_1 = 2016-10-21T14:49Z hipsgen_params_1 = in=2MPZ.gz_0.02_0.03_smoothed.fits out=HIPS_002_003 ivorn=ivo://CDS/P/LIGO/002 "Publisher=M.Buga [CDS]" hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 bib_reference = 2016MNRAS.462.1085A hips_order_min = 0 hipsgen_date_2 = 2019-05-21T06:36Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/pub/arxiv.1602.07710v1/HIPS_002_003 UPDATE hips_service_url = https://alasky.cds.unistra.fr/pub/arxiv.1602.07710v1/HIPS_002_003 hips_service_url_1 = https://alaskybis.cds.unistra.fr/pub/arxiv.1602.07710v1/HIPS_002_003 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 8 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.2290324274544937 TIMESTAMP = 1721288464846 ID = CDS/P/GalaxyCounts/2MPZ/003-004 creator_did = ivo://CDS/P/GalaxyCounts/2MPZ/003-004 client_category = Ancillary/GalaxyCounts/2MPZ obs_collection = LIGO/Virgo probability maps (0.03 < z < 0.04, 40 to 80 Mpc) obs_title = LIGO (0.03 < z < 0.04, 40 to 80 Mpc) obs_description = The initial discovery of LIGO on 14 September 2015 was the in-spiral merger and ring-down of the black hole binary at a distance of about 500 Mpc or a redshift of about 0.1. The search for electromagnetic counterparts for the in-spiral of binary black holes is impeded by poor initial source localizations and a lack of a compelling model for the counterpart; therefore, rapid electromagnetic follow-up is required to understand the astrophysical context of these sources. Because astrophysical sources of gravitational radiation are likely to reside in galaxies, it would make sense to search rst in regions where the LIGO-Virgo probability is large and where the density of galaxies is large as well. Under the Bayesian prior assumption that the probability of a gravitational-wave event from a given region of space is proportional to the density of galaxies within the probed volume, one can calculate an improved localization of the position of the source simply by multiplying the LIGO-Virgo skymap by the density of galaxies in the range of redshifts. We propose using the 2-MASS Photometric Redshift Galaxy Catalogue for this purpose and demonstrate that using it can dramatically reduce the search region for electromagnetic counterparts. obs_ack = The software and galaxy maps used in this paper is available at http://ubc-astrophysics.github.io . We used the VizieR Service, the NASA ADS service, the Super-COSMOS Science Archive, the NASA/IPAC Infrared Science Archive, the HEALPy libraries and arXiv.org. hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra prov_progenitor = UBC-Astrophysics bib_reference_url = https://ui.adsabs.harvard.edu/abs/2016MNRAS.462.1085A/abstract obs_copyright = UBC-Astrophysics obs_copyright_url = http://copyright.ubc.ca/guidelines-and-resources/faq/ t_min = 50600 t_max = 51941 obs_regime = Infrared hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T06:37Z hips_frame = equatorial hips_order = 3 hips_tile_width = 32 hips_master_url = http://alasky.unistra.fr/pub/arxiv.1602.07710v1/HIPS_003_004/ hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_bitpix = -32 hips_pixel_cut = -1.356E-6 0.4006 hips_data_range = -0.3117 0.935 hips_pixel_scale = 0.229 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 6566 hipsgen_date = 2016-10-21T14:50Z hipsgen_params = in=2MPZ.gz_0.03_0.04_smoothed.fits out=HIPS_003_004 ivorn=ivo://CDS/P/LIGO/003 "Publisher=M.Buga [CDS]" hips_creation_date = 2016-10-21T14:50Z hipsgen_date_1 = 2016-10-21T14:50Z hipsgen_params_1 = in=2MPZ.gz_0.03_0.04_smoothed.fits out=HIPS_003_004 ivorn=ivo://CDS/P/LIGO/003 "Publisher=M.Buga [CDS]" hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 bib_reference = 2016MNRAS.462.1085A hips_order_min = 0 hipsgen_date_2 = 2019-05-21T06:37Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/pub/arxiv.1602.07710v1/HIPS_003_004 UPDATE hips_service_url = https://alasky.cds.unistra.fr/pub/arxiv.1602.07710v1/HIPS_003_004 hips_service_url_1 = https://alaskybis.cds.unistra.fr/pub/arxiv.1602.07710v1/HIPS_003_004 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 8 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.2290324274544937 TIMESTAMP = 1721288464898 ID = CDS/P/GalaxyCounts/2MPZ/004-005 creator_did = ivo://CDS/P/GalaxyCounts/2MPZ/004-005 client_category = Ancillary/GalaxyCounts/2MPZ obs_collection = LIGO/Virgo probability maps (0.04 < z < 0.05, 40 to 80 Mpc) obs_title = LIGO (0.04 < z < 0.05, 40 to 80 Mpc) obs_description = The initial discovery of LIGO on 14 September 2015 was the in-spiral merger and ring-down of the black hole binary at a distance of about 500 Mpc or a redshift of about 0.1. The search for electromagnetic counterparts for the in-spiral of binary black holes is impeded by poor initial source localizations and a lack of a compelling model for the counterpart; therefore, rapid electromagnetic follow-up is required to understand the astrophysical context of these sources. Because astrophysical sources of gravitational radiation are likely to reside in galaxies, it would make sense to search rst in regions where the LIGO-Virgo probability is large and where the density of galaxies is large as well. Under the Bayesian prior assumption that the probability of a gravitational-wave event from a given region of space is proportional to the density of galaxies within the probed volume, one can calculate an improved localization of the position of the source simply by multiplying the LIGO-Virgo skymap by the density of galaxies in the range of redshifts. We propose using the 2-MASS Photometric Redshift Galaxy Catalogue for this purpose and demonstrate that using it can dramatically reduce the search region for electromagnetic counterparts. obs_ack = The software and galaxy maps used in this paper is available at http://ubc-astrophysics.github.io . We used the VizieR Service, the NASA ADS service, the Super-COSMOS Science Archive, the NASA/IPAC Infrared Science Archive, the HEALPy libraries and arXiv.org. hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra prov_progenitor = UBC-Astrophysics bib_reference_url = https://ui.adsabs.harvard.edu/abs/2016MNRAS.462.1085A/abstract obs_copyright = UBC-Astrophysics obs_copyright_url = http://copyright.ubc.ca/guidelines-and-resources/faq/ t_min = 50600 t_max = 51941 obs_regime = Infrared hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T06:37Z hips_frame = equatorial hips_order = 3 hips_tile_width = 32 hips_master_url = http://alasky.unistra.fr/pub/arxiv.1602.07710v1/HIPS_004_005/ hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_bitpix = -32 hips_pixel_cut = -7.349E-7 0.4508 hips_data_range = -0.3217 0.965 hips_pixel_scale = 0.229 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 6566 hipsgen_date = 2016-10-21T14:50Z hipsgen_params = in=2MPZ.gz_0.04_0.05_smoothed.fits out=HIPS_004_005 ivorn=ivo://CDS/P/LIGO/004 "Publisher=M.Buga [CDS]" hips_creation_date = 2016-10-21T14:50Z hipsgen_date_1 = 2016-10-21T14:50Z hipsgen_params_1 = in=2MPZ.gz_0.04_0.05_smoothed.fits out=HIPS_004_005 ivorn=ivo://CDS/P/LIGO/004 "Publisher=M.Buga [CDS]" hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 bib_reference = 2016MNRAS.462.1085A hips_order_min = 0 hipsgen_date_2 = 2019-05-21T06:37Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/pub/arxiv.1602.07710v1/HIPS_004_005 UPDATE hips_service_url = https://alasky.cds.unistra.fr/pub/arxiv.1602.07710v1/HIPS_004_005 hips_service_url_1 = https://alaskybis.cds.unistra.fr/pub/arxiv.1602.07710v1/HIPS_004_005 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 8 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.2290324274544937 TIMESTAMP = 1721288464954 ID = CDS/P/GalaxyCounts/2MPZ/005-007 creator_did = ivo://CDS/P/GalaxyCounts/2MPZ/005-007 client_category = Ancillary/GalaxyCounts/2MPZ obs_collection = LIGO/Virgo probability maps (0.05 < z < 0.07, 40 to 80 Mpc) obs_title = LIGO (0.05 < z < 0.07, 40 to 80 Mpc) obs_description = The initial discovery of LIGO on 14 September 2015 was the in-spiral merger and ring-down of the black hole binary at a distance of about 500 Mpc or a redshift of about 0.1. The search for electromagnetic counterparts for the in-spiral of binary black holes is impeded by poor initial source localizations and a lack of a compelling model for the counterpart; therefore, rapid electromagnetic follow-up is required to understand the astrophysical context of these sources. Because astrophysical sources of gravitational radiation are likely to reside in galaxies, it would make sense to search rst in regions where the LIGO-Virgo probability is large and where the density of galaxies is large as well. Under the Bayesian prior assumption that the probability of a gravitational-wave event from a given region of space is proportional to the density of galaxies within the probed volume, one can calculate an improved localization of the position of the source simply by multiplying the LIGO-Virgo skymap by the density of galaxies in the range of redshifts. We propose using the 2-MASS Photometric Redshift Galaxy Catalogue for this purpose and demonstrate that using it can dramatically reduce the search region for electromagnetic counterparts. obs_ack = The software and galaxy maps used in this paper is available at http://ubc-astrophysics.github.io . We used the VizieR Service, the NASA ADS service, the Super-COSMOS Science Archive, the NASA/IPAC Infrared Science Archive, the HEALPy libraries and arXiv.org. hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra prov_progenitor = UBC-Astrophysics bib_reference_url = https://ui.adsabs.harvard.edu/ads/2016MNRAS.462.1085A/abstract obs_copyright = UBC-Astrophysics obs_copyright_url = http://copyright.ubc.ca/guidelines-and-resources/faq/ t_min = 50600 t_max = 51941 obs_regime = Infrared hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T06:37Z hips_frame = equatorial hips_order = 3 hips_tile_width = 32 hips_master_url = http://alasky.unistra.fr/pub/arxiv.1602.07710v1/HIPS_005_007/ hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_bitpix = -32 hips_pixel_cut = -8.968E-7 0.6313 hips_data_range = -0.4141 1.242 hips_pixel_scale = 0.229 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 6566 hipsgen_date = 2016-10-21T14:51Z hipsgen_params = in=2MPZ.gz_0.05_0.07_smoothed.fits out=HIPS_005_007 ivorn=ivo://CDS/P/LIGO/005 "Publisher=M.Buga [CDS]" hips_creation_date = 2016-10-21T14:51Z hipsgen_date_1 = 2016-10-21T14:51Z hipsgen_params_1 = in=2MPZ.gz_0.05_0.07_smoothed.fits out=HIPS_005_007 ivorn=ivo://CDS/P/LIGO/005 "Publisher=M.Buga [CDS]" hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 bib_reference = 2016MNRAS.462.1085A hips_order_min = 0 hipsgen_date_2 = 2019-05-21T06:37Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/pub/arxiv.1602.07710v1/HIPS_005_007 UPDATE hips_service_url = https://alasky.cds.unistra.fr/pub/arxiv.1602.07710v1/HIPS_005_007 hips_service_url_1 = https://alaskybis.cds.unistra.fr/pub/arxiv.1602.07710v1/HIPS_005_007 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 8 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.2290324274544937 TIMESTAMP = 1721288465030 ID = CDS/P/GalaxyCounts/2MPZ/007-01 creator_did = ivo://CDS/P/GalaxyCounts/2MPZ/007-01 client_category = Ancillary/GalaxyCounts/2MPZ obs_collection = LIGO/Virgo probability maps (0.07 < z < 0.1, 40 to 80 Mpc) obs_title = LIGO (0.07 < z < 0.1, 40 to 80 Mpc) obs_description = The initial discovery of LIGO on 14 September 2015 was the in-spiral merger and ring-down of the black hole binary at a distance of about 500 Mpc or a redshift of about 0.1. The search for electromagnetic counterparts for the in-spiral of binary black holes is impeded by poor initial source localizations and a lack of a compelling model for the counterpart; therefore, rapid electromagnetic follow-up is required to understand the astrophysical context of these sources. Because astrophysical sources of gravitational radiation are likely to reside in galaxies, it would make sense to search rst in regions where the LIGO-Virgo probability is large and where the density of galaxies is large as well. Under the Bayesian prior assumption that the probability of a gravitational-wave event from a given region of space is proportional to the density of galaxies within the probed volume, one can calculate an improved localization of the position of the source simply by multiplying the LIGO-Virgo skymap by the density of galaxies in the range of redshifts. We propose using the 2-MASS Photometric Redshift Galaxy Catalogue for this purpose and demonstrate that using it can dramatically reduce the search region for electromagnetic counterparts. obs_ack = The software and galaxy maps used in this paper is available at http://ubc-astrophysics.github.io . We used the VizieR Service, the NASA ADS service, the Super-COSMOS Science Archive, the NASA/IPAC Infrared Science Archive, the HEALPy libraries and arXiv.org. hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra prov_progenitor = UBC-Astrophysics bib_reference_url = https://ui.adsabs.harvard.edu/abs/2016MNRAS.462.1085A/abstract obs_copyright = UBC-Astrophysics obs_copyright_url = http://copyright.ubc.ca/guidelines-and-resources/faq/ t_min = 50600 t_max = 51941 obs_regime = Infrared hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T06:37Z hips_frame = equatorial hips_order = 3 hips_tile_width = 32 hips_master_url = http://alasky.unistra.fr/pub/arxiv.1602.07710v1/HIPS_007_01/ hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_bitpix = -32 hips_pixel_cut = -1.468E-6 0.688 hips_data_range = -0.4203 1.261 hips_pixel_scale = 0.229 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 6566 hipsgen_date = 2016-10-21T14:51Z hipsgen_params = in=2MPZ.gz_0.07_0.1_smoothed.fits out=HIPS_007_01 ivorn=ivo://CDS/P/LIGO/007 "Publisher=M.Buga [CDS]" hips_creation_date = 2016-10-21T14:51Z hipsgen_date_1 = 2016-10-21T14:51Z hipsgen_params_1 = in=2MPZ.gz_0.07_0.1_smoothed.fits out=HIPS_007_01 ivorn=ivo://CDS/P/LIGO/007 "Publisher=M.Buga [CDS]" hips_initial_fov = 58.63230142835039 hips_initial_ra = 0 hips_initial_dec = +0 bib_reference = 2016MNRAS.462.1085A hips_order_min = 0 hipsgen_date_2 = 2019-05-21T06:37Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/pub/arxiv.1602.07710v1/HIPS_007_01 UPDATE hips_service_url = https://alasky.cds.unistra.fr/pub/arxiv.1602.07710v1/HIPS_007_01 hips_service_url_1 = https://alaskybis.cds.unistra.fr/pub/arxiv.1602.07710v1/HIPS_007_01 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 8 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 0.2290324274544937 TIMESTAMP = 1721288465098 ID = CDS/P/Ganymede/VoyagerGalileo-SSI-1km client_category = Solar system/Jupiter/Ganymede hips_initial_fov = 180 hips_initial_ra = 0 hips_initial_dec = 0 creator_did = ivo://CDS/P/Ganymede/VoyagerGalileo-SSI-1km hips_overlay = mean hips_hierarchy = median hips_creator = Fernique P. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = Ganymede VoyagerGalileo SSI 1km obs_description = This global mosaic of Ganymede utilizes the best image quality and moderate resolution coverage supplied by Galileo Solid-State Imaging (SSI) and Voyager 1 and 2. This mosaic was prepared by the USGS Astrogeology Science Center using the ISIS 2 image processing and cartographic system. The image data was selected on the basis of overall image quality, reasonable input resolution (from 20 km/pixel for gap fill to approximately 400 meters/pixel), and availability of moderate viewing and sun angles for topography. prov_progenitor = USGS Astrogeology Science Center prov_progenitor_url = https://astrogeology.usgs.gov/search/map/Ganymede/Voyager-Galileo/Ganymede_Voyager_GalileoSSI_global_mosaic_1km hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T07:03Z hips_frame = ganymede hips_body = ganymede hips_order = 3 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg hips_pixel_scale = 0.01431 s_pixel_scale = 0.02177 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 18357 hipsgen_date = 2018-01-16T15:12Z hipsgen_params = -maxthread=10 in=Ganymede creator_did=CDS/P/Ganymede/VoyagerGalileo-SSI-1km color=true INDEX TILES hips_creation_date = 2018-01-16T15:12Z hips_order_min = 0 dataproduct_subtype = color hipsgen_date_1 = 2019-05-21T07:03Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume6/Planets/CDS_P_Ganymede_VoyagerGalileo-SSI-1km UPDATE hips_service_url = https://alasky.cds.unistra.fr/Planets/CDS_P_Ganymede_VoyagerGalileo-SSI-1km hips_service_url_1 = https://alaskybis.cds.unistra.fr/Planets/CDS_P_Ganymede_VoyagerGalileo-SSI-1km hips_status_1 = public mirror clonableOnce client_application = AladinDesktopBeta>=10.040 AladinDesktop>=11.125 moc_type = smoc moc_order = 3 obs_initial_ra = 0 obs_initial_dec = 0 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288466994 ID = CDS/P/HGPS/Flux hips_initial_fov = 100 hips_initial_ra = 266.40498829 hips_initial_dec = -28.93617776 creator_did = ivo://CDS/P/HGPS/Flux hips_overlay = mean hips_hierarchy = median obs_title = HGPS integral flux > 1 TeV hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T08:58Z hips_frame = equatorial hips_order = 3 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png hips_pixel_scale = 0.01431 s_pixel_scale = 0.02 dataproduct_type = image moc_sky_fraction = 0.03253 hips_estsize = 27532 hipsgen_date = 2018-07-07T13:47Z hipsgen_params = in=hips/flux_inputs out=hips/flux hips_frame=equatorial order=3 mocOrder=9 region=hips/significance_inputs/Moc.fits label=HGPS_Flux creator_did=CDS/P/HGPS/Flux color=png client_category = Image/Gamma-ray/HESS obs_regime = Gamma-ray obs_collection = HGPS obs_description = H.E.S.S. is an array of ground-based gamma-ray telescopes located in Namibia. The H.E.S.S. Galactic Plane Survey (HGPS) is the first deep and wide survey of the Milky Way in TeV gamma-rays. The flux values are given as integral photon flux above 1 TeV assuming a power law spectrum for the differential flux with an index of -2.3. The pixel values represent integrated values within a circular region of 0.1 deg. t_min = 53005 t_max = 56293 em_min = 1.242e-20 em_max = 6.199e-18 bib_reference = 2018A&A...612A...1H bib_reference_url = https://ui.adsabs.harvard.edu/#abs/2018A%26A...612A...1H hips_creator = Deil C. (MPI fur Kernphysik) , Donath A. (CFA Harward) , Fernique P. (CDS) hips_creation_date = 2018-07-07T13:47Z hips_order_min = 0 dataproduct_subtype = color hipsgen_date_1 = 2019-05-21T08:58Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume6/pub/10.1051_0004-6361_201732098flux UPDATE hips_service_url = https://alasky.cds.unistra.fr/pub/10.1051_0004-6361_201732098flux hips_service_url_1 = https://alaskybis.cds.unistra.fr/pub/10.1051_0004-6361_201732098flux hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 9 obs_initial_ra = 266.40498829 obs_initial_dec = -28.93617776 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288479186 ID = CDS/P/HGPS/Significance hips_initial_fov = 100 hips_initial_ra = 266.40498829 hips_initial_dec = -28.93617776 creator_did = ivo://CDS/P/HGPS/Significance hips_overlay = mean hips_hierarchy = median obs_title = HGPS significance (Gaussian sigma) hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T08:58Z hips_frame = equatorial hips_order = 3 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png hips_pixel_scale = 0.01431 dataproduct_type = image moc_sky_fraction = 0.03253 hips_estsize = 27532 hipsgen_date = 2018-07-07T13:47Z hipsgen_params = in=hips/significance_inputs out=hips/significance hips_frame=equatorial order=3 mocOrder=9 region=hips/significance_inputs/Moc.fits label=HGPS_Significance creator_did=CDS/P/HGPS/Significance color=png obs_regime = Gamma-ray client_category = Image/Gamma-ray/HESS obs_collection = HGPS obs_description = H.E.S.S. is an array of ground-based gamma-ray telescopes located in Namibia. The H.E.S.S. Galactic Plane Survey (HGPS) is the first deep and wide survey of the Milky Way in TeV gamma-rays. The flux values are given as integral photon flux above 1 TeV assuming a power law spectrum for the differential flux with an index of -2.3. The pixel values represent integrated values within a circular region of 0.1 deg. t_min = 53005 t_max = 56293 em_min = 1.242e-20 em_max = 6.199e-18 bib_reference = 2018A&A...612A...1H bib_reference_url = https://ui.adsabs.harvard.edu/#abs/2018A%26A...612A...1H hips_creator = Deil C. (MPI fur Kernphysik) , Donath A. (CFA Harward) , Fernique P. (CDS) hips_creation_date = 2018-07-07T13:47Z hips_order_min = 0 dataproduct_subtype = color hipsgen_date_1 = 2019-05-21T08:58Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume6/pub/10.1051_0004-6361_201732098significance UPDATE hips_service_url = https://alasky.cds.unistra.fr/pub/10.1051_0004-6361_201732098significance hips_service_url_1 = https://alaskybis.cds.unistra.fr/pub/10.1051_0004-6361_201732098significance hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 9 obs_initial_ra = 266.40498829 obs_initial_dec = -28.93617776 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288479118 ID = CDS/P/HI creator_did = ivo://CDS/P/HI obs_collection = HI obs_title = HI composite survey obs_description = Composite all-sky map of neutral hydrogen column density (N_HI), formed from the Leiden/Dwingeloo HI survey data (Hartmann & Burton 1997) and the composite N_HI map of Dickey and Lockman (1990). The two datasets are not matched in sensitivity or resolution: note that discontinuities exist in the constructed composite map. A pixel mask is provided to indicate which dataset was used for each location on the sky. Hartmann & Burton provide a velocity integrated (-450 km/s < V_lsr < +400 km/s) HI brightness temperature map in Galactic coordinates, sampled every 0.5 degrees. This entire data set was converted to N_HI by multiplying by their factor of 1.8224e18 K km s-1 cm-2 and then interpolated to pixel centers appropriate for HEALPix Nside=512. Since the Leiden/Dwingeloo survey does not have sky coverage for declinations < -30 deg., the lower resolution Dickey & Lockman map was also interpolated to HEALPix and used to fill in the coverage gap. The Dickey & Lockman N_HI map is itself a composite of several surveys which had been merged and averaged onto 1 deg. bins in Galactic coordinates. Their map includes emission between -250 km/s < V_lsr < 250 km/s (excluding the LMC and SMC). The Leiden/Dwingeloo Survey data were obtained from the CDS. The Dickey & Lockman map was obtained from NCSA ADIL. This original HEALPix file is distributed and maintained by LAMBDA. obs_copyright = Composite HI map by LAMBDA obs_copyright_url = http://lambda.gsfc.nasa.gov/product/foreground/fg_HI_get.cfm client_category = Image/Gas-lines/HI client_sort_key = 06-05 hips_creation_date = 2011-02-14T12:00Z hips_release_date = 2019-05-05T06:29Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 3 hips_frame = galactic hips_tile_width = 64 hips_tile_format = jpeg fits dataproduct_type = image moc_access_url = http://alasky.u-strasbg.fr/HI/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = We acknowledge the use of the Legacy Archive for Microwave Background Data Analysis (LAMBDA), part of the High Energy Astrophysics Science Archive Center (HEASARC). HEASARC/LAMBDA is a service of the Astrophysics Science Division at the NASA Goddard Space Flight Center. prov_progenitor = HEASARC/LAMBDA bib_reference = 1990ARA&A..28..215D bib_reference_url = http://adsabs.harvard.edu/abs/1990ARA%26A..28..215D t_min = 44239 t_max = 47892 obs_regime = Radio em_min = 0.21 em_max = 0.21 hips_pixel_scale = 0.01431 hips_initial_fov = 120.0 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1 hips_estsize = 1112337 hipsgen_date = 2019-05-05T06:29Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/HI UPDATE hips_service_url = https://alasky.cds.unistra.fr/HI hips_service_url_1 = https://alaskybis.cds.unistra.fr/HI hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288415898 ID = CDS/P/HI4PI/NHI creator_did = ivo://CDS/P/HI4PI/NHI client_category = Image/Gas-lines/HI obs_collection = HI4PI NHI obs_title = HI4PI NHI survey (full-sky HI column density distribution) obs_description = The HI4PI data release comprises 21-cm neutral atomic hydrogen data of the Milky Way (-600km/s0deg; -470km/s 2) that are rare or in short-lived phases of galaxy evolution at rest-frame optical wavelengths. The region covered by the survey spans RA 09:58:00 to 10:02:57 and dec +01:36:00 to +02:51:00 (ICRS). prov_progenitor = STScI MAST portal bib_reference = doi:10.17909/srcz-2b67 bib_reference_url = https://doi.org/10.17909/srcz-2b67 obs_copyright = These HLSP data products are licensed for use under CC BY 4.0 t_min = 57198.50826041 t_max = 59552.67468857 obs_regime = Infrared client_category = Image/Infrared/HST em_min = 1.3939e-06 em_max = 1.8094e-06 hips_builder = Aladin/HipsGen v11.071 hips_version = 1.4 hips_release_date = 2022-07-05T06:58Z hips_frame = equatorial hips_order = 13 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = -0.04 6 hips_data_range = -13.94 30.82 hips_pixel_scale = 1.397E-5 s_pixel_scale = 2.777E-5 dataproduct_type = image moc_sky_fraction = 4.778E-5 hips_estsize = 56654725 hipsgen_date = 2022-07-04T12:04Z hipsgen_params = in=tiles/drz-sci out=hips/ creator_did=CDS/P/3D-DASH TILES hips_creation_date = 2022-07-04T12:04Z hipsgen_date_1 = 2022-07-04T14:45Z hipsgen_params_1 = in=tiles/drz-sci out=hips/ creator_did=CDS/P/3D-DASH "hips_pixel_cut=-0.04 6 asinh" PNG hipsgen_date_2 = 2022-07-05T06:43Z hipsgen_params_2 = in=tiles/drz-sci out=hips/ creator_did=CDS/P/3D-DASH "hips_pixel_cut=-0.04 6 asinh" method=mean PNG -f hips_service_url = https://alasky.cds.unistra.fr/HST-programs/CDS_P_HST-programs_3D-DASH hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-programs/CDS_P_HST-programs_3D-DASH hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 13 obs_initial_ra = 150.0560833 obs_initial_dec = 2.2257333 obs_initial_fov = 0.007157263357952928 TIMESTAMP = 1721288492274 ID = CDS/P/HST/B creator_did = ivo://CDS/P/HST/B data_pixel_bitpix = -32 dataproduct_type = image em_min = 3.70e-07 em_max = 4.959e-07 client_category = Image/Optical/HST hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:3256400453 fits:2912631035 hips_copyright = CNRS/Unistra hips_creation_date = 2018-11-25T18:05Z hips_creator = Durand D. (CDS) hips_data_range = -0.7797 1.719 hips_estsize = 351332823 hips_frame = equatorial hipsgen_date = 2023-03-24T16:16Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=B -in=/data-test-iscsi/d.durand/2023A/HST/B.extract -id=CDS/P/HST/B -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/B.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_ra = 10.6847083 hips_initial_dec = 41.2687500 hips_initial_fov = 0.3 hips_nb_tiles = 631798 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = -0.001934 0.009032 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-03-25T04:03Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555." obs_collection = HST-B obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F450W, F439W, F438W and F435W filters between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community. In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Optical obs_title = HST-B includes the following filters : F450W, F439W, F438W, F435W prov_progenitor = Canadian Astronomy Data Centre s_pixel_scale = 1.100E-5 t_min = 49352.5335346065 t_max = 59981.887984919 moc_sky_fraction = 1.852E-4 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_B_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_B_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_B_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 16 obs_initial_ra = 10.6847083 obs_initial_dec = 41.2687500 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288455182 ID = CDS/P/HST/CO creator_did = ivo://CDS/P/HST/CO data_pixel_bitpix = -32 dataproduct_type = image em_min = 2.1457e-06 em_max = 2.2911e-06 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:3968375222 fits:3892971329 hips_copyright = CNRS/Unistra hips_creation_date = 2018-11-08T13:48Z hips_creator = Durand D. (CDS) hips_data_range = -26.05 72.26 hips_estsize = 32410129 hips_frame = equatorial hipsgen_date_1 = 2023-03-16T13:04Z hipsgen_date = 2023-03-14T11:18Z hipsgen_params_1 = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=CO -in=/data-test-iscsi/d.durand/2023A/HST/CO.extract -id=CDS/P/HST/CO -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/CO.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=CO -in=/data-test-iscsi/d.durand/2023A/HST/CO.extract -id=CDS/P/HST/CO -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/CO.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_dec = 47.5 hips_initial_fov = 0.01468 hips_initial_ra = 344.0 client_category = Image/Gas-lines/CO hips_nb_tiles = 62082 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwrite treeMean hips_pixel_bitpix = -32 hips_pixel_cut = -0.361 47.25 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-03-16T13:08Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555." obs_collection = HST-CO obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F222M filter between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Infrared obs_title = HST-CO includes the following filters: F222M prov_progenitor = Canadian Astronomy Data Centre s_pixel_scale = 5.704E-5 t_min = 50542.16171296 t_max = 55126.4589002315 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_CO_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_CO_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_CO_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 5.156E-6 moc_order = 16 obs_initial_ra = 344.0 obs_initial_dec = 47.5 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288455246 ID = CDS/P/HST/EPO hips_initial_fov = 0.18949 hips_initial_ra = 83.09729 hips_initial_dec = -67.70117 creator_did = ivo://CDS/P/HST/EPO hips_overlay = mean hips_hierarchy = median client_category = Outreach/Hubble hips_creator = Boch T. (CDS) hips_copyright = CNRS/Unistra obs_title = HST Outreach obs_collection = HST obs_description = HST Outreach images. Hipsilized by CDS obs_ack = ESA/Hubble obs_ack_url = https://esahubble.org/copyright/ prov_progenitor = https://esahubble.org/images/ obs_copyright = NASA, ESA, and STScI obs_copyright_url = https://esahubble.org/copyright/ t_min = 49322 t_max = 59792 obs_regime = Infrared em_min = 2e-7 em_max = 2e-6 hips_builder = Aladin/HipsGen v11.071 hips_version = 1.4 hips_release_date = 2022-08-03T14:06Z hips_frame = equatorial hips_order = 14 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png hips_pixel_scale = 6.989E-6 s_pixel_scale = 1.111E-5 dataproduct_type = image dataproduct_subtype = color moc_sky_fraction = 8.115E-4 hips_estsize = 93707526 hipsgen_date = 2022-08-03T14:06Z hipsgen_params = in=data creator_did=CDS/P/HST/EPO maxThread=32 hips_service_url = https://alasky.cds.unistra.fr/HST-outreach/CDS_P_HST_EPO hips_progenitor_url = https://alasky.cds.unistra.fr/HST-outreach/CDS_P_HST_EPO/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-outreach/CDS_P_HST_EPO hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 14 obs_initial_ra = 83.09729 obs_initial_dec = -67.70117 obs_initial_fov = 0.003578631678976464 TIMESTAMP = 1721288492150 ID = CDS/P/HST/GOODS/b creator_did = ivo://CDS/P/HST/GOODS/b obs_collection = HST GOODS b obs_title = GOODS b obs_description = The P/HST/GOODS/b Hierarchical Progressive Survey (HiPS) has been built by Francois Bonnarel from CDS and distributed by CDS. It sets together all GOODS HST ACS version1.0 observations done in F435W band as part of the GOODS survey. GOODS is the Great Observatories Deep survey. GOODS unites extremely deep observations from NASA's Great Observatories, Spitzer, Hubble, and Chandra, ESA's Herschel and XMM-Newton, and from the most powerful ground-based facilities, to survey the distant universe to the faintest flux limits across the electromagnetic spectrum. obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555."" obs_copyright = NASA/ESA/AURA obs_copyright_url = http://www.stsci.edu/institute/Copyright client_category = Image/Optical/HST/GOODS client_sort_key = 03-05-02-01 hips_release_date = 2019-05-05T06:29Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 14 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png fits dataproduct_type = image hips_pixel_cut = -6.808E-4 0.005674 hips_data_range = -1000 1000 moc_access_url = http://alasky.unistra.fr/GOODS/GOODSb/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = STScI (NASA) bib_reference = 2004ApJ...600L..93G bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2004ApJ...600L..93G t_min = 52249 t_max = 52880 obs_regime = Optical em_min = 3.599e-7 em_max = 4.861e-7 hips_creation_date = 2014-03-24T11:56Z hips_pixel_scale = 6.989E-6 hips_pixel_bitpix = -32 moc_sky_fraction = 2.223E-6 hips_estsize = 18165915 hipsgen_date = 2017-03-27T14:34Z hipsgen_params = out=GOODSb "-pixelCut=-6.808E-4 0.005674" UPDATE hips_initial_fov = 0.05 hips_initial_ra = 53.1239372 hips_initial_dec = -27.7398687 hips_order_min = 0 hipsgen_date_1 = 2019-05-05T06:29Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/GOODS/GOODSb UPDATE hips_service_url = https://alasky.cds.unistra.fr/GOODS/GOODSb hips_service_url_1 = https://alaskybis.cds.unistra.fr/GOODS/GOODSb hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 14 obs_initial_ra = 53.1239372 obs_initial_dec = -27.7398687 obs_initial_fov = 0.003578631678976464 TIMESTAMP = 1721288415986 ID = CDS/P/HST/GOODS/color creator_did = ivo://CDS/P/HST/GOODS/color obs_collection = HST GOODS color obs_title = GOODS color obs_description = The P/HST/GOODS/color Hierarchical Progressive Survey (HiPS) has been built by Francois Bonnarel from CDS and distributed by CDS. It sets together all GOODS HST ACS version1.0 observations done in v,i and z bands as part of the GOODS survey. GOODS is the Great Observatories Deep survey. GOODS unites extremely deep observations from NASA's Great Observatories, Spitzer, Hubble, and Chandra, ESA's Herschel and XMM-Newton, and from the most powerful ground-based facilities,\nto survey the distant universe to the faintest flux limits across the electromagnetic spectrum. obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555."" obs_copyright = NASA/ESA/AURA obs_copyright_url = http://www.stsci.edu/institute/Copyright client_category = Image/Optical/HST/GOODS client_sort_key = 03-05-02-00 hips_release_date = 2019-05-05T06:30Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 14 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png dataproduct_type = image hips_rgb_red = ACS_GOODSzHiPS [-2.308E-4 0.0053846 0.011 Linear] hips_rgb_green = ACS_GOODSiHiPS [-2.308E-4 0.0053846 0.011 Linear] hips_rgb_blue = ACS_GOODSvHiPS [-2.308E-4 0.0053846 0.011 Linear] moc_access_url = http://alasky.unistra.fr/GOODS/GOODS-color/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = STScI (NASA) bib_reference = 2004ApJ...600L..93G bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2004ApJ...600L..93G t_min = 52249 t_max = 52880 obs_regime = Optical em_min = 4.632e-7 em_max = 1.0946e-6 hips_creation_date = 2014-04-03T09:31Z hips_pixel_scale = 6.989E-6 hips_estsize = 57723479662 hipsgen_date = 2017-03-27T15:14Z hipsgen_params = out=GOODS-color UPDATE hips_initial_fov = 0.05 hips_initial_ra = 53.1239372 hips_initial_dec = -27.7398687 hips_order_min = 0 dataproduct_subtype = color moc_sky_fraction = 2.650E-6 hipsgen_date_1 = 2019-05-05T06:30Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/GOODS/GOODS-color UPDATE hips_service_url = https://alasky.cds.unistra.fr/GOODS/GOODS-color hips_service_url_1 = https://alaskybis.cds.unistra.fr/GOODS/GOODS-color hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 14 obs_initial_ra = 53.1239372 obs_initial_dec = -27.7398687 obs_initial_fov = 0.003578631678976464 TIMESTAMP = 1721288416046 ID = CDS/P/HST/GOODS/i creator_did = ivo://CDS/P/HST/GOODS/i obs_collection = HST GOODS i obs_title = GOODS i obs_description = The P/HST/GOODS/i Hierarchical Progressive Survey (HiPS) has been built by Francois Bonnarel from CDS and distributed by CDS. It sets together all GOODS HST ACS version1.0 observations done in F814W band as part of the GOODS survey. GOODS is the Great Observatories Deep survey. GOODS unites extremely deep observations from NASA's Great Observatories, Spitzer, Hubble, and Chandra, ESA's Herschel and XMM-Newton, and from the most powerful ground-based facilities,\nto survey the distant universe to the faintest flux limits across the electromagnetic spectrum. obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555."" obs_copyright = NASA/ESA/AURA obs_copyright_url = http://www.stsci.edu/institute/Copyright client_category = Image/Optical/HST/GOODS client_sort_key = 03-05-02-03 hips_release_date = 2019-05-05T06:30Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 14 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png fits dataproduct_type = image hips_pixel_cut = -0.002305 0.01359 hips_data_range = -1000 1000 moc_access_url = http://alasky.unistra.fr/GOODS/GOODSi/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = STScI (NASA) bib_reference = 2004ApJ...600L..93G bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2004ApJ...600L..93G t_min = 52249 t_max = 52880 obs_regime = Optical em_min = 6.801e-7 em_max = 8.63e-7 hips_creation_date = 2014-03-26T14:40Z hips_pixel_scale = 6.989E-6 hips_pixel_bitpix = -32 moc_sky_fraction = 2.628E-6 hips_estsize = 19199936 hipsgen_date = 2017-03-27T15:03Z hipsgen_params = out=GOODSi mocorder=14 "pixelCut=-0.002305 0.01359" UPDATE hips_initial_fov = 0.05 hips_initial_ra = 53.1239372 hips_initial_dec = -27.7398687 hips_order_min = 0 hipsgen_date_1 = 2019-05-05T06:30Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/GOODS/GOODSi UPDATE hips_service_url = https://alasky.cds.unistra.fr/GOODS/GOODSi hips_service_url_1 = https://alaskybis.cds.unistra.fr/GOODS/GOODSi hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 14 obs_initial_ra = 53.1239372 obs_initial_dec = -27.7398687 obs_initial_fov = 0.003578631678976464 TIMESTAMP = 1721288416102 ID = CDS/P/HST/GOODS/v creator_did = ivo://CDS/P/HST/GOODS/v obs_collection = HST GOODS v obs_title = GOODS v obs_description = The P/HST/GOODS/v Hierarchical Progressive Survey (HiPS) has been built by Francois Bonnarel from CDS and distributed by CDS. It sets together all GOODS HST ACS version1.0 observations done in F606W band as part of the GOODS survey. GOODS is the Great Observatories Deep survey. GOODS unites extremely deep observations from NASA's Great Observatories, Spitzer, Hubble, and Chandra, ESA's Herschel and XMM-Newton, and from the most powerful ground-based facilities, to survey the distant universe to the faintest flux limits across the electromagnetic spectrum. obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555."" obs_copyright = NASA/ESA/AURA obs_copyright_url = http://www.stsci.edu/institute/Copyright client_category = Image/Optical/HST/GOODS client_sort_key = 03-05-02-02 hips_release_date = 2019-05-05T06:30Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 14 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png fits dataproduct_type = image hips_pixel_cut = -0.003281 0.01266 hips_data_range = -1000 1000 moc_access_url = http://alasky.unistra.fr/GOODS/GOODSv/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = STScI (NASA) bib_reference = 2004ApJ...600L..93G bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2004ApJ...600L..93G t_min = 52249 t_max = 52880 obs_regime = Optical em_min = 4.632e-7 em_max = 7.179e-7 hips_creation_date = 2014-03-26T10:55Z hips_pixel_scale = 6.989E-6 hips_pixel_bitpix = -32 moc_sky_fraction = 2.626E-6 hips_estsize = 19199936 hipsgen_date = 2017-03-27T15:07Z hipsgen_params = out=GOODSv mocorder=14 "pixelCut=-0.003281 0.01266" UPDATE hips_initial_fov = 0.05 hips_initial_ra = 53.1239372 hips_initial_dec = -27.7398687 hips_order_min = 0 hipsgen_date_1 = 2019-05-05T06:30Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/GOODS/GOODSv UPDATE hips_service_url = https://alasky.cds.unistra.fr/GOODS/GOODSv hips_service_url_1 = https://alaskybis.cds.unistra.fr/GOODS/GOODSv hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 14 obs_initial_ra = 53.1239372 obs_initial_dec = -27.7398687 obs_initial_fov = 0.003578631678976464 TIMESTAMP = 1721288416154 ID = CDS/P/HST/GOODS/z creator_did = ivo://CDS/P/HST/GOODS/z obs_collection = HST GOODS z obs_title = GOODS z obs_description = The P/HST/GOODS/z Hierarchical Progressive Survey (HiPS) has been built by Francois Bonnarel from CDS and distributed by CDS. It sets together all GOODS HST ACS version1.0 observations done in F850LP band as part of the GOODS survey. GOODS is the Great Observatories Deep survey. GOODS unites extremely deep observations from NASA's Great Observatories, Spitzer, Hubble, and Chandra, ESA's Herschel and XMM-Newton, and from the most powerful ground-based facilities, to survey the distant universe to the faintest flux limits across the electromagnetic spectrum. obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555."" obs_copyright = NASA/ESA/AURA obs_copyright_url = http://www.stsci.edu/institute/Copyright client_category = Image/Optical/HST/GOODS client_sort_key = 03-05-02-04 hips_release_date = 2019-05-05T06:31Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 14 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png fits dataproduct_type = image hips_pixel_cut = -7.28E-4 0.008567 hips_data_range = -1000 1000 moc_access_url = http://alasky.unistra.fr/GOODS/GOODSz/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = STScI (NASA) bib_reference = 2004ApJ...600L..93G bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2004ApJ...600L..93G t_min = 52249 t_max = 52880 obs_regime = Optical em_min = 8.015e-7 em_max = 1.0946e-6 hips_creation_date = 2014-03-26T15:31Z hips_pixel_scale = 6.989E-6 hips_pixel_bitpix = -32 moc_sky_fraction = 2.512E-6 hips_estsize = 18149918 hipsgen_date = 2017-03-27T15:10Z hipsgen_params = out=GOODSz mocorder=14 "pixelCut=-7.28E-4 0.008567" UPDATE hips_initial_fov = 0.05 hips_initial_ra = 53.1239372 hips_initial_dec = -27.7398687 hips_order_min = 0 hipsgen_date_1 = 2019-05-05T06:31Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume10/GOODS/GOODSz UPDATE hips_service_url = https://alasky.cds.unistra.fr/GOODS/GOODSz hips_service_url_1 = https://alaskybis.cds.unistra.fr/GOODS/GOODSz hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 14 obs_initial_ra = 53.1239372 obs_initial_dec = -27.7398687 obs_initial_fov = 0.003578631678976464 TIMESTAMP = 1721288416222 ID = CDS/P/HST/H creator_did = ivo://CDS/P/HST/H data_pixel_bitpix = -32 dataproduct_type = image em_max = 1.8094e-06 em_min = 1.3939e-06 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:3183992321 fits:2673248344 hips_copyright = CNRS/Unistra hips_creation_date = 2019-02-25T17:15Z hips_creator = Durand D. (CDS) hips_data_range = -227.1 677.2 hips_estsize = 448032447 hips_frame = equatorial hipsgen_date = 2023-04-03T12:44Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=H -in=/data-test-iscsi/d.durand/2023A/HST/H.extract -id=CDS/P/HST/H -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/H.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_dec = 41.26939 hips_initial_fov = 0.0388 hips_initial_ra = 135.81015 hips_nb_tiles = 829872 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = 0.5396 4.412 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-04-03T17:33Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-H obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F160W filter between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Infrared client_category = Image/Infrared/HST obs_title = HST-H includes the following filters: F160W prov_progenitor = CDS (Daniel Durand) s_pixel_scale = 3.561E-5 t_max = 59995.2266813657 t_min = 50527.65335648 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_H_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_H_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_H_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 2.197E-4 moc_order = 16 obs_initial_ra = 135.81015 obs_initial_dec = 41.26939 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288455482 ID = CDS/P/HST/H2O creator_did = ivo://CDS/P/HST/H2O data_pixel_bitpix = -32 dataproduct_type = image em_min = 1.3468e-06 em_max = 1.4222e-06 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:2614946271 fits:2936564353 hips_copyright = CNRS/Unistra hips_creation_date = 2018-11-05T19:46Z hips_creator = Durand D. (CDS) hips_data_range = -3393 10111 hips_estsize = 43756637 hips_frame = equatorial hipsgen_date = 2023-03-17T18:25Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=H2O -in=/data-test-iscsi/d.durand/2023A/HST/H2O.extract -id=CDS/P/HST/H2O -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/H2O.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_dec = 30.14635 hips_initial_fov = 0.00495 hips_initial_ra = 247.89112 client_category = Image/Gas-lines/H2O hips_nb_tiles = 80130 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = -5.545 628.4 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-03-17T20:23Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-H2O obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F139M filter between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Infrared obs_title = HST-H2O includes the following filters: F139M prov_progenitor = Canadian Astronomy Data Centre s_pixel_scale = 3.562E-5 t_min = 55025.181175544 t_max = 59995.2250709838 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_H2O_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_H2O_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_H2O_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 2.626E-5 moc_order = 16 obs_initial_ra = 247.89112 obs_initial_dec = 30.14635 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288455302 ID = CDS/P/HST/Halpha creator_did = ivo://CDS/P/HST/Halpha data_pixel_bitpix = -32 dataproduct_type = image em_max = 6.649e-07 em_min = 6.493e-07 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:1055916385 fits:197743067 hips_creation_date = 2018-11-06T01:33Z hips_creator = Durand D. (CDS) hips_data_range = -2.715 6.035 hips_estsize = 83949949 hips_frame = equatorial hipsgen_date = 2023-03-21T15:30Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=Halpha -in=/data-test-iscsi/d.durand/2023A/HST/Halpha.extract -id=CDS/P/HST/Halpha -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/Halpha.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_dec = -56.3536 hips_initial_fov = 0.00603 hips_initial_ra = 10.39742 hips_nb_tiles = 153014 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = -0.2584 0.00622 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-03-21T19:29Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-Halpha obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F656N and F657N filters between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Optical client_category = Image/Gas-lines/Halpha obs_title = HST-Halpha includes the following filters: F656N and F657N prov_progenitor = CDS (Daniel Durand) s_pixel_scale = 1.100E-5 t_max = 59995.1102658218 t_min = 49350.7682582523 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_Halpha_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_Halpha_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_Halpha_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 4.338E-5 moc_order = 16 obs_initial_ra = 10.39742 obs_initial_dec = -56.3536 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288455358 ID = CDS/P/HST/Hbeta creator_did = ivo://CDS/P/HST/Hbeta data_pixel_bitpix = -32 dataproduct_type = image em_min = 4.836e-07 em_max = 4.908e-07 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:3108654858 fits:292998122 hips_copyright = CNRS/Unistra hips_creation_date = 2018-10-28T14:14Z hips_creator = Durand D. (CDS) hips_data_range = -207.1 617.8 hips_estsize = 8905568 hips_frame = equatorial hipsgen_date = 2023-03-27T13:50Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=Hbeta -in=/data-test-iscsi/d.durand/2023A/HST/Hbeta.extract -id=CDS/P/HST/Hbeta -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/Hbeta.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_dec = 22.03007 hips_initial_fov = 0.00601 hips_initial_ra = 194.2594 client_category = Image/Gas-lines/Hbeta hips_nb_tiles = 16084 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = -0.2216 0.963 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-03-27T13:57Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-Hbeta obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F487N filter between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Optical obs_title = HST-Hbeta includes the following filters: F487N prov_progenitor = Canadian Astronomy Data Centre s_pixel_scale = 1.100E-5 t_min = 49406.2842309028 t_max = 59756.6976070255 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_Hbeta_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_Hbeta_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_Hbeta_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 4.030E-6 moc_order = 16 obs_initial_ra = 194.2594 obs_initial_dec = 22.03007 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288455414 ID = CDS/P/HST/I creator_did = ivo://CDS/P/HST/I data_pixel_bitpix = -32 dataproduct_type = image em_max = 9.829e-07 em_min = 6.90e-07 hips_builder = Aladin/HipsGen v12.060 hips_copyright = CNRS/Unistra hips_creation_date = 2019-01-11T21:09Z hips_creator = Durand D. (CDS) hips_data_range = -249.7 716 hips_frame = equatorial hipsgen_date = 2023-04-11T09:50Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=I -in=/data-test-iscsi/d.durand/2023A/HST/I.extract -id=CDS/P/HST/I -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/I.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_dec = -82.2138 hips_initial_fov = 0.00591 hips_initial_ra = 225.07724 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwrite treeMedian hips_pixel_bitpix = 0 hips_pixel_cut = -0.1219 6.923 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-11-22T07:42Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-I obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F814W, F791W, F785LP and F775W filters between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Optical client_category = Image/Optical/HST obs_title = HST-I includes the following filters: F814W, F791W, F785LP and F775W prov_progenitor = CDS (Daniel Durand) s_pixel_scale = 1.100E-5 t_max = 59994.3190034722 t_min = 52365.277021331 moc_sky_fraction = 8.109E-4 hipsgen_date_1 = 2023-11-21T10:00Z hipsgen_params_1 = out=/var/www/HST-hips/filter_I_hips region=9/2632716 tree hipsgen_date_2 = 2023-11-21T10:01Z hipsgen_params_2 = out=/var/www/HST-hips/filter_I_hips region=9/2632716 tree hipsgen_date_3 = 2023-11-21T10:02Z hipsgen_params_3 = out=/var/www/HST-hips/filter_I_hips region=9/2632716 tree hipsgen_date_4 = 2023-11-21T10:02Z hipsgen_params_4 = out=/var/www/HST-hips/filter_I_hips region=9/2632716 color=png tree hipsgen_date_5 = 2023-11-21T10:04Z hipsgen_params_5 = out=/var/www/HST-hips/filter_I_hips region=9/2632716 color=png tree hipsgen_date_6 = 2023-11-21T10:04Z hipsgen_params_6 = out=/var/www/HST-hips/filter_I_hips region=9/2632716 tree hipsgen_date_7 = 2023-11-21T10:05Z hipsgen_params_7 = out=/var/www/HST-hips/filter_I_hips region=9/2632716 tree hipsgen_date_8 = 2023-11-21T10:06Z hipsgen_params_8 = out=/var/www/HST-hips/filter_I_hips region=0/0 tree hipsgen_date_9 = 2023-11-22T07:42Z hipsgen_params_9 = out=/var/www/HST-hips/filter_I_hips tree dataproduct_subtype = color hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_I_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_I_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_I_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 41 moc_time_range = 25363 moc_order = 13 obs_initial_ra = 225.07724 obs_initial_dec = -82.2138 obs_initial_fov = 0.007157263357952928 TIMESTAMP = 1728979462585 ID = CDS/P/HST/J creator_did = ivo://CDS/P/HST/J data_pixel_bitpix = -32 dataproduct_type = image em_max = 1.8121e-06 em_min = 1.0891e-06 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:3907604799 fits:35796354 hips_copyright = CNRS/Unistra hips_creation_date = 2018-12-11T19:44Z hips_creator = Durand D. (CDS) hips_data_range = -4.48 14.96 hips_estsize = 159601253 hips_frame = equatorial hipsgen_date = 2023-03-17T23:17Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=J -in=/data-test-iscsi/d.durand/2023A/HST/J.extract -id=CDS/P/HST/J -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/J.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_dec = 33.97389 hips_initial_fov = 0.04524 hips_initial_ra = 338.97432 hips_nb_tiles = 299524 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = 0.5623 1.469 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-03-18T09:25Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-J obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F140W, F125W, F125LP and F115LP filters between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community. In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Infrared client_category = Image/Infrared/HST obs_title = HST-J includes the following filters: F140W, F125W, F125LP and F115LP prov_progenitor = CDS (Daniel Durand) s_pixel_scale = 3.562E-5 t_max = 59995.2317146991 t_min = 50558.21274306 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_J_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_J_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_J_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 7.744E-5 moc_order = 16 obs_initial_ra = 338.97432 obs_initial_dec = 33.97389 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288455598 ID = CDS/P/HST/NII creator_did = ivo://CDS/P/HST/NII data_pixel_bitpix = -32 dataproduct_type = image em_max = 6.62e-07 em_min = 6.542e-07 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:277140197 fits:2532732223 hips_copyright = CNRS/Unistra hips_creation_date = 2018-11-06T15:32Z hips_creator = Durand D. (CDS) hips_data_range = -6.121 17.63 hips_estsize = 93895160 hips_frame = equatorial hipsgen_date = 2023-03-17T11:08Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=NII -in=/data-test-iscsi/d.durand/2023A/HST/NII.extract -id=CDS/P/HST/NII -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/NII.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_dec = 69.67393 hips_initial_fov = 0.00603 hips_initial_ra = 148.92554 hips_nb_tiles = 167038 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = -0.02882 0.1657 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-03-17T16:35Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-NII obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F658N filter between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Optical client_category = Image/Gas-lines/NII obs_title = HST-NII includes the following filters: F658N prov_progenitor = CDS (Daniel Durand) s_pixel_scale = 1.100E-5 t_max = 59988.4341886227 t_min = 49350.7752026968 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_NII_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_NII_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_NII_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 5.291E-5 moc_order = 16 obs_initial_ra = 148.92554 obs_initial_dec = 69.67393 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288455662 ID = CDS/P/HST/OII creator_did = ivo://CDS/P/HST/OII data_pixel_bitpix = -32 dataproduct_type = image em_min = 3.70e-07 em_max = 3.7618e-07 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:1185639961 fits:3149417244 hips_copyright = CNRS/Unistra hips_creation_date = 2018-11-27T15:35Z hips_creator = Durand D. (CDS) hips_data_range = -2.153 3.42 hips_estsize = 6646546 hips_frame = equatorial hipsgen_date = 2023-03-17T17:13Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=OII -in=/data-test-iscsi/d.durand/2023A/HST/OII.extract -id=CDS/P/HST/OII -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/OII.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_dec = -7.73557 hips_initial_fov = 0.01201 hips_initial_ra = 111.4637 hips_nb_tiles = 12088 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = -0.1958 0.5497 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-03-17T17:24Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-OII obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F375N and F373N filters between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Optical client_category = Image/Gas-lines/OII obs_title = HST-OII includes the following filters: F375N and F373N prov_progenitor = Canadian Astronomy Data Centre s_pixel_scale = 1.100E-5 t_min = 49352.8710346065 t_max = 59635.7550915162 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_OII_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_OII_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_OII_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 3.080E-6 moc_order = 16 obs_initial_ra = 111.4637 obs_initial_dec = -7.73557 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288455718 ID = CDS/P/HST/OIII creator_did = ivo://CDS/P/HST/OIII data_pixel_bitpix = -32 dataproduct_type = image em_min = 4.972e-07 em_max = 5.05e-07 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:1250509992 fits:3524012594 hips_copyright = CNRS/Unistra hips_creation_date = 2018-11-30T15:29Z hips_creator = Durand D. (CDS) hips_data_range = -113.2 339.4 hips_estsize = 62762147 hips_frame = equatorial hipsgen_date = 2023-03-21T07:12Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=OIII -in=/data-test-iscsi/d.durand/2023A/HST/OIII.extract -id=CDS/P/HST/OIII -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/OIII.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_dec = -59.81907 hips_initial_fov = 0.04514 hips_initial_ra = 160.08098 hips_nb_tiles = 113508 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = 0.01116 0.4309 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-03-21T13:12Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-OIII obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F502N filter between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Optical client_category = Image/Gas-lines/OIII obs_title = HST-OIII includes the following filters : F502N prov_progenitor = Canadian Astronomy Data Centre s_pixel_scale = 1.100E-5 t_min = 49350.7890915856 t_max = 59957.7228217245 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_OIII_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_OIII_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_OIII_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 3.143E-5 moc_order = 16 obs_initial_ra = 160.08098 obs_initial_dec = -59.81907 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288455814 ID = CDS/P/HST/PHAT/F110W creator_did = ivo://CDS/P/HST/PHAT/F110W obs_collection = HST PHAT F110W obs_title = HST PHAT - F110W - WFC3/IR obs_description = The Panchromatic Hubble Andromeda Treasury is a Hubble Space Telescope Multi-cycle program to map roughly a third of M31's star forming disk, using 6 filters covering from the ultraviolet through the near infrared - see 2012ApJS..200...18D obs_ack = Original images retrieved from MAST/NASA obs_copyright = PHAT team obs_copyright_url = http://www.astro.washington.edu/groups/phat/Home.html client_category = Image/Optical/HST/PHAT client_sort_key = 03-05-05-01 hips_release_date = 2019-05-05T06:32Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Boch T. (CDS) hips_version = 1.4 hips_order = 14 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png jpeg fits dataproduct_type = image hips_pixel_cut = 0 15 hips_data_range = -9800 6038 hips_initial_ra = 10.72797 hips_initial_dec = +41.25464 hips_initial_fov = 0.45616 moc_access_url = http://alasky.u-strasbg.fr/PHAT/F110W/Moc.fits hips_progenitor_url = https://alasky.cds.unistra.fr/PHAT/F110W/HpxFinder hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = MAST archives bib_reference = 2012ApJS..200...18D bib_reference_url = http://adsabs.harvard.edu/cgi-bin/nph-bib_query?db_key=AST&bibcode=2012ApJS..200...18D t_min = 55398 t_max = 55807 obs_regime = Optical em_min = 8.832e-7 em_max = 1.4121e-6 hips_pixel_scale = 6.989E-6 hips_creation_date = 2015-02-03T11:17Z hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1.204E-5 hips_estsize = 65534776 hipsgen_date = 2019-05-05T06:32Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/PHAT/F110W UPDATE hips_service_url = https://alasky.cds.unistra.fr/PHAT/F110W hips_service_url_1 = https://alaskybis.cds.unistra.fr/PHAT/F110W hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 19 obs_initial_ra = 10.72797 obs_initial_dec = +41.25464 obs_initial_fov = 1.118322399680145E-4 TIMESTAMP = 1721288416274 ID = CDS/P/HST/PHAT/F160W creator_did = ivo://CDS/P/HST/PHAT/F160W obs_collection = HST PHAT F160W obs_title = HST PHAT - F160W - WFC3/IR obs_description = The Panchromatic Hubble Andromeda Treasury is a Hubble Space Telescope Multi-cycle program to map roughly a third of M31's star forming disk, using 6 filters covering from the ultraviolet through the near infrared - see 2012ApJS..200...18D obs_ack = Original images retrieved from MAST/NASA obs_copyright = PHAT team obs_copyright_url = http://www.astro.washington.edu/groups/phat/Home.html client_category = Image/Optical/HST/PHAT client_sort_key = 03-05-05-02 hips_release_date = 2019-05-05T06:33Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Boch T. (CDS) hips_version = 1.4 hips_order = 14 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png jpeg fits dataproduct_type = image hips_pixel_cut = 0 6 hips_data_range = -29.11 101.7 hips_initial_ra = 10.72797 hips_initial_dec = +41.25464 hips_initial_fov = 0.45616 moc_access_url = http://alasky.u-strasbg.fr/PHAT/F160W/Moc.fits hips_progenitor_url = https://alasky.cds.unistra.fr/PHAT/F160W/HpxFinder hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = MAST archives bib_reference = 2012ApJS..200...18D bib_reference_url = http://adsabs.harvard.edu/cgi-bin/nph-bib_query?db_key=AST&bibcode=2012ApJS..200...18D t_min = 55398 t_max = 55807 obs_regime = Optical em_min = 1.3854e-6 em_max = 1.6999e-6 hips_pixel_scale = 6.989E-6 hips_creation_date = 2015-02-03T16:13Z hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1.205E-5 hips_estsize = 65558235 hipsgen_date = 2019-05-05T06:33Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/PHAT/F160W UPDATE hips_service_url = https://alasky.cds.unistra.fr/PHAT/F160W hips_service_url_1 = https://alaskybis.cds.unistra.fr/PHAT/F160W hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 19 obs_initial_ra = 10.72797 obs_initial_dec = +41.25464 obs_initial_fov = 1.118322399680145E-4 TIMESTAMP = 1721288416330 ID = CDS/P/HST/PHAT/F275W creator_did = ivo://CDS/P/HST/PHAT/F275W obs_collection = HST PHAT F275W obs_title = HST PHAT - F275W - WFC3/UVIS obs_description = The Panchromatic Hubble Andromeda Treasury is a Hubble Space Telescope Multi-cycle program to map roughly a third of M31's star forming disk, using 6 filters covering from the ultraviolet through the near infrared - see 2012ApJS..200...18D obs_ack = Original images retrieved from MAST/NASA obs_copyright = PHAT team obs_copyright_url = http://www.astro.washington.edu/groups/phat/Home.html client_category = Image/Optical/HST/PHAT client_sort_key = 03-05-05-02 hips_release_date = 2019-05-05T06:33Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Boch T. (CDS) hips_version = 1.4 hips_order = 14 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png jpeg fits dataproduct_type = image hips_pixel_cut = 0 0.02 hips_data_range = -0.4033 1.147 hips_initial_ra = 10.72793 hips_initial_dec = +41.25472 hips_initial_fov = 0.43254 moc_access_url = http://alasky.u-strasbg.fr/PHAT/F275W/Moc.fits hips_progenitor_url = https://alasky.cds.unistra.fr/PHAT/F275W/HpxFinder hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = MAST archives bib_reference = 2012ApJS..200...18D bib_reference_url = http://adsabs.harvard.edu/cgi-bin/nph-bib_query?db_key=AST&bibcode=2012ApJS..200...18D t_min = 55398 t_max = 55807 obs_regime = Optical em_min = 2.282e-7 em_max = 3.119e-7 hips_pixel_scale = 6.989E-6 hips_creation_date = 2015-02-04T13:43Z hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1.263E-5 hips_estsize = 67439454 hipsgen_date = 2019-05-05T06:33Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/PHAT/F275W UPDATE hips_service_url = https://alasky.cds.unistra.fr/PHAT/F275W hips_service_url_1 = https://alaskybis.cds.unistra.fr/PHAT/F275W hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 19 obs_initial_ra = 10.72793 obs_initial_dec = +41.25472 obs_initial_fov = 1.118322399680145E-4 TIMESTAMP = 1721288416390 ID = CDS/P/HST/PHAT/F336W creator_did = ivo://CDS/P/HST/PHAT/F336W obs_collection = HST PHAT F336W obs_title = HST PHAT - F336W - WFC3/UVIS obs_description = The Panchromatic Hubble Andromeda Treasury is a Hubble Space Telescope Multi-cycle program to map roughly a third of M31's star forming disk, using 6 filters covering from the ultraviolet through the near infrared - see 2012ApJS..200...18D obs_ack = Original images retrieved from MAST/NASA obs_copyright = PHAT team obs_copyright_url = http://www.astro.washington.edu/groups/phat/Home.html client_category = Image/Optical/HST/PHAT client_sort_key = 03-05-05-04 hips_release_date = 2019-05-05T06:33Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Boch T. (CDS) hips_version = 1.4 hips_order = 14 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png jpeg fits dataproduct_type = image hips_pixel_cut = 0 0.015 hips_data_range = -1.182 3.582 hips_initial_ra = 10.72793 hips_initial_dec = +41.25472 hips_initial_fov = 0.43256 moc_access_url = http://alasky.u-strasbg.fr/PHAT/F336W/Moc.fits hips_progenitor_url = https://alasky.cds.unistra.fr/PHAT/F336W/HpxFinder hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = MAST archives bib_reference = 2012ApJS..200...18D bib_reference_url = http://adsabs.harvard.edu/cgi-bin/nph-bib_query?db_key=AST&bibcode=2012ApJS..200...18D t_min = 55398 t_max = 55807 obs_regime = Optical em_min = 3.014e-7 em_max = 3.707e-7 hips_pixel_scale = 6.989E-6 hips_creation_date = 2015-02-05T17:14Z hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1.263E-5 hips_estsize = 67435056 hipsgen_date = 2019-05-05T06:33Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/PHAT/F336W UPDATE hips_service_url = https://alasky.cds.unistra.fr/PHAT/F336W hips_service_url_1 = https://alaskybis.cds.unistra.fr/PHAT/F336W hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 19 obs_initial_ra = 10.72793 obs_initial_dec = +41.25472 obs_initial_fov = 1.118322399680145E-4 TIMESTAMP = 1721288416446 ID = CDS/P/HST/PHAT/F475W creator_did = ivo://CDS/P/HST/PHAT/F475W obs_collection = HST PHAT F475W obs_title = HST PHAT - F475W - ACS/WFC obs_description = The Panchromatic Hubble Andromeda Treasury is a Hubble Space Telescope Multi-cycle program to map roughly a third of M31's star forming disk, using 6 filters covering from the ultraviolet through the near infrared - see 2012ApJS..200...18D obs_ack = Original images retrieved from MAST/NASA obs_copyright = PHAT team obs_copyright_url = http://www.astro.washington.edu/groups/phat/Home.html client_category = Image/Optical/HST/PHAT client_sort_key = 03-05-05-05 hips_release_date = 2019-05-05T06:34Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Boch T. (CDS) hips_version = 1.4 hips_order = 14 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png jpeg fits dataproduct_type = image hips_pixel_cut = 0 1.6 hips_data_range = -16.61 52.56 hips_initial_ra = 10.7279 hips_initial_dec = +41.25452 hips_initial_fov = 0.46288 moc_access_url = http://alasky.u-strasbg.fr/PHAT/F475W/Moc.fits hips_progenitor_url = https://alasky.cds.unistra.fr/PHAT/F475W/HpxFinder hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = MAST archives bib_reference = 2012ApJS..200...18D bib_reference_url = http://adsabs.harvard.edu/cgi-bin/nph-bib_query?db_key=AST&bibcode=2012ApJS..200...18D t_min = 55398 t_max = 55807 obs_regime = Optical em_min = 3.863e-7 em_max = 5.563e-7 hips_pixel_scale = 6.989E-6 hips_creation_date = 2015-02-06T12:36Z hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1.338E-5 hips_estsize = 91316134 hipsgen_date = 2019-05-05T06:34Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/PHAT/F475W UPDATE hips_service_url = https://alasky.cds.unistra.fr/PHAT/F475W hips_service_url_1 = https://alaskybis.cds.unistra.fr/PHAT/F475W hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 19 obs_initial_ra = 10.7279 obs_initial_dec = +41.25452 obs_initial_fov = 1.118322399680145E-4 TIMESTAMP = 1721288416502 ID = CDS/P/HST/PHAT/F814W creator_did = ivo://CDS/P/HST/PHAT/F814W obs_collection = HST PHAT F814W obs_title = HST PHAT - F814W - ACS/WFC obs_description = The Panchromatic Hubble Andromeda Treasury is a Hubble Space Telescope Multi-cycle program to map roughly a third of M31's star forming disk, using 6 filters covering from the ultraviolet through the near infrared - see 2012ApJS..200...18D obs_ack = Original images retrieved from MAST/NASA obs_copyright = PHAT team obs_copyright_url = http://www.astro.washington.edu/groups/phat/Home.html client_category = Image/Optical/HST/PHAT client_sort_key = 03-05-05-06 hips_release_date = 2019-05-05T06:34Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Boch T. (CDS) hips_version = 1.4 hips_order = 14 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png jpeg fits dataproduct_type = image hips_pixel_cut = 0 3 hips_data_range = -6.698 27.91 hips_initial_ra = 10.72791 hips_initial_dec = +41.25453 hips_initial_fov = 0.4627 moc_access_url = http://alasky.u-strasbg.fr/PHAT/F814W/Moc.fits hips_progenitor_url = https://alasky.cds.unistra.fr/PHAT/F814W/HpxFinder hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = MAST archives bib_reference = 2012ApJS..200...18D bib_reference_url = http://adsabs.harvard.edu/cgi-bin/nph-bib_query?db_key=AST&bibcode=2012ApJS..200...18D t_min = 55398 t_max = 55807 obs_regime = Optical em_min = 6.885e-7 em_max = 9.648e-7 hips_pixel_scale = 6.989E-6 hips_creation_date = 2015-02-10T02:50Z hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 1.339E-5 hips_estsize = 91316134 hipsgen_date = 2019-05-05T06:34Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/PHAT/F814W UPDATE hips_service_url = https://alasky.cds.unistra.fr/PHAT/F814W hips_service_url_1 = https://alaskybis.cds.unistra.fr/PHAT/F814W hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 19 obs_initial_ra = 10.72791 obs_initial_dec = +41.25453 obs_initial_fov = 1.118322399680145E-4 TIMESTAMP = 1721288416558 ID = CDS/P/HST/PHAT/color creator_did = ivo://CDS/P/HST/PHAT/color obs_collection = HST PHAT obs_title = HST PHAT color obs_description = The Panchromatic Hubble Andromeda Treasury is a HST program to map a third of M31's star forming disk. This color HiPS has been generated from filters F475W (blue) and F814W (red). obs_ack = Original images retrieved from MAST/NASA obs_copyright = PHAT team obs_copyright_url = http://www.astro.washington.edu/groups/phat/Home.html client_category = Image/Optical/HST/PHAT client_sort_key = 03-05-05-07 hips_release_date = 2023-06-27T12:05Z hips_builder = Aladin/HipsGen v12.060 hips_creator = Boch T. (CDS) hips_version = 1.4 hips_order = 14 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png dataproduct_type = image hips_initial_ra = 11.0447921 hips_initial_dec = +41.5343786 hips_initial_fov = 1.45616 hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = MAST archives bib_reference = 2012ApJS..200...18D bib_reference_url = http://adsabs.harvard.edu/cgi-bin/nph-bib_query?db_key=AST&bibcode=2012ApJS..200...18D t_min = 55398 t_max = 55807 obs_regime = Optical em_min = 3.863e-7 em_max = 9.648e-7 hips_pixel_scale = 6.989E-6 hips_creation_date = 2023-06-27T12:05Z hips_order_min = 0 moc_sky_fraction = 1.369E-5 hips_overlay = overlayMean mergeOverwrite treeMedian hipsgen_date = 2023-06-27T08:07Z hipsgen_params = out=/volume10/PHAT/color TREE hipsgen_date_1 = 2023-06-27T08:15Z hipsgen_params_1 = out=/volume10/PHAT/color TREE hipsgen_date_2 = 2023-06-27T08:17Z hipsgen_params_2 = out=/volume10/PHAT/color TREE hipsgen_date_3 = 2023-06-27T08:20Z hipsgen_params_3 = out=/volume10/PHAT/color TREE hipsgen_date_4 = 2023-06-27T08:23Z hipsgen_params_4 = out=/volume10/PHAT/color TREE hipsgen_date_5 = 2023-06-27T08:26Z hipsgen_params_5 = out=/volume10/PHAT/color TREE hipsgen_date_6 = 2023-06-27T08:29Z hipsgen_params_6 = out=/volume10/PHAT/color TREE hipsgen_date_7 = 2023-06-27T08:32Z hipsgen_params_7 = out=/volume10/PHAT/color TREE hipsgen_date_8 = 2023-06-27T08:44Z hipsgen_params_8 = out=/volume10/PHAT/color TREE hipsgen_date_9 = 2023-06-27T08:45Z hipsgen_params_9 = out=/volume10/PHAT/color TREE hipsgen_date_10 = 2023-06-27T08:48Z hipsgen_params_10 = out=/volume10/PHAT/color TREE hipsgen_date_11 = 2023-06-27T08:49Z hipsgen_params_11 = out=/volume10/PHAT/color TREE hipsgen_date_12 = 2023-06-27T08:51Z hipsgen_params_12 = out=/volume10/PHAT/color TREE hipsgen_date_13 = 2023-06-27T08:52Z hipsgen_params_13 = out=/volume10/PHAT/color TREE hipsgen_date_14 = 2023-06-27T08:52Z hipsgen_params_14 = out=/volume10/PHAT/color TREE hipsgen_date_15 = 2023-06-27T08:53Z hipsgen_params_15 = out=/volume10/PHAT/color TREE hipsgen_date_16 = 2023-06-27T08:55Z hipsgen_params_16 = out=/volume10/PHAT/color TREE hipsgen_date_17 = 2023-06-27T08:55Z hipsgen_params_17 = out=/volume10/PHAT/color TREE hipsgen_date_18 = 2023-06-27T08:56Z hipsgen_params_18 = out=/volume10/PHAT/color TREE hipsgen_date_19 = 2023-06-27T08:57Z hipsgen_params_19 = out=/volume10/PHAT/color TREE hipsgen_date_20 = 2023-06-27T08:58Z hipsgen_params_20 = out=/volume10/PHAT/color TREE hipsgen_date_21 = 2023-06-27T08:58Z hipsgen_params_21 = out=/volume10/PHAT/color TREE hipsgen_date_22 = 2023-06-27T08:59Z hipsgen_params_22 = out=/volume10/PHAT/color TREE hipsgen_date_23 = 2023-06-27T09:00Z hipsgen_params_23 = out=/volume10/PHAT/color TREE hipsgen_date_24 = 2023-06-27T09:00Z hipsgen_params_24 = out=/volume10/PHAT/color TREE hipsgen_date_25 = 2023-06-27T09:01Z hipsgen_params_25 = out=/volume10/PHAT/color TREE hipsgen_date_26 = 2023-06-27T09:02Z hipsgen_params_26 = out=/volume10/PHAT/color TREE hipsgen_date_27 = 2023-06-27T09:03Z hipsgen_params_27 = out=/volume10/PHAT/color TREE hipsgen_date_28 = 2023-06-27T09:30Z hipsgen_params_28 = out=/volume10/PHAT/color TREE hipsgen_date_29 = 2023-06-27T09:42Z hipsgen_params_29 = out=/volume10/PHAT/color TREE hipsgen_date_30 = 2023-06-27T11:59Z hipsgen_params_30 = out=/volume10/PHAT/color TREE hipsgen_date_31 = 2023-06-27T12:05Z hipsgen_params_31 = out=/volume10/PHAT/color TREE dataproduct_subtype = color hips_service_url = https://alasky.cds.unistra.fr/PHAT/color hips_service_url_1 = https://alaskybis.cds.unistra.fr/PHAT/color hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 14 obs_initial_ra = 11.0447921 obs_initial_dec = +41.5343786 obs_initial_fov = 0.003578631678976464 TIMESTAMP = 1721288416630 ID = CDS/P/HST/Palpha creator_did = ivo://CDS/P/HST/Palpha data_pixel_bitpix = -32 dataproduct_type = image em_min = 1.863e-06 em_max = 1.884e-06 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:1955719950 fits:54145660 hips_copyright = CNRS/Unistra hips_creation_date = 2018-11-05T20:10Z hips_creator = Durand D. (CDS) hips_data_range = -8.072 18.39 hips_estsize = 17062403 hips_frame = equatorial hipsgen_date = 2023-03-16T17:11Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=Palpha -in=/data-test-iscsi/d.durand/2023A/HST/Palpha.extract -id=CDS/P/HST/Palpha -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/Palpha.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_dec = -5.3885432 hips_initial_fov = 0.00309 hips_initial_ra = 83.8166730 hips_nb_tiles = 32248 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = -0.1657 1.301 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-03-16T17:17Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-Palpha obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F187N filter between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community. In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Infrared client_category = Image/Gas-lines/Palpha obs_title = HST-Palpha includes the following filters : F187N prov_progenitor = Canadian Astronomy Data Centre s_pixel_scale = 1.203E-5 t_min = 50546.00081019 t_max = 55094.0826043171 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_Palpha_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_Palpha_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_Palpha_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 5.057E-6 moc_order = 16 obs_initial_ra = 83.8166730 obs_initial_dec = -5.3885432 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288456002 ID = CDS/P/HST/Palpha_c creator_did = ivo://CDS/P/HST/Palpha_c data_pixel_bitpix = -32 dataproduct_type = image em_min = 1.89085e-06 em_max = 1.90875e-06 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:3966897905 fits:2715405292 hips_copyright = CNRS/Unistra hips_creation_date = 2018-11-05T20:16Z hips_creator = Durand D. (CDS) hips_data_range = -6.179 16.76 hips_estsize = 15303793 hips_frame = equatorial hipsgen_date = 2023-03-16T18:55Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=Palpha_c -in=/data-test-iscsi/d.durand/2023A/HST/Palpha_c.extract -id=CDS/P/HST/Palpha_c -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/Palpha_c.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_dec = -29.8654127 hips_initial_fov = 0.0109 hips_initial_ra = 204.2525923 hips_nb_tiles = 28888 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = -0.03987 1.115 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-03-16T19:25Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-Palpha_c obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F190N filter between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Infrared client_category = Image/Gas-lines/Palphac obs_title = HST-Palpha_c includes the following filters : F190N prov_progenitor = Canadian Astronomy Data Centre s_pixel_scale = 1.203E-5 t_min = 50546.01451389 t_max = 55094.08190972 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_Palpha_c_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_Palpha_c_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_Palpha_c_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 5.273E-6 moc_order = 16 obs_initial_ra = 204.2525923 obs_initial_dec = -29.8654127 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288455938 ID = CDS/P/HST/R creator_did = ivo://CDS/P/HST/R data_pixel_bitpix = -32 dataproduct_type = image em_min = 6.1256e-07 em_max = 7.792e-07 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:2980294800 fits:2647648570 hips_copyright = CNRS/Unistra hips_creation_date = 2018-11-05T23:27Z hips_creator = Durand D. (CDS) hips_data_range = -209.3 594.6 hips_estsize = 98149807 hips_frame = equatorial hipsgen_date = 2023-03-18T12:12Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=R -in=/data-test-iscsi/d.durand/2023A/HST/R.extract -id=CDS/P/HST/R -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/R.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_dec = +47.1952583 hips_initial_fov = 0.04216 hips_initial_ra = 202.4695750 hips_nb_tiles = 183156 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = -0.02662 1.175 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-03-18T18:53Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-R obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F702W and F675W filters between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Optical client_category = Image/Optical/HST obs_title = HST-R includes the following filters : F702W and F675W prov_progenitor = Canadian Astronomy Data Centre s_pixel_scale = 2.762E-5 t_min = 49350.9939512384 t_max = 54950.1693591088 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_R_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_R_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_R_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 4.555E-5 moc_order = 16 obs_initial_ra = 202.4695750 obs_initial_dec = +47.1952583 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288456066 ID = CDS/P/HST/SDSSg creator_did = ivo://CDS/P/HST/SDSSg data_pixel_bitpix = -32 dataproduct_type = image em_max = 5.541e-07 em_min = 3.90e-07 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:4078104273 fits:1156517727 hips_copyright = CNRS/Unistra hips_creation_date = 2018-12-12T23:20Z hips_creator = Durand D. (CDS) hips_data_range = -5813 16522 hips_estsize = 243690116 hips_frame = equatorial hipsgen_date = 2023-03-18T20:37Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=SDSSg -in=/data-test-iscsi/d.durand/2023A/HST/SDSSg.extract -id=CDS/P/HST/SDSSg -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/SDSSg.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_dec = +30.6601751 hips_initial_fov = 0.07 hips_initial_ra = 23.4620691 hips_nb_tiles = 430270 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = -1.618 25.34 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-03-19T17:33Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-SDSSg obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F475W filter between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Optical client_category = Image/Optical/HST obs_title = HST-SDSSg incudes the following filters: F475W prov_progenitor = CDS (Daniel Durand) s_pixel_scale = 1.100E-5 t_max = 59988.3558437847 t_min = 52355.8182133102 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_SDSSg_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_SDSSg_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_SDSSg_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 1.347E-4 moc_order = 16 obs_initial_ra = 23.4620691 obs_initial_dec = +30.6601751 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288456130 ID = CDS/P/HST/SDSSr creator_did = ivo://CDS/P/HST/SDSSr data_pixel_bitpix = -32 dataproduct_type = image em_max = 7.093e-07 em_min = 5.454e-07 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:1406365085 fits:1623891900 hips_copyright = CNRS/Unistra hips_creation_date = 2018-12-03T18:51Z hips_creator = Durand D. (CDS) hips_data_range = -38.21 111.6 hips_estsize = 95707274 hips_frame = equatorial hipsgen_date = 2023-03-19T18:17Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=SDSSr -in=/data-test-iscsi/d.durand/2023A/HST/SDSSr.extract -id=CDS/P/HST/SDSSr -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/SDSSr.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_ra = 49.9506666 hips_initial_dec = 41.5116969 hips_initial_fov = 0.04827 hips_nb_tiles = 170104 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = -0.005109 0.05189 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-03-20T01:01Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-SDSSr obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F625W and F622W filters between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Optical client_category = Image/Optical/HST obs_title = HST-SDSSr includes the following filters: F625W and F622W prov_progenitor = CDS (Daniel Durand) s_pixel_scale = 1.100E-5 t_max = 59994.6446400463 t_min = 49409.6654794792 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_SDSSr_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_SDSSr_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_SDSSr_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 4.945E-5 moc_order = 16 obs_initial_ra = 49.9506666 obs_initial_dec = 41.5116969 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288456182 ID = CDS/P/HST/SDSSz creator_did = ivo://CDS/P/HST/SDSSz data_pixel_bitpix = -32 dataproduct_type = image em_max = 1.0074e-06 em_min = 8.414e-07 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:2258977454 fits:1711475728 hips_copyright = CNRS/Unistra hips_creation_date = 2018-12-13T13:31Z hips_creator = Durand D. (CDS) hips_data_range = -509.6 1522 hips_estsize = 173234555 hips_frame = equatorial hipsgen_date = 2023-03-20T18:01Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=SDSSz -in=/data-test-iscsi/d.durand/2023A/HST/SDSSz.extract -id=CDS/P/HST/SDSSz -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/SDSSz.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_ra = 187.7055511 hips_initial_dec = 12.3913690 hips_initial_fov = 0.034 hips_nb_tiles = 307488 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = -0.07657 2.873 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-03-21T03:20Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-SDSSz obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F850LP filter between the beginning of the mission to early 2021.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Optical client_category = Image/Optical/HST obs_title = HST-SDSSz includes the following filters: F850LP prov_progenitor = CDS (Daniel Durand) s_pixel_scale = 1.100E-5 t_max = 59981.8992693287 t_min = 49604.1119957176 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_SDSSz_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_SDSSz_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_SDSSz_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 9.537E-5 moc_order = 16 obs_initial_ra = 187.7055511 obs_initial_dec = 12.3913690 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288456238 ID = CDS/P/HST/SIII creator_did = ivo://CDS/P/HST/SIII data_pixel_bitpix = -32 dataproduct_type = image em_min = 6.697e-07 em_max = 6.84e-07 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:3304371963 fits:2797569037 hips_copyright = CNRS/Unistra hips_creation_date = 2018-12-01T20:05Z hips_creator = Durand D. (CDS) hips_data_range = -8.13 24.76 hips_estsize = 33341047 hips_frame = equatorial hipsgen_date = 2023-03-20T14:13Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=SIII -in=/data-test-iscsi/d.durand/2023A/HST/SIII.extract -id=CDS/P/HST/SIII -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/SIII.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_dec = -5.40244 hips_initial_fov = 0.02401 hips_initial_ra = 83.80693 hips_nb_tiles = 60442 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = 0.1367 0.7955 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-03-20T15:32Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-SIII obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F673N, FQ672N and FQ674N filters between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Optical client_category = Image/Gas-lines/SIII obs_title = HST-SIII includes the following fiters: F673N, FQ672N and FQ674N prov_progenitor = CDS (Daniel Durand) s_pixel_scale = 1.100E-5 t_min = 49354.8050638542 t_max = 59746.6990074074 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_SIII_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_SIII_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_SIII_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 1.689E-5 moc_order = 16 obs_initial_ra = 83.80693 obs_initial_dec = -5.40244 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288456290 ID = CDS/P/HST/U creator_did = ivo://CDS/P/HST/U data_pixel_bitpix = -32 dataproduct_type = image em_min = 2.432e-07 em_max = 3.70e-07 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:3039601896 fits:501597783 hips_copyright = CNRS/Unistra hips_creation_date = 2018-12-04T22:55Z hips_creator = Durand D. (CDS) hips_data_range = -3800 10397 hips_estsize = 420678358 hips_frame = equatorial hipsgen_date = 2023-03-25T14:39Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=U -in=/data-test-iscsi/d.durand/2023A/HST/U.extract -id=CDS/P/HST/U -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/U.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_dec = 22.03113 hips_initial_fov = 0.00633 hips_initial_ra = 194.2599 hips_nb_tiles = 757934 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = -1.659 12.44 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-03-26T00:00Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-U obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F336W, F330W, F300W and F275W filters between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = UV client_category = Image/UV/HST obs_title = HST-U includes the following filters : F336W, F330W, F300W and F275W prov_progenitor = Canadian Astronomy Data Centre s_pixel_scale = 1.100E-5 t_min = 49354.4599234954 t_max = 59994.9394558218 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_U_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_U_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_U_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 2.183E-4 moc_order = 16 obs_initial_ra = 194.2599 obs_initial_dec = 22.03113 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288456346 ID = CDS/P/HST/UV creator_did = ivo://CDS/P/HST/UV data_pixel_bitpix = -32 dataproduct_type = image em_min = 1.4352e-07 em_max = 1.9803e-07 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:945339934 fits:1220995521 hips_copyright = CNRS/Unistra hips_creation_date = 2018-11-05T20:31Z hips_creator = Durand D. (CDS) hips_data_range = -492.7 1189 hips_estsize = 13914445 hips_frame = equatorial hipsgen_date = 2023-03-20T10:35Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=UV -in=/data-test-iscsi/d.durand/2023A/HST/UV.extract -id=CDS/P/HST/UV -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/UV.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_dec = 33.96446 hips_initial_fov = 0.04208 hips_initial_ra = 66.15013 hips_nb_tiles = 25986 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = -0.05474 5.932 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-03-20T11:24Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-UV obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F170W filter between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = UV obs_title = HST-UV includes the following filters: F170W prov_progenitor = Canadian Astronomy Data Centre s_pixel_scale = 2.766E-5 t_min = 49354.6092290856 t_max = 54957.6758407755 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_UV_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_UV_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_UV_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 7.121E-6 moc_order = 16 obs_initial_ra = 66.15013 obs_initial_dec = 33.96446 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288456414 ID = CDS/P/HST/V creator_did = ivo://CDS/P/HST/V data_pixel_bitpix = -32 dataproduct_type = image em_min = 4.417e-07 em_max = 6.591e-07 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:2679388138 fits:3802114409 hips_copyright = CNRS/Unistra hips_creation_date = 2019-01-08T22:06Z hips_creator = Durand D. (CDS) hips_data_range = -6011 17345 hips_estsize = 216266415 hips_frame = equatorial hipsgen_date = 2023-03-28T19:51Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=V -in=/data-test-iscsi/d.durand/2023A/HST/V.extract -id=CDS/P/HST/V -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/V.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_ra = 40.6696215 hips_initial_dec = -0.0132943 hips_initial_fov = 0.0633 hips_nb_tiles = 386258 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = -1.973 22.59 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-03-28T23:11Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-V obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F555W, F547M and F569W filters between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Optical client_category = Image/Optical/HST obs_title = HST-V includes the following filters: F555W, F547M, F569W prov_progenitor = Canadian Astronomy Data Centre s_pixel_scale = 1.100E-5 t_min = 49341.4036734144 t_max = 59994.9346176736 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_V_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_V_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_V_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 1.088E-4 moc_order = 16 obs_initial_ra = 40.6696215 obs_initial_dec = -0.0132943 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288456478 ID = CDS/P/HST/Y creator_did = ivo://CDS/P/HST/Y data_pixel_bitpix = -32 dataproduct_type = image em_min = 8.4225e-07 em_max = 1.42975e-06 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:978164543 fits:2356483153 hips_copyright = CNRS/Unistra hips_creation_date = 2018-12-04T16:59Z hips_creator = Durand D. (CDS) hips_data_range = -759.8 2279 hips_estsize = 299253250 hips_frame = equatorial hipsgen_date = 2023-04-03T22:00Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=Y -in=/data-test-iscsi/d.durand/2023A/HST/Y.extract -id=CDS/P/HST/Y -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/Y.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_dec = 7.5033 hips_initial_fov = 0.03883 hips_initial_ra = 207.51031 hips_nb_tiles = 555682 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = 2.944 6.147 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-04-04T00:57Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-Y obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F110W and F105W filters between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Infrared client_category = Image/Infrared/HST obs_title = HST-Y includes the following filters: F110W and F105W prov_progenitor = Canadian Astronomy Data Centre s_pixel_scale = 3.561E-5 t_min = 50511.6990537847 t_max = 59995.2202117245 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_Y_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_Y_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_Y_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 1.363E-4 moc_order = 16 obs_initial_ra = 207.51031 obs_initial_dec = 7.5033 obs_initial_fov = 8.94657919744116E-4 TIMESTAMP = 1721288456682 ID = CDS/P/HST/other hips_initial_fov = 0.02386 hips_initial_ra = 11.70394 hips_initial_dec = +85.26036 creator_did = ivo://CDS/P/HST/other hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = median hips_creator = Durand D. (CDS) hips_copyright = CNRS/Unistra obs_title = HST-Others includes the ALL the other filters not used in other HIPS obs_collection = HST-Others obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done with filters NOT included within the other HIPS between the beginning of the mission to the end of 2018.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope,obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. This research used the facilities of the Canadian Astronomy Data Centre operated by the National Research Council of Canada with the support of the Canadian Space Agency. " prov_progenitor = Canadian Astronomy Data Centre t_min = 49404.4050642 t_max = 58388.777623 client_category = Image/Optical/HST obs_regime = Optical hips_builder = Aladin/HipsGen v10.123 hips_version = 1.4 hips_release_date = 2019-05-07T11:21Z hips_frame = equatorial hips_order = 13 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = 0 0.15 hips_data_range = -122.9 355.5 hips_pixel_scale = 1.397E-5 s_pixel_scale = 1.100E-5 dataproduct_type = image moc_sky_fraction = 1.295E-4 hips_estsize = 153579078 hipsgen_date = 2019-01-14T18:04Z hipsgen_params = -maxThread=25 "-creator=CADC (Daniel Durand)" -label=other -in=filter_other_extract -ID=CDS/P/HST/other -force -blank=0 -order=13 -mocOrder=16 -out=filter_other_hips "-pixelCut=0.0 0.15" "-fitskeys=INSTRUME OPT_ELE DETECTOR T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME NMEMBERS DSNAME OBS_DATE URLPATH URLPREV" hips_creation_date = 2019-01-14T18:04Z hipsgen_date_1 = 2019-01-14T19:28Z hipsgen_params_1 = -maxThread=25 "-creator=CADC (Daniel Durand)" -label=other -in=filter_other_extract -ID=CDS/P/HST/other -force -blank=0 -order=13 -mocOrder=16 -out=filter_other_hips "-pixelCut=0.0 0.15" "-fitskeys=INSTRUME OPT_ELE DETECTOR T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME NMEMBERS DSNAME OBS_DATE URLPATH URLPREV" hipsgen_date_2 = 2019-02-22T01:19Z hipsgen_params_2 = -maxThread=25 "-creator=CADC (Daniel Durand)" -label=other -in=filter_other_extract -ID=CDS/P/HST/other -force -blank=0 -order=13 -mocOrder=16 -out=filter_other_hips "-pixelCut=0.0 0.15" "-fitskeys=INSTRUME OPT_ELE DETECTOR T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME NMEMBERS DSNAME OBS_DATE URLPATH URLPREV" hipsgen_date_3 = 2019-02-22T02:51Z hipsgen_params_3 = -maxThread=25 "-creator=CADC (Daniel Durand)" -label=other -in=filter_other_extract -ID=CDS/P/HST/other -force -blank=0 -order=13 -mocOrder=16 -out=filter_other_hips "-pixelCut=0.0 0.15" "-fitskeys=INSTRUME OPT_ELE DETECTOR T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME NMEMBERS DSNAME OBS_DATE URLPATH URLPREV" hipsgen_date_4 = 2019-05-07T11:21Z hipsgen_params_4 = out=/asd-volumes/sc1-asd-volume8/HST-hips/filter_other_hips UPDATE hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_other_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_other_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_other_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 41 moc_time_range = 12160 moc_order = 13 obs_initial_ra = 11.70394 obs_initial_dec = +85.26036 obs_initial_fov = 0.007157263357952928 TIMESTAMP = 1721288455882 ID = CDS/P/HST/wideUV creator_did = ivo://CDS/P/HST/wideUV data_pixel_bitpix = -32 dataproduct_type = image em_min = 1.85e-07 em_max = 3.40e-07 hips_builder = Aladin/HipsGen v12.060 hips_copyright = CNRS/Unistra hips_creation_date = 2018-11-06T22:34Z hips_creator = Durand D. (CDS) hips_data_range = -0.6436 0.6151 hips_frame = equatorial hipsgen_date = 2023-03-25T10:21Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=wideUV -in=/data-test-iscsi/d.durand/2023A/HST/wideUV.extract -id=CDS/P/HST/wideUV -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/wideUV.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_initial_dec = 7.77683 hips_initial_fov = 0.04827 hips_initial_ra = 169.56126 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = -0.002088 0.00658 hips_pixel_scale = 0.229 hips_release_date = 2023-06-29T10:06Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-wideUV obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F255W, F250W, F225W, F220W and F218W filters between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = UV client_category = Image/UV/HST obs_title = HST-wideUV includes the following filters : F255W, F250W, F225W, F220W and F218W prov_progenitor = Canadian Astronomy Data Centre s_pixel_scale = 1.093E-5 t_min = 49386.0849252662 t_max = 59984.9037137732 moc_sky_fraction = 6.646E-5 hipsgen_date_1 = 2023-06-29T09:50Z hipsgen_params_1 = out=/var/www/HST-hips/filter_wideUV_hips "-pixelCut=9% 99.9% byRegion/20Mpix log" PNG hips_estsize = 97278740 hips_nb_tiles = 173574 hips_check_code = png:2531693457 fits:2983497987 hipsgen_date_2 = 2023-06-29T10:06Z hipsgen_params_2 = out=/var/www/HST-hips/filter_wideUV_hips CHECKCODE hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_wideUV_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_wideUV_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_wideUV_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 41 moc_time_range = 4869 moc_order = 13 obs_initial_ra = 169.56126 obs_initial_dec = 7.77683 obs_initial_fov = 0.007157263357952928 TIMESTAMP = 1721288456534 ID = CDS/P/HST/wideV creator_did = ivo://CDS/P/HST/wideV data_pixel_bitpix = -32 dataproduct_type = image em_max = 9.96e-07 em_min = 4.70e-07 hips_builder = Aladin/HipsGen v12.044 hips_check_code = png:929198719 fits:2406550959 hips_copyright = CNRS/Unistra hips_creation_date = 2019-03-01T21:28Z hips_creator = Durand D. (CDS) hips_data_range = -123.6 369.6 hips_estsize = 1112344200 hips_frame = equatorial hipsgen_date = 2023-04-19T19:18Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=wideV -in=/data-test-iscsi/d.durand/2023A/HST/wideV.extract -id=CDS/P/HST/wideV -blank=0 -order=13 -mocOrder=16 -out=/data-test-iscsi/d.durand/2023A/HST/wideV.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" -d hips_initial_dec = -53.66632 hips_initial_fov = 0.04826 hips_initial_ra = 265.14828 hips_nb_tiles = 2006878 hips_order = 13 hips_order_min = 0 hips_overlay = overlayMean mergeOverwriteTile treeMean hips_pixel_bitpix = -32 hips_pixel_cut = 0.02362 240 hips_pixel_scale = 1.397E-5 hips_release_date = 2023-04-20T20:25Z hips_sampling = bilinear hips_status = public master clonableOnce hips_tile_format = png fits hips_tile_width = 512 hips_version = 1.4 obs_ack = All publications based on HST data should carry the following footnote: "Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. " obs_collection = HST-wideV obs_description = The HST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all HST observations done in F606W and F600LP filters between the beginning of the mission to early 2023.\nThe Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautics and Space Administration (NASA) to operate a space-based observatory for the benefit of the international astronomical community.In this new release we tried to correct the astrometry of individual images before building the HIPS images using CASU tools thanks to Jim Lewis. obs_regime = Optical client_category = Image/Optical/HST obs_title = HST-wideV includes the following filters: F606W and F600LP prov_progenitor = CDS (Daniel Durand) s_pixel_scale = 1.100E-5 t_max = 59994.9786560532 t_min = 49351.005756794 hips_service_url = https://alasky.cds.unistra.fr/HST-hips/filter_wideV_hips hips_progenitor_url = https://alasky.cds.unistra.fr/HST-hips/filter_wideV_hips/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/HST-hips/filter_wideV_hips hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_sky_fraction = 6.142E-4 moc_order = 15 obs_initial_ra = 265.14828 obs_initial_dec = -53.66632 obs_initial_fov = 0.001789315839488232 TIMESTAMP = 1721288456594 ID = CDS/P/Haslam408 creator_did = ivo://CDS/P/Haslam408 obs_collection = Haslam 408MHz obs_title = Haslam 408MHz obs_description = The survey data were obtained from the archives of the NCSA ADIL in equatorial 1950 coordinates, and subsequently processed further in the Fourier domain to mitigate baseline striping and strong point sources. The data were then interpolated onto a Galactic coordinate system and HEALPix projection. This file is distributed and maintained by LAMBDA obs_copyright = LAMBDA/NASA client_category = Image/Radio client_sort_key = 05-08 hips_release_date = 2019-05-05T06:35Z hips_creator = Fernique P. (CDS) hips_version = 1.4 hips_order = 3 hips_tile_format = jpeg fits dataproduct_type = image hips_status = public master clonableOnce obs_ack = see Haslam et al. (1982) prov_progenitor = LAMBDA/NASA bib_reference = 1982A&AS...47....1H bib_reference_url = http://adsabs.harvard.edu/cgi-bin/bib_query?1982A&AS...47....1H obs_copyright_url = http://skyview.gsfc.nasa.gov/current/cgi/survey.pl t_min = 39065 t_max = 44117 em_min = 0.731647243441123 em_max = 0.737950665846154 hips_builder = Aladin/HipsGen v10.123 hips_frame = galactic hips_tile_width = 64 hips_pixel_bitpix = -32 hips_sampling = none hips_skyval = none hips_overlay = none hips_hierarchy = mean hips_pixel_scale = 0.01431 moc_sky_fraction = 1 hips_estsize = 1112337 hips_copyright = CNRS/Unistra obs_regime = Radio hips_creation_date = 2015-04-10T13:58Z hips_initial_fov = 100.0 hips_initial_ra = 266.4150089 hips_initial_dec = -29.0061110 hips_order_min = 0 hipsgen_date = 2019-05-05T06:35Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/Haslam408 UPDATE hips_service_url = https://alasky.cds.unistra.fr/Haslam408 hips_service_url_1 = https://alaskybis.cds.unistra.fr/Haslam408 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 8 obs_initial_ra = 266.4150089 obs_initial_dec = -29.0061110 obs_initial_fov = 0.2290324274544937 TIMESTAMP = 1721288416930 ID = CDS/P/Haslam408/v2 creator_did = ivo://CDS/P/Haslam408/v2 obs_collection = Haslam 408Mhz reprocessed obs_title = Haslam 408Mhz reprocessed obs_description = Remazeilles et al. 2014 have re-evaluated and re-processed the rawest Haslam 408 MHz data, available from the Max Planck Institute for Radioastronomy Survey Sampler website, to produce an improved source-subtracted and destriped 408 MHz all-sky map. Large-scale striations associated with correlated low-frequency noise in the scan direction are reduced using a Fourier-based filtering technique. The most important improvement results from the removal of extra-galactic sources. An iterative combination of two techniques - two-dimensional Gaussian fitting and minimum curvature spline surface inpainting - are used to remove the brightest sources (with flux density larger than 2 Jy).Desources destrier map. obs_copyright_url = http://lambda.gsfc.nasa.gov/product/foreground/2014_haslam_408_info.cfm obs_ack = see Remazeilles et al. (2014) prov_progenitor = LAMBDA/NASA client_category = Image/Radio client_sort_key = 05-08a hips_release_date = 2019-05-05T06:35Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Fernique P. (CDS) hips_version = 1.4 hips_order = 3 hips_frame = galactic hips_tile_format = png jpeg fits dataproduct_type = image hips_pixel_cut = 13.66 298.4 hips_data_range = -2440 7363 moc_access_url = http://alasky.u-strasbg.fr/Haslam408_2014/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra bib_reference = 2015MNRAS.451.4311R bib_reference_url = http://adsabs.harvard.edu/abs/2015MNRAS.451.4311R obs_copyright = LAMBDA/NASA t_min = 39065 t_max = 44117 obs_regime = Radio em_min = 0.731647243441123 em_max = 0.737950665846154 hips_creation_date = 2014-11-25T15:40Z hips_tile_width = 256 hips_pixel_scale = 0.01431 hips_initial_fov = 100.0 hips_initial_ra = 266.4150089 hips_initial_dec = -29.0061110 hips_order_min = 0 hips_pixel_bitpix = 32 moc_sky_fraction = 1 hips_estsize = 1126099 hipsgen_date = 2019-05-05T06:35Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/Haslam408_2014 UPDATE hips_service_url = https://alasky.cds.unistra.fr/Haslam408_2014 hips_service_url_1 = https://alaskybis.cds.unistra.fr/Haslam408_2014 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 8 obs_initial_ra = 266.4150089 obs_initial_dec = -29.0061110 obs_initial_fov = 0.2290324274544937 TIMESTAMP = 1721288416710 ID = CDS/P/INTGAL/35 creator_did = ivo://CDS/P/INTGAL/35 obs_collection = INTGAL 35 obs_title = Nine Year INTEGRAL IBIS 17-35 keV Galactic Plane obs_description = This survey combines 9 years of INTEGRAL IBIS observations from December 2002 through January 2011 into a single Galactic Plane image. A total of 135 megaseconds of exposure is included in the observations used. Survey data is generated for the Galactic plane in the region |b| <= 17.5. The original flux data has been convolved with 5' seeing kernel. To minimize loss of resolution in transformations, the Lanczos sampler is suggested as the default, but may be overriden by the user. The exposure and sensitivity vary considerably over the coverage region, but 90% of the field has a limiting sensitivity better than 2.2 x 10-11ergs s-1cm-2 or about 1.56 mCrab. Further details of the survey construction are given in the reference. The flux map use the PSF convolved maps from the survey. The flux maps are in millicrab units. See Krivonos, R. et al. in 2012 A&A (2012A&A...545A..27K). obs_ack = Based on observations with INTEGRAL, an ESA project with instruments and science data centre funded by ESA member states (especially the PI countries: Denmark, France, Germany, Italy, Switzerland and Spain), Poland, and participation of Russia and the USA. Obtained through SkyView NASA/HEASARC. HiPSized by CDS. obs_copyright = HiPSized & color composition by CDS client_category = Image/X/INTEGRAL/INTGAL client_sort_key = 01-03-01-01 hips_release_date = 2019-05-05T06:36Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Fernique P. (CDS) hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_format = png fits dataproduct_type = image hips_pixel_cut = -0.3 5 hips_data_range = -110.6 327 moc_access_url = http://alasky.u-strasbg.fr/INTGAL/INTGAL35/Moc.fits hips_progenitor_url = https://alasky.cds.unistra.fr/INTGAL/INTGAL35/HpxFinder hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = Space Research Institute (IKI) bib_reference = 2012A&A...545A..27K bib_reference_url = http://adsabs.harvard.edu/cgi-bin/nph-bib_query?db_key=AST&bibcode=2012A&A...545A..27K obs_copyright_url = http://hea.iki.rssi.ru/integral/nine-years-galactic-survey/index.php t_min = 52609 t_max = 55562 obs_regime = X-ray em_min = 3.5424e-11 em_max = 7.2932e-11 hips_tile_width = 512 hips_pixel_scale = 0.01431 hips_initial_fov = 120.0 hips_initial_ra = 266.4049948 hips_initial_dec = -28.9361739 hips_creation_date = 2015-01-12T17:23Z hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 0.3108 hips_estsize = 427577 hipsgen_date = 2019-05-05T06:36Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/INTGAL/INTGAL35 UPDATE hips_service_url = https://alasky.cds.unistra.fr/INTGAL/INTGAL35 hips_service_url_1 = https://alaskybis.cds.unistra.fr/INTGAL/INTGAL35 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 8 obs_initial_ra = 266.4049948 obs_initial_dec = -28.9361739 obs_initial_fov = 0.2290324274544937 TIMESTAMP = 1721288417010 ID = CDS/P/INTGAL/60 creator_did = ivo://CDS/P/INTGAL/60 obs_collection = INTGAL 60 obs_title = Nine Year INTEGRAL IBIS 17-60 keV Galactic Plane obs_description = This survey combines 9 years of INTEGRAL IBIS observations from December 2002 through January 2011 into a single Galactic Plane image. A total of 135 megaseconds of exposure is included in the observations used. Survey data is generated for the Galactic plane in the region |b| <= 17.5. The original flux data has been convolved with 5' seeing kernel. To minimize loss of resolution in transformations, the Lanczos sampler is suggested as the default, but may be overriden by the user. The exposure and sensitivity vary considerably over the coverage region, but 90% of the field has a limiting sensitivity better than 2.2 x 10-11ergs s-1cm-2 or about 1.56 mCrab. Further details of the survey construction are given in the reference. The flux map use the PSF convolved maps from the survey. The flux maps are in millicrab units. See Krivonos, R. et al. in 2012 A&A (2012A&A...545A..27K). obs_ack = Based on observations with INTEGRAL, an ESA project with instruments and science data centre funded by ESA member states (especially the PI countries: Denmark, France, Germany, Italy, Switzerland and Spain), Poland, and participation of Russia and the USA. Obtained through SkyView NASA/HEASARC. HiPSized by CDS. obs_copyright = Space Research Institute (IKI), Moscow, Russia obs_copyright_url = http://hea.iki.rssi.ru/integral/nine-years-galactic-survey/index.php client_category = Image/X/INTEGRAL/INTGAL client_sort_key = 01-03-01-02 hips_release_date = 2019-05-05T06:36Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Fernique P. (CDS) hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_format = png fits dataproduct_type = image hips_pixel_cut = -0.3 5 hips_data_range = -82.77 243.5 moc_access_url = http://alasky.u-strasbg.fr/INTGAL/INTGAL60/Moc.fits hips_progenitor_url = https://alasky.cds.unistra.fr/INTGAL/INTGAL60/HpxFinder hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = Space Research Institute (IKI) bib_reference = 2012A&A...545A..27K bib_reference_url = http://adsabs.harvard.edu/cgi-bin/nph-bib_query?db_key=AST&bibcode=2012A&A...545A..27K t_min = 52609 t_max = 55562 obs_regime = X-ray em_min = 2.0664e-11 em_max = 7.2932e-11 hips_tile_width = 512 hips_pixel_scale = 0.01431 hips_initial_fov = 120.0 hips_initial_ra = 266.4049948 hips_initial_dec = -28.9361739 hips_creation_date = 2015-01-12T17:28Z hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 0.3108 hips_estsize = 427577 hipsgen_date = 2019-05-05T06:36Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/INTGAL/INTGAL60 UPDATE hips_service_url = https://alasky.cds.unistra.fr/INTGAL/INTGAL60 hips_service_url_1 = https://alaskybis.cds.unistra.fr/INTGAL/INTGAL60 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 8 obs_initial_ra = 266.4049948 obs_initial_dec = -28.9361739 obs_initial_fov = 0.2290324274544937 TIMESTAMP = 1721288417090 ID = CDS/P/INTGAL/80 creator_did = ivo://CDS/P/INTGAL/80 obs_collection = INTGAL 80 obs_title = Nine Year INTEGRAL IBIS 35-80 keV Galactic Plane obs_description = This survey combines 9 years of INTEGRAL IBIS observations from December 2002 through January 2011 into a single Galactic Plane image. A total of 135 megaseconds of exposure is included in the observations used. Survey data is generated for the Galactic plane in the region |b| <= 17.5. The original flux data has been convolved with 5' seeing kernel. To minimize loss of resolution in transformations, the Lanczos sampler is suggested as the default, but may be overriden by the user. The exposure and sensitivity vary considerably over the coverage region, but 90% of the field has a limiting sensitivity better than 2.2 x 10-11ergs s-1cm-2 or about 1.56 mCrab. Further details of the survey construction are given in the reference. The flux map use the PSF convolved maps from the survey. The flux maps are in millicrab units. See Krivonos, R. et al. in 2012 A&A (2012A&A...545A..27K). obs_ack = Based on observations with INTEGRAL, an ESA project with instruments and science data centre funded by ESA member states (especially the PI countries: Denmark, France, Germany, Italy, Switzerland and Spain), Poland, and participation of Russia and the USA. Obtained through SkyView NASA/HEASARC. HiPSized by CDS. obs_copyright = Space Research Institute (IKI), Moscow, Russia obs_copyright_url = http://hea.iki.rssi.ru/integral/nine-years-galactic-survey/index.php client_category = Image/X/INTEGRAL/INTGAL client_sort_key = 01-03-01-03 hips_release_date = 2019-05-05T06:36Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Fernique P. (CDS) hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_format = png fits dataproduct_type = image hips_pixel_cut = -0.3 5 hips_data_range = -40.75 114.9 moc_access_url = http://alasky.u-strasbg.fr/INTGAL/INTGAL80/Moc.fits hips_progenitor_url = https://alasky.cds.unistra.fr/INTGAL/INTGAL80/HpxFinder hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = Space Research Institute (IKI) bib_reference = 2012A&A...545A..27K bib_reference_url = http://adsabs.harvard.edu/cgi-bin/nph-bib_query?db_key=AST&bibcode=2012A&A...545A..27K t_min = 52609 t_max = 55562 obs_regime = X-ray em_min = 1.5498e-11 em_max = 3.5428e-11 hips_tile_width = 512 hips_pixel_scale = 0.01431 hips_initial_fov = 120.0 hips_initial_ra = 266.4049948 hips_initial_dec = -28.9361739 hips_creation_date = 2015-01-12T17:28Z hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 0.3108 hips_estsize = 427577 hipsgen_date = 2019-05-05T06:36Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/INTGAL/INTGAL80 UPDATE hips_service_url = https://alasky.cds.unistra.fr/INTGAL/INTGAL80 hips_service_url_1 = https://alaskybis.cds.unistra.fr/INTGAL/INTGAL80 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 8 obs_initial_ra = 266.4049948 obs_initial_dec = -28.9361739 obs_initial_fov = 0.2290324274544937 TIMESTAMP = 1721288417146 ID = CDS/P/INTGAL/Color creator_did = ivo://CDS/P/INTGAL/Color obs_collection = INTGAL Color obs_title = Nine Year INTEGRAL IBIS Galactic Plane Color Composition (35-60-80KeV) obs_description = This survey combines the 3 bands of the 9 years of INTEGRAL IBIS surveys described in Krivonos, R. et al. in 2012 A&A (2012A&A...545A..27K). obs_ack = Based on observations with INTEGRAL, an ESA project with instruments and science data centre funded by ESA member states (especially the PI countries: Denmark, France, Germany, Italy, Switzerland and Spain), Poland, and participation of Russia and the USA. Obtained through SkyView NASA/HEASARC. HiPSized by CDS. obs_copyright = Space Research Institute (IKI), Moscow, Russia obs_copyright_url = http://hea.iki.rssi.ru/integral/nine-years-galactic-survey/index.php client_category = Image/X/INTEGRAL/INTGAL client_sort_key = 01-03-01-00 hips_release_date = 2019-05-05T06:37Z hips_builder = Aladin/HipsGen v10.123 hips_creator = CDS hips_version = 1.4 hips_order = 3 hips_frame = equatorial hips_tile_format = png jpeg dataproduct_type = image hips_rgb_red = INTGAL35 [0.0 2.5 5.0 Log] hips_rgb_green = INTGAL60 [0.0 2.5 5.0 Log] hips_rgb_blue = INTGAL80 [0.0 2.5 5.0 Log] moc_access_url = http://alasky.u-strasbg.fr/INTGAL/INTColor/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = Space Research Institute (IKI) bib_reference = 2012A&A...545A..27K bib_reference_url = http://adsabs.harvard.edu/cgi-bin/nph-bib_query?db_key=AST&bibcode=2012A&A...545A..27K t_min = 52609 t_max = 55562 obs_regime = X-ray em_min = 1.5498e-11 em_max = 7.2932e-11 hips_tile_width = 512 hips_pixel_scale = 0.01431 hips_initial_fov = 120.0 hips_initial_ra = 266.4049948 hips_initial_dec = -28.9361739 hips_creation_date = 2015-01-12T17:48Z hips_order_min = 0 dataproduct_subtype = color moc_sky_fraction = 0.3828 hips_estsize = 22944 hipsgen_date = 2019-05-05T06:37Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/INTGAL/INTColor UPDATE hips_service_url = https://alasky.cds.unistra.fr/INTGAL/INTColor hips_service_url_1 = https://alaskybis.cds.unistra.fr/INTGAL/INTColor hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 3 obs_initial_ra = 266.4049948 obs_initial_dec = -28.9361739 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288417206 ID = CDS/P/IPHAS/DR2/halpha creator_did = ivo://CDS/P/IPHAS/DR2/halpha obs_title = IPHAS DR2 halpha obs_collection = IPHAS DR2 halpha obs_description = The INT/WFC Photometric H-Alpha Survey of the Northern Galactic Plane (IPHAS) is a 1860 square deg imaging survey of the Northern Milky Way at red visible wavelengths. It covers Galactic latitudes |b| < 5deg and longitudes l = 30-215deg in the broad-band r, i and narrow-band Halpha filters. hips_initial_fov = 0.37843 hips_initial_ra = 298.07095 hips_initial_dec = +32.76356 hips_pixel_bitpix = 16 data_pixel_bitpix = 16 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = median hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra obs_ack = It makes use of data obtained as part of the INT Photometric Halpha Survey of the Northern Galactic Plane (IPHAS, www.iphas.org) carried out at the Isaac Newton Telescope (INT). The INT is operated on the island of La Palma by the Isaac Newton Group in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. All IPHAS data are processed by the Cambridge Astronomical Survey Unit, at the Institute of Astronomy in Cambridge. The bandmerged DR2 catalogue was assembled at the Centre for Astrophysics Research, University of Hertfordshire, supported by STFC grant ST/J001333/1. prov_progenitor = IPHAS bib_reference = 2014MNRAS.444.3230B bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2014MNRAS.444.3230B t_min = 52821 t_max = 56079 obs_regime = Optical em_min = 6.494e-7 em_max = 6.642e-7 client_category = Image/Optical/IPHAS hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T09:03Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = 21 497 hips_data_range = -1009 80009 hips_pixel_scale = 5.591E-5 s_pixel_scale = 9.238E-5 dataproduct_type = image moc_sky_fraction = 0.04503 hips_estsize = 1691136587 hipsgen_date = 2019-03-15T13:14Z hipsgen_params = in=halpha_DR2 out=hips/ creator_did=CDS/P/IPHAS/DR2/halpha maxThread=50 "hips_pixel_cut=21 497" mocorder=11 INDEX TILES PNG DETAILS hips_creation_date = 2019-03-15T13:14Z hipsgen_date_1 = 2019-03-16T10:14Z hipsgen_params_1 = in=halpha_DR2 out=hips/ creator_did=CDS/P/IPHAS/DR2/halpha maxThread=50 "hips_pixel_cut=21 497" mocorder=11 INDEX TILES PNG DETAILS hipsgen_date_2 = 2019-05-21T09:03Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/IPHAS/DR2/halpha UPDATE hips_service_url = https://alasky.cds.unistra.fr/IPHAS/DR2/halpha hips_progenitor_url = https://alasky.cds.unistra.fr/IPHAS/DR2/halpha/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/IPHAS/DR2/halpha hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 21 moc_time_range = 131 moc_order = 10 obs_initial_ra = 298.07095 obs_initial_dec = +32.76356 obs_initial_fov = 0.057258106863623426 TIMESTAMP = 1721288484318 ID = CDS/P/IPHAS/DR2/i hips_initial_fov = 0.37871 hips_initial_ra = 25.136 hips_initial_dec = +65.21698 creator_did = ivo://CDS/P/IPHAS/DR2/i obs_title = IPHAS DR2 i obs_collection = IPHAS DR2 i obs_description = The INT/WFC Photometric H-Alpha Survey of the Northen Galactic Plane (IPHAS) is a 1860 square deg imaging survey of the Northen Milky Way at red visible wavelenghts. It covers Galactic latitude |b| <5 deg and logitudes l = 30-215 deg in the broad-band r, i, and narrow-bnad Halpha filters. hips_pixel_bitpix = 16 data_pixel_bitpix = 16 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = median hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra obs_ack = It makes use of data obtained as part of the INT Photometric Halpha Survey of the Northern Galactic Plane (IPHAS, www.iphas.org) carried outt prov_progenitor = IPHAS bib_reference = 2014MNRAS.444.3230B bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2014MNRAS.444.3230B t_min = 52821 t_max = 56079 obs_regime = Optical em_min = 6.689e-7 em_max = 8.389e-7 client_category = Image/Optical/IPHAS hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T09:03Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = 56 849 hips_data_range = -1009 58778 hips_pixel_scale = 5.591E-5 s_pixel_scale = 9.245E-5 dataproduct_type = image moc_sky_fraction = 0.04448 hips_estsize = 1691348110 hipsgen_date = 2019-03-12T11:33Z hipsgen_params = in=i_true/ out=/data4/buga/IPHAS/hips_i/ creator_did=CDS/P/IPHAS/DR2/i maxThread=50 mocorder=11 "hips_pixel_cut=56 849" INDEX TILES PNG DETAILS hips_creation_date = 2019-03-12T11:33Z hipsgen_date_1 = 2019-03-13T07:19Z hipsgen_params_1 = in=i_true/ out=/data4/buga/IPHAS/hips_i/ creator_did=CDS/P/IPHAS/DR2/i maxThread=50 mocorder=11 "hips_pixel_cut=56 849" INDEX TILES PNG DETAILS hipsgen_date_2 = 2019-05-21T09:03Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/IPHAS/DR2/i/CDS_P_IPHAS_DR2_i UPDATE hips_service_url = https://alasky.cds.unistra.fr/IPHAS/DR2/i/CDS_P_IPHAS_DR2_i hips_progenitor_url = https://alasky.cds.unistra.fr/IPHAS/DR2/i/CDS_P_IPHAS_DR2_i/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/IPHAS/DR2/i/CDS_P_IPHAS_DR2_i hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 23 moc_time_range = 219 moc_order = 11 obs_initial_ra = 25.136 obs_initial_dec = +65.21698 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288484262 ID = CDS/P/IPHAS/DR2/r creator_did = ivo://CDS/P/IPHAS/DR2/r obs_title = IPHAS DR2 r obs_collection = IPHAS DR2 r obs_description = The INT/WFC Photometric H-Alpha Survey of the Northern Galactic Plane (IPHAS) is a 1860 square deg imaging survey of the Northern Milky Way at red visible wavelengths. It covers Galactic latitudes |b| < 5deg and longitudes l = 30-215deg in the broad-band r, i and narrow-band Halpha filters. hips_initial_fov = 0.37875 hips_initial_ra = 102.24486 hips_initial_dec = +8.3823 hips_pixel_bitpix = 16 data_pixel_bitpix = 16 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = median hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra obs_ack = It makes use of data obtained as part of the INT Photometric Halpha Survey of the Northern Galactic Plane (IPHAS, www.iphas.org) carried out at the Isaac Newton Telescope (INT). The INT is operated on the island of La Palma by the Isaac Newton Group in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. All IPHAS data are processed by the Cambridge Astronomical Survey Unit, at the Institute of Astronomy in Cambridge. The bandmerged DR2 catalogue was assembled at the Centre for Astrophysics Research, University of Hertfordshire, supported by STFC grant ST/J001333/1. prov_progenitor = IPHAS bib_reference = 2014MNRAS.444.3230B bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2014MNRAS.444.3230B t_min = 52821 t_max = 56079 obs_regime = Optical em_min = 5.5e-7 em_max = 6.98e-7 client_category = Image/Optical/IPHAS hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T09:02Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = 60 1900 hips_data_range = 1 65535 hips_pixel_scale = 5.591E-5 s_pixel_scale = 9.246E-5 dataproduct_type = image moc_sky_fraction = 0.04504 hips_estsize = 1691331491 hipsgen_date = 2019-03-17T15:25Z hipsgen_params = in=r_true/ out=/data4/buga/IPHAS/r/ creator_did=CDS/P/IPHAS/DR2/r maxThread=50 mocorder=11 "hips_pixel_cut=60 1900" INDEX TILES PNG DETAILS hips_creation_date = 2019-03-17T15:25Z hipsgen_date_1 = 2019-03-18T10:59Z hipsgen_params_1 = in=r_true/ out=/data4/buga/IPHAS/r/ creator_did=CDS/P/IPHAS/DR2/r maxThread=50 mocorder=11 "hips_pixel_cut=60 1900" INDEX TILES PNG DETAILS hipsgen_date_2 = 2019-05-21T09:02Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/IPHAS/DR2/r/CDS_P_IPHAS_DR2_r UPDATE hips_service_url = https://alasky.cds.unistra.fr/IPHAS/DR2/r/CDS_P_IPHAS_DR2_r hips_progenitor_url = https://alasky.cds.unistra.fr/IPHAS/DR2/r/CDS_P_IPHAS_DR2_r/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/IPHAS/DR2/r/CDS_P_IPHAS_DR2_r hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 23 moc_time_range = 241 moc_order = 10 obs_initial_ra = 102.24486 obs_initial_dec = +8.3823 obs_initial_fov = 0.057258106863623426 TIMESTAMP = 1721288484198 ID = CDS/P/IRIS/color creator_did = ivo://CDS/P/IRIS/color obs_collection = IRIS color obs_title = IRAS-IRIS HEALPix survey, color obs_description = The Infrared Astronomical Satellite (IRAS) had a tremendous impact on many areas of modern astrophysics. In particular it revealed the ubiquity of infrared cirrus that are a spectacular manifestation of the interstellar medium complexity but also an important foreground for observational cosmology. With the forthcoming Planck satellite there is a need for all-sky complementary data sets with arcminute resolution that can bring informations on specific foreground emissions that contaminate the Cosmic Microwave Background radiation. With its ~4' resolution matching perfectly the high-frequency bands of Planck, IRAS is a natural data set to study the variations of dust properties at all scales. But the latest version of the images delivered by the IRAS team (the ISSA plates) suffers from calibration, zero level and striping problems that can preclude its use, especially at 12 and 25 micron. In this paper we present how we proceeded to solve each of these problems and enhance significantly the general quality of the ISSA plates in the four bands (12, 25, 60 and 100 microns). This new generation of IRAS images, called IRIS, benefits from a better zodiacal light subtraction, from a calibration and zero level compatible with DIRBE, and from a better destriping. At 100 micron the IRIS product is also a significant improvement from the Schlegel et al. (1998) maps. IRIS keeps the full ISSA resolution, it includes well calibrated point sources and the diffuse emission calibration at scales smaller than 1 degree was corrected for the variation of the IRAS detector responsivity with scale and brightness. The uncertainty on the IRIS calibration and zero level are dominated by the uncertainty on the DIRBE calibration and on the accuracy of the zodiacal light model. The color HiPS has been created from individual bands 100 (red channel), 60 (green channel) and 25 (blue channel) microns. obs_copyright = Healpixed by CDS client_category = Image/Infrared/IRIS client_sort_key = 04-02-01 hips_release_date = 2019-05-05T06:37Z hips_creator = CDS hips_version = 1.4 hips_order = 3 hips_frame = galactic hips_tile_format = jpeg dataproduct_type = image client_application = AladinLite client_application = AladinDesktop moc_access_url = http://alasky.u-strasbg.fr/IRISColor/Moc.fits hips_status = public master clonableOnce hips_copyright = CNRS/Unistra obs_ack = This research has made use of the NASA/ IPAC Infrared Science Archive, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. prov_progenitor = IPAC/NASA bib_reference = 2005ApJS..157..302M bib_reference_url = https://ui.adsabs.harvard.edu/?#abs/2005ApJS..157..302M obs_copyright_url = http://irsa.ipac.caltech.edu/data/IRIS/ t_min = 45335 t_max = 45639 obs_regime = Infrared em_min = 0.000012 em_max = 0.0001 hips_builder = Aladin/HipsGen v10.123 hips_tile_width = 256 hips_pixel_scale = 0.01431 hips_initial_fov = 100.0 hips_initial_ra = 82.5185467 hips_initial_dec = +25.8941503 hips_creation_date = 2010-06-09T06:33Z hips_order_min = 0 dataproduct_subtype = color moc_sky_fraction = 1 hips_estsize = 9182 hipsgen_date = 2019-05-05T06:37Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/IRISColor UPDATE hips_service_url = https://alasky.cds.unistra.fr/IRISColor hips_service_url_1 = https://alaskybis.cds.unistra.fr/IRISColor hips_status_1 = public mirror clonableOnce hips_service_url_2 = https://irsa.ipac.caltech.edu/data/hips/CDS/IRIS/color hips_status_2 = public mirror unclonable hips_service_url_3 = https://healpix.ias.u-psud.fr/CDS_P_IRIS_color hips_status_3 = public mirror unclonable hips_service_url_4 = http://skies.esac.esa.int/IRISColor hips_status_4 = public mirror unclonable moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 8 obs_initial_ra = 82.5185467 obs_initial_dec = +25.8941503 obs_initial_fov = 0.2290324274544937 TIMESTAMP = 1729584625541 ID = CDS/P/ISOPHOT/170 creator_did = ivo://CDS/P/ISOPHOT/170 obs_collection = ISOPHOT 170 um obs_title = The ISOPHOT 170um Serendipity Survey obs_description = The 170 micron far-infrared slew data of the ISOPHOT Serendipity Survey (ISOSS) has been assembled to a sky atlas with about 15% sky coverage. The redundant information of the brightnesss at slew crossings has been used to globally rescale and homogenize the slew brightnesses, leading to significantly increased photometric accuracy and reproducibility as well as the homogeneity of the maps. The corrected slew data were remapped with a constant grid size of 22.4arcsec onto 124 maps in galactic coordinates - (Stickel et al., 2007) obs_ack = Manfred Stickel, stickel(at)mpia-hd.mpg.de obs_copyright = Stickel et al., 2007 - HiPSed by CDS obs_copyright_url = http://cdsarc.u-strasbg.fr/viz-bin/Cat?J/A%2bA/466/1205 client_category = Image/Infrared/ISO client_sort_key = 04-xx hips_release_date = 2019-05-05T06:38Z hips_builder = Aladin/HipsGen v10.123 hips_creator = Fernique P. (CDS) hips_version = 1.4 hips_order = 5 hips_frame = equatorial hips_tile_width = 512 hips_tile_format = png fits dataproduct_type = image hips_pixel_cut = 0 200 hips_data_range = -435.6 1307 hips_initial_ra = 271.92853 hips_initial_dec = 344.6104410 hips_initial_fov = 61.6115552 moc_access_url = http://alasky.u-strasbg.fr/ISO/ISOPHOT/Moc.fits hips_progenitor_url = https://alasky.cds.unistra.fr/ISO/ISOPHOT/HpxFinder hips_status = public master clonableOnce hips_copyright = CNRS/Unistra prov_progenitor = Stickel et al., 2007 bib_reference = 2007A&A...466.1205S bib_reference_url = http://cdsbib.u-strasbg.fr/cgi-bin/cdsbib?2007A%26A...466.1205S t_min = 50038 t_max = 50814 obs_regime = Infrared em_min = 0.00017 em_max = 0.00017 hips_pixel_scale = 0.003579 hips_creation_date = 2014-12-05T13:45Z hips_order_min = 0 hips_pixel_bitpix = -32 moc_sky_fraction = 0.4111 hips_estsize = 17870688 hipsgen_date = 2019-05-05T06:38Z hipsgen_params = out=/asd-volumes/sc1-asd-volume10/ISO/ISOPHOT UPDATE hips_service_url = https://alasky.cds.unistra.fr/ISO/ISOPHOT hips_service_url_1 = https://alaskybis.cds.unistra.fr/ISO/ISOPHOT hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 9 obs_initial_ra = 271.92853 obs_initial_dec = 344.6104410 obs_initial_fov = 0.11451621372724685 TIMESTAMP = 1721288417342 ID = CDS/P/Iapetus/Cassini-PIA18436 client_category = Solar system/Saturn/Iapetus hips_initial_fov = 180 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/Iapetus/Cassini-PIA18436 hips_overlay = mean hips_hierarchy = median hips_creator = Fernique P. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = Iapetus Cassini PIA18436 obs_description = This set of global, color mosaics of Saturn's moon Iapetus was produced from images taken by NASA's Cassini spacecraft during its first ten years exploring the Saturn system. These are the first global color maps of these moons produced from the Cassini data. The colors shown in these global mosaics are enhanced, or broader, relative to human vision, extending into the ultraviolet and infrared range. Resolution on Iapetus in the maps is 400 meters per pixel. Image selection, radiometric calibration, geographic registration and photometric correction, as well as mosaic selection and assembly were performed by Paul Schenk at the Lunar and Planetary Institute. Original image planning and targeting for Saturn's icy moons were performed by Tilman Denk (Frei Universitat, Berlin) and Paul Helfenstein (Cornell University, Ithaca, New York). The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo. obs_ack = NASA/JPL-Caltech/Space Science Institute/Lunar and Planetary Institute prov_progenitor = JPL/PhotoJournal prov_progenitor_url = https://photojournal.jpl.nasa.gov/catalog/PIA18436 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T07:07Z hips_frame = iapetus hips_body = iapetus hips_order = 3 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg hips_pixel_scale = 0.01431 s_pixel_scale = 0.03066 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 18357 hipsgen_date = 2018-01-24T14:14Z hipsgen_params = "hhh=Iapetus/Iapetus.jpg 11741x5871" partitioning=5871 -maxthread=10 in=Iapetus creator_did=CDS/P/Iapetus/Cassini-PIA18436 -f color=jpg INDEX TILES hips_creation_date = 2018-01-24T14:14Z hips_order_min = 0 dataproduct_subtype = color hipsgen_date_1 = 2019-05-21T07:07Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume6/Planets/CDS_P_Iapetus_Cassini-PIA18436 UPDATE hips_service_url = https://alasky.cds.unistra.fr/Planets/CDS_P_Iapetus_Cassini-PIA18436 hips_service_url_1 = https://alaskybis.cds.unistra.fr/Planets/CDS_P_Iapetus_Cassini-PIA18436 hips_status_1 = public mirror clonableOnce client_application = AladinDesktopBeta>=10.040 AladinDesktop>=11.125 moc_type = smoc moc_order = 3 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288467746 ID = CDS/P/Io/Galileo-SSI-1km client_category = Solar system/Jupiter/Io hips_initial_fov = 180 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/Io/Galileo-SSI-1km hips_overlay = mean hips_hierarchy = median hips_creator = Fernique P. (CDS) hips_copyright = Universite de Strasbourg/CNRS obs_title = Io Galileo-SSI-1km obs_description = This basemap of Jupiter's moon Io was produced by combining the best images from both the Voyager 1 and Galileo Missions. Although the subjovian hemisphere of Io was poorly seen by Galileo, superbly detailed Voyager 1 images cover longitudes from 240deg W to 40deg W and the nearby southern latitudes. A monochrome mosaic of the highest resolution images from both Galileo and Voyager 1 was assembled that includes 29 Voyager 1 images with spatial resolutions sometimes exceeding the 1 km/pixel scale of the final mosaic. Because this mosaic is made up of images taken at various local times of day, care must be taken to note the solar illumination direction when deciding whether topographic features display positive or negative relief. In general, the illumination is from the west over longitudes 40 deg to 270 deg W, and from the east over longitudes 270 deg W to 40 deg W. Color information was later superimposed from Galileo low phase angle violet, green, and near-infrared (756 nanometer wavelength) images. The Galileo Solid-State Imaging (SSI) camera's silicon charge-coupled device (CCD) was sensitive to longer wavelengths than the vidicon cameras of Voyager, so that distinctions between red and yellow hues can be more easily discerned. The "true" colors that would be visible to the eye are similar but much more muted than shown here. Image resolutions range from 1 to 10 km/pixel along the equator, with the poorest coverage centered on longitude 50 W prov_progenitor = Planetary Data System, from USGS Astrogeology Science Center prov_progenitor_url = https://astrogeology.usgs.gov/search/map/Io/Voyager-Galileo/Io_Galileo_SSI_Global_Mosaic_FalseColor_1km bib_reference = doi:10.1007/BF00216864, doi:10.1016/j.icarus.2011.05.007 obs_copyright = Public domain hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T06:59Z hips_frame = io hips_body = io hips_order = 3 hips_tile_width = 512 hips_status = public master clonableOnce hips_pixel_scale = 0.01431 s_pixel_scale = 0.03145 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 18357 hipsgen_date = 2018-01-14T18:33Z hipsgen_params = "in=D:\\Planet\\IoPIA09257" "out=D:\\Planet\\IoPIA09257HiPS" color=true creator_did=CDS/P/Io/Galileo-SSI-1km -f INDEX TILES hips_tile_format = jpeg hips_creation_date = 2018-01-14T18:34Z hips_order_min = 0 dataproduct_subtype = color hipsgen_date_1 = 2019-05-21T06:59Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume6/Planets/CDS_P_Io_Galileo-SSI-1km UPDATE hips_service_url = https://alasky.cds.unistra.fr/Planets/CDS_P_Io_Galileo-SSI-1km hips_service_url_1 = https://alaskybis.cds.unistra.fr/Planets/CDS_P_Io_Galileo-SSI-1km hips_status_1 = public mirror clonableOnce client_application = AladinDesktopBeta>=10.040 AladinDesktop>=11.125 moc_type = smoc moc_order = 3 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288467062 ID = CDS/P/JPSPR1 creator_did = ivo://CDS/P/JPSPR1 client_category = Image/Infrared obs_collection = JPS-PR1 obs_title = JPS-PR1 850um obs_description = The first data release of the James Clerk Maxwell Telescope (JCMT) Plane Survey (JPS), the JPS Public Release 1 (JPSPR1). JPS is an 850-um continuum survey of six fields in the northern inner Galactic Plane in a longitude range of l=7-63, made with the Sub-millimetre Common-User Bolometer Array 2 (SCUBA-2). This first data release consists of emission maps of the six JPS regions with an average pixel-to-pixel noise of 7.19 mJy beam^-1, when smoothed over the beam, and a compact-source catalogue containing 7,813 sources. The 95 per cent completeness limits of the catalogue are estimated at 0.04 Jy beam^-1 and 0.3 Jy for the peak and integrated flux densities, respectively. The emission contained in the compact-source catalogue is 42 +- 5 per cent of the total and, apart from the large-scale (greater than 8') emission, there is excellent correspondence with features in the 500-um Herschel maps. hips_initial_fov = 7.07 hips_initial_ra = 290.81517 hips_initial_dec = +15.07195 hips_pixel_bitpix = -64 data_pixel_bitpix = -64 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = median hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra prov_progenitor = CANFAR bib_reference = 2017MNRAS.469.2163E bib_reference_url = https://ui.adsabs.harvard.edu/abs/2017MNRAS.469.2163E/abstract t_min = 56063.54682 t_max = 57047.86049 obs_regime = Infrared em_min = 0.00085 em_max = 0.00085 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T06:38Z hips_frame = equatorial hips_order = 8 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = -52.2 638.1 hips_data_range = -7537 8151 hips_pixel_scale = 4.473E-4 s_pixel_scale = 8.333E-4 dataproduct_type = image moc_sky_fraction = 0.002219 hips_estsize = 7470921 hipsgen_date = 2017-05-03T14:19Z hipsgen_params = in=JPSPR1 out=hips ID=CDS/C/JPSPR1 INDEX TILES PNG DETAILS hips_creation_date = 2017-05-03T14:19Z hipsgen_date_1 = 2017-05-03T14:20Z hipsgen_params_1 = in=JPSPR1 out=hips ID=CDS/C/JPSPR1 INDEX TILES PNG DETAILS hips_order_min = 0 hipsgen_date_2 = 2019-05-21T06:38Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/pub/arXiv.1704.02982v1/JPSPR1 UPDATE hips_service_url = https://alasky.cds.unistra.fr/pub/arXiv.1704.02982v1/JPSPR1 hips_progenitor_url = https://alasky.cds.unistra.fr/pub/arXiv.1704.02982v1/JPSPR1/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/pub/arXiv.1704.02982v1/JPSPR1 hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 13 obs_initial_ra = 290.81517 obs_initial_dec = +15.07195 obs_initial_fov = 0.007157263357952928 TIMESTAMP = 1721288465418 ID = CDS/P/JWST/Carina-Nebula/NIRCam hips_initial_fov = 0.12146 hips_initial_ra = 159.21303 hips_initial_dec = -58.62017 creator_did = ivo://CDS/P/JWST/Carina-Nebula/NIRCam client_category = Image/Infrared/JWST hips_overlay = mean hips_hierarchy = median hips_creator = Boch T. (CDS) hips_copyright = CNRS/Unistra obs_title = Cosmic Cliffs in the Carina Nebula obs_collection = JWST obs_description = What looks much like craggy mountains on a moonlit evening is actually the edge of a nearby, young, star-forming region NGC 3324 in the Carina Nebula. Captured in infrared light by the Near-Infrared Camera (NIRCam) on NASA's James Webb Space Telescope, this image reveals previously obscured areas of star birth. Hipsilized by CDS. obs_ack = NASA, ESA, CSA, and STScI obs_ack_url = https://www.nasa.gov/webbfirstimages prov_progenitor = https://webbtelescope.org/news/first-images obs_copyright = NASA, ESA, CSA, and STScI obs_copyright_url = https://webbtelescope.org/copyright t_min = 59700 t_max = 59761 obs_regime = Infrared em_min = 6e-7 em_max = 5e-6 hips_builder = Aladin/HipsGen v11.071 hips_version = 1.4 hips_release_date = 2022-07-13T10:03Z hips_frame = equatorial hips_order = 14 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png hips_pixel_scale = 6.989E-6 s_pixel_scale = 1.012E-5 dataproduct_type = image dataproduct_subtype = color moc_sky_fraction = 2.287E-7 hips_estsize = 26421 hipsgen_date = 2022-07-13T10:03Z hipsgen_params = in=carina/stsci_2022-031a_12000.jpg creator_did=CDS/P/JWST/Carina-Nebula/NIRCam hips_service_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_Carina-Nebula_NIRCam hips_progenitor_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_Carina-Nebula_NIRCam/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/JWST/CDS_P_JWST_Carina-Nebula_NIRCam hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 14 obs_initial_ra = 159.21303 obs_initial_dec = -58.62017 obs_initial_fov = 0.003578631678976464 TIMESTAMP = 1721288490962 ID = CDS/P/JWST/Cartwheel/NIRCam+MIRI hips_initial_fov = 0.03904 hips_initial_ra = 9.42348 hips_initial_dec = -33.71324 creator_did = ivo://CDS/P/JWST/Cartwheel/NIRCam+MIRI client_category = Image/Infrared/JWST hips_overlay = mean hips_hierarchy = median hips_creator = Boch T. (CDS) hips_copyright = CNRS/Unistra obs_title = Cartwheel Galaxy obs_collection = JWST obs_description = This image of the Cartwheel and its companion galaxies is a composite from Webb's Near-Infrared Camera (NIRCam) and Mid-Infrared Instrument (MIRI), which reveals details that are difficult to see in the individual images alone. Webb's observations capture the Cartwheel in a very transitory stage. The form that the Cartwheel Galaxy will eventually take, given these two competing forces, is still a mystery. However, this snapshot provides perspective on what happened to the galaxy in the past and what it will do in the future. Hipslized by CDS. obs_ack = NASA, ESA, CSA, and STScI obs_ack_url = https://www.nasa.gov/webbfirstimages prov_progenitor = https://webbtelescope.org/news/first-images obs_copyright = NASA, ESA, CSA, and STScI obs_copyright_url = https://webbtelescope.org/copyright t_min = 59700 t_max = 59761 obs_regime = Infrared em_min = 6e-7 em_max = 2.8e-5 hips_builder = Aladin/HipsGen v11.071 hips_version = 1.4 hips_release_date = 2022-08-03T07:45Z hips_frame = equatorial hips_order = 14 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png hips_pixel_scale = 6.989E-6 s_pixel_scale = 8.333E-6 dataproduct_type = image dataproduct_subtype = color moc_sky_fraction = 4.221E-8 hips_estsize = 4882 hipsgen_date = 2022-08-03T07:45Z hipsgen_params = in=cartwheel/cartwheel-JWST.png creator_did=CDS/P/JWST/Cartwheel/NIRCam+MIRI hips_service_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_Cartwheel_NIRCam+MIRI hips_progenitor_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_Cartwheel_NIRCam+MIRI/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/JWST/CDS_P_JWST_Cartwheel_NIRCam+MIRI hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 14 obs_initial_ra = 9.42348 obs_initial_dec = -33.71324 obs_initial_fov = 0.003578631678976464 TIMESTAMP = 1721288491198 ID = CDS/P/JWST/Deep-Field-SMAC0723/NIRCam hips_initial_fov = 0.03857 hips_initial_ra = 110.8278 hips_initial_dec = -73.4539 creator_did = ivo://CDS/P/JWST/Deep-Field-SMAC0723/NIRCam client_category = Image/Infrared/JWST hips_overlay = mean hips_hierarchy = median hips_creator = Boch T. (CDS) hips_copyright = CNRS/Unistra obs_title = Webb's First Deep Field SMAC 0723 obs_collection = JWST obs_description = NASA's James Webb Space Telescope has produced the deepest and sharpest infrared image of the distant universe to date. Known as Webb's First Deep Field, this image of galaxy cluster SMACS 0723 is overflowing with detail. Thousands of galaxies - including the faintest objects ever observed in the infrared - have appeared in Webb's view for the first time. This slice of the vast universe covers a patch of sky approximately the size of a grain of sand held at arm's length by someone on the ground. This deep field, taken by Webb's Near-Infrared Camera (NIRCam), is a composite made from images at different wavelengths, totaling 12.5 hour. Hipsilized by CDS. obs_ack = NASA, ESA, CSA, and STScI obs_ack_url = https://www.nasa.gov/webbfirstimages prov_progenitor = https://webbtelescope.org/news/first-images obs_copyright = NASA, ESA, CSA, and STScI obs_copyright_url = https://webbtelescope.org/copyright t_min = 59700 t_max = 59761 obs_regime = Infrared em_min = 6e-7 em_max = 5e-6 hips_builder = Aladin/HipsGen v11.071 hips_version = 1.4 hips_release_date = 2022-07-11T22:32Z hips_frame = equatorial hips_order = 14 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png hips_pixel_scale = 6.989E-6 s_pixel_scale = 1.350E-5 dataproduct_type = image dataproduct_subtype = color moc_sky_fraction = 4.315E-8 hips_estsize = 4989 hipsgen_date = 2022-07-11T22:32Z hipsgen_params = in=in/main_image_deep_field_smacs0723-5mb.jpg creator_did=CDS/P/JWST/deep_field_smacs0723-5mb hips_service_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_deep_field_smacs0723-5mb hips_progenitor_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_deep_field_smacs0723-5mb/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/JWST/CDS_P_JWST_deep_field_smacs0723-5mb hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 14 obs_initial_ra = 110.8278 obs_initial_dec = -73.4539 obs_initial_fov = 0.003578631678976464 TIMESTAMP = 1721288490878 ID = CDS/P/JWST/EPO client_category = Outreach/JWST hips_creator = Boch T. 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APPEND/P/1719393753 addendum_id = APPEND/P/1719393773 addendum_id = APPEND/P/1719393788 addendum_id = APPEND/P/1719393805 addendum_id = APPEND/P/1719393823 addendum_id = APPEND/P/1719393835 addendum_id = APPEND/P/1719393850 addendum_id = APPEND/P/1719393869 addendum_id = APPEND/P/1719393883 addendum_id = APPEND/P/1719393899 addendum_id = APPEND/P/1719393915 addendum_id = APPEND/P/1719393930 addendum_id = APPEND/P/1719393948 addendum_id = APPEND/P/1719393963 addendum_id = APPEND/P/1719393980 addendum_id = APPEND/P/1719393995 addendum_id = APPEND/P/1719394008 addendum_id = APPEND/P/1719394022 addendum_id = APPEND/P/1719394034 addendum_id = APPEND/P/1719394049 addendum_id = APPEND/P/1719394062 addendum_id = APPEND/P/1719394075 addendum_id = APPEND/P/1719394089 addendum_id = APPEND/P/1719394101 addendum_id = APPEND/P/1719394114 addendum_id = APPEND/P/1719394126 addendum_id = APPEND/P/1719394139 addendum_id = APPEND/P/1719394152 addendum_id = APPEND/P/1719394165 addendum_id = 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APPEND/P/1719394969 addendum_id = APPEND/P/1719394979 addendum_id = APPEND/P/1719394989 addendum_id = APPEND/P/1719394998 addendum_id = APPEND/P/1719395006 addendum_id = APPEND/P/1719395014 hips_creation_date = 2024-06-26T09:01Z hipsgen_date_1 = 2024-06-26T09:01Z hipsgen_params_1 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392464 CONCAT hipsgen_date_2 = 2024-06-26T09:02Z hipsgen_params_2 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392494 CONCAT hipsgen_date_3 = 2024-06-26T09:02Z hipsgen_params_3 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392529 CONCAT hipsgen_date_4 = 2024-06-26T09:03Z hipsgen_params_4 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392558 CONCAT hipsgen_date_5 = 2024-06-26T09:03Z hipsgen_params_5 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392590 CONCAT hipsgen_date_6 = 2024-06-26T09:03Z hipsgen_params_6 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392620 CONCAT hipsgen_date_7 = 2024-06-26T09:04Z hipsgen_params_7 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392638 CONCAT hipsgen_date_8 = 2024-06-26T09:04Z hipsgen_params_8 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392662 CONCAT hipsgen_date_9 = 2024-06-26T09:05Z hipsgen_params_9 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392691 CONCAT hipsgen_date_10 = 2024-06-26T09:05Z hipsgen_params_10 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392717 CONCAT hipsgen_date_11 = 2024-06-26T09:06Z hipsgen_params_11 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392745 CONCAT hipsgen_date_12 = 2024-06-26T09:06Z hipsgen_params_12 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392771 CONCAT hipsgen_date_13 = 2024-06-26T09:06Z hipsgen_params_13 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392796 CONCAT hipsgen_date_14 = 2024-06-26T09:07Z hipsgen_params_14 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392825 CONCAT hipsgen_date_15 = 2024-06-26T09:07Z hipsgen_params_15 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392850 CONCAT hipsgen_date_16 = 2024-06-26T09:08Z hipsgen_params_16 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392878 CONCAT hipsgen_date_17 = 2024-06-26T09:08Z hipsgen_params_17 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392903 CONCAT hipsgen_date_18 = 2024-06-26T09:09Z hipsgen_params_18 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392930 CONCAT hipsgen_date_19 = 2024-06-26T09:09Z hipsgen_params_19 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392954 CONCAT hipsgen_date_20 = 2024-06-26T09:09Z hipsgen_params_20 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719392980 CONCAT hipsgen_date_21 = 2024-06-26T09:10Z hipsgen_params_21 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393002 CONCAT hipsgen_date_22 = 2024-06-26T09:10Z hipsgen_params_22 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393032 CONCAT hipsgen_date_23 = 2024-06-26T09:11Z hipsgen_params_23 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393055 CONCAT hipsgen_date_24 = 2024-06-26T09:11Z hipsgen_params_24 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393074 CONCAT hipsgen_date_25 = 2024-06-26T09:11Z hipsgen_params_25 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393102 CONCAT hipsgen_date_26 = 2024-06-26T09:12Z hipsgen_params_26 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393121 CONCAT hipsgen_date_27 = 2024-06-26T09:12Z hipsgen_params_27 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393148 CONCAT hipsgen_date_28 = 2024-06-26T09:12Z hipsgen_params_28 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393167 CONCAT hipsgen_date_29 = 2024-06-26T09:13Z hipsgen_params_29 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393183 CONCAT hipsgen_date_30 = 2024-06-26T09:13Z hipsgen_params_30 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393206 CONCAT hipsgen_date_31 = 2024-06-26T09:13Z hipsgen_params_31 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393225 CONCAT hipsgen_date_32 = 2024-06-26T09:14Z hipsgen_params_32 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393245 CONCAT hipsgen_date_33 = 2024-06-26T09:14Z hipsgen_params_33 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393267 CONCAT hipsgen_date_34 = 2024-06-26T09:15Z hipsgen_params_34 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393289 CONCAT hipsgen_date_35 = 2024-06-26T09:15Z hipsgen_params_35 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393310 CONCAT hipsgen_date_36 = 2024-06-26T09:15Z hipsgen_params_36 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393330 CONCAT hipsgen_date_37 = 2024-06-26T09:15Z hipsgen_params_37 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393344 CONCAT hipsgen_date_38 = 2024-06-26T09:16Z hipsgen_params_38 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393364 CONCAT hipsgen_date_39 = 2024-06-26T09:16Z hipsgen_params_39 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393381 CONCAT hipsgen_date_40 = 2024-06-26T09:16Z hipsgen_params_40 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393400 CONCAT hipsgen_date_41 = 2024-06-26T09:17Z hipsgen_params_41 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393421 CONCAT hipsgen_date_42 = 2024-06-26T09:17Z hipsgen_params_42 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393443 CONCAT hipsgen_date_43 = 2024-06-26T09:17Z hipsgen_params_43 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393459 CONCAT hipsgen_date_44 = 2024-06-26T09:18Z hipsgen_params_44 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393477 CONCAT hipsgen_date_45 = 2024-06-26T09:18Z hipsgen_params_45 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393497 CONCAT hipsgen_date_46 = 2024-06-26T09:18Z hipsgen_params_46 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393519 CONCAT hipsgen_date_47 = 2024-06-26T09:19Z hipsgen_params_47 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393543 CONCAT hipsgen_date_48 = 2024-06-26T09:19Z hipsgen_params_48 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393563 CONCAT hipsgen_date_49 = 2024-06-26T09:19Z hipsgen_params_49 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393575 CONCAT hipsgen_date_50 = 2024-06-26T09:20Z hipsgen_params_50 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393591 CONCAT hipsgen_date_51 = 2024-06-26T09:20Z hipsgen_params_51 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393611 CONCAT hipsgen_date_52 = 2024-06-26T09:20Z hipsgen_params_52 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393625 CONCAT hipsgen_date_53 = 2024-06-26T09:20Z hipsgen_params_53 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393640 CONCAT hipsgen_date_54 = 2024-06-26T09:22Z hipsgen_params_54 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393753 CONCAT hipsgen_date_55 = 2024-06-26T09:23Z hipsgen_params_55 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393773 CONCAT hipsgen_date_56 = 2024-06-26T09:23Z hipsgen_params_56 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393788 CONCAT hipsgen_date_57 = 2024-06-26T09:23Z hipsgen_params_57 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393805 CONCAT hipsgen_date_58 = 2024-06-26T09:23Z hipsgen_params_58 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393823 CONCAT hipsgen_date_59 = 2024-06-26T09:24Z hipsgen_params_59 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393835 CONCAT hipsgen_date_60 = 2024-06-26T09:24Z hipsgen_params_60 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393850 CONCAT hipsgen_date_61 = 2024-06-26T09:24Z hipsgen_params_61 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393869 CONCAT hipsgen_date_62 = 2024-06-26T09:24Z hipsgen_params_62 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393883 CONCAT hipsgen_date_63 = 2024-06-26T09:25Z hipsgen_params_63 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393899 CONCAT hipsgen_date_64 = 2024-06-26T09:25Z hipsgen_params_64 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393914 CONCAT hipsgen_date_65 = 2024-06-26T09:25Z hipsgen_params_65 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393930 CONCAT hipsgen_date_66 = 2024-06-26T09:25Z hipsgen_params_66 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393947 CONCAT hipsgen_date_67 = 2024-06-26T09:26Z hipsgen_params_67 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393963 CONCAT hipsgen_date_68 = 2024-06-26T09:26Z hipsgen_params_68 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393980 CONCAT hipsgen_date_69 = 2024-06-26T09:26Z hipsgen_params_69 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719393995 CONCAT hipsgen_date_70 = 2024-06-26T09:26Z hipsgen_params_70 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394008 CONCAT hipsgen_date_71 = 2024-06-26T09:27Z hipsgen_params_71 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394022 CONCAT hipsgen_date_72 = 2024-06-26T09:27Z hipsgen_params_72 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394034 CONCAT hipsgen_date_73 = 2024-06-26T09:27Z hipsgen_params_73 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394048 CONCAT hipsgen_date_74 = 2024-06-26T09:27Z hipsgen_params_74 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394062 CONCAT hipsgen_date_75 = 2024-06-26T09:28Z hipsgen_params_75 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394075 CONCAT hipsgen_date_76 = 2024-06-26T09:28Z hipsgen_params_76 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394089 CONCAT hipsgen_date_77 = 2024-06-26T09:28Z hipsgen_params_77 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394101 CONCAT hipsgen_date_78 = 2024-06-26T09:28Z hipsgen_params_78 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394114 CONCAT hipsgen_date_79 = 2024-06-26T09:28Z hipsgen_params_79 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394126 CONCAT hipsgen_date_80 = 2024-06-26T09:29Z hipsgen_params_80 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394139 CONCAT hipsgen_date_81 = 2024-06-26T09:29Z hipsgen_params_81 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394152 CONCAT hipsgen_date_82 = 2024-06-26T09:29Z hipsgen_params_82 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394165 CONCAT hipsgen_date_83 = 2024-06-26T09:29Z hipsgen_params_83 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394179 CONCAT hipsgen_date_84 = 2024-06-26T09:30Z hipsgen_params_84 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394193 CONCAT hipsgen_date_85 = 2024-06-26T09:30Z hipsgen_params_85 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394208 CONCAT hipsgen_date_86 = 2024-06-26T09:30Z hipsgen_params_86 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394221 CONCAT hipsgen_date_87 = 2024-06-26T09:30Z hipsgen_params_87 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394233 CONCAT hipsgen_date_88 = 2024-06-26T09:30Z hipsgen_params_88 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394246 CONCAT hipsgen_date_89 = 2024-06-26T09:31Z hipsgen_params_89 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394259 CONCAT hipsgen_date_90 = 2024-06-26T09:31Z hipsgen_params_90 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394274 CONCAT hipsgen_date_91 = 2024-06-26T09:31Z hipsgen_params_91 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394286 CONCAT hipsgen_date_92 = 2024-06-26T09:31Z hipsgen_params_92 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394299 CONCAT hipsgen_date_93 = 2024-06-26T09:32Z hipsgen_params_93 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394316 CONCAT hipsgen_date_94 = 2024-06-26T09:32Z hipsgen_params_94 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394331 CONCAT hipsgen_date_95 = 2024-06-26T09:32Z hipsgen_params_95 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394346 CONCAT hipsgen_date_96 = 2024-06-26T09:32Z hipsgen_params_96 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394360 CONCAT hipsgen_date_97 = 2024-06-26T09:33Z hipsgen_params_97 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394374 CONCAT hipsgen_date_98 = 2024-06-26T09:33Z hipsgen_params_98 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394389 CONCAT hipsgen_date_99 = 2024-06-26T09:33Z hipsgen_params_99 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394404 CONCAT hipsgen_date_100 = 2024-06-26T09:33Z hipsgen_params_100 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394419 CONCAT hipsgen_date_101 = 2024-06-26T09:34Z hipsgen_params_101 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394438 CONCAT hipsgen_date_102 = 2024-06-26T09:34Z hipsgen_params_102 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394458 CONCAT hipsgen_date_103 = 2024-06-26T09:34Z hipsgen_params_103 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394472 CONCAT hipsgen_date_104 = 2024-06-26T09:34Z hipsgen_params_104 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394485 CONCAT hipsgen_date_105 = 2024-06-26T09:35Z hipsgen_params_105 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394499 CONCAT hipsgen_date_106 = 2024-06-26T09:35Z hipsgen_params_106 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394514 CONCAT hipsgen_date_107 = 2024-06-26T09:35Z hipsgen_params_107 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394528 CONCAT hipsgen_date_108 = 2024-06-26T09:35Z hipsgen_params_108 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394541 CONCAT hipsgen_date_109 = 2024-06-26T09:36Z hipsgen_params_109 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394556 CONCAT hipsgen_date_110 = 2024-06-26T09:36Z hipsgen_params_110 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394571 CONCAT hipsgen_date_111 = 2024-06-26T09:36Z hipsgen_params_111 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394586 CONCAT hipsgen_date_112 = 2024-06-26T09:36Z hipsgen_params_112 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394601 CONCAT hipsgen_date_113 = 2024-06-26T09:37Z hipsgen_params_113 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394615 CONCAT hipsgen_date_114 = 2024-06-26T09:37Z hipsgen_params_114 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394628 CONCAT hipsgen_date_115 = 2024-06-26T09:37Z hipsgen_params_115 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394644 CONCAT hipsgen_date_116 = 2024-06-26T09:37Z hipsgen_params_116 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394658 CONCAT hipsgen_date_117 = 2024-06-26T09:38Z hipsgen_params_117 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394671 CONCAT hipsgen_date_118 = 2024-06-26T09:38Z hipsgen_params_118 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394685 CONCAT hipsgen_date_119 = 2024-06-26T09:38Z hipsgen_params_119 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394699 CONCAT hipsgen_date_120 = 2024-06-26T09:38Z hipsgen_params_120 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394711 CONCAT hipsgen_date_121 = 2024-06-26T09:38Z hipsgen_params_121 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394726 CONCAT hipsgen_date_122 = 2024-06-26T09:39Z hipsgen_params_122 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394740 CONCAT hipsgen_date_123 = 2024-06-26T09:39Z hipsgen_params_123 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394752 CONCAT hipsgen_date_124 = 2024-06-26T09:39Z hipsgen_params_124 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394768 CONCAT hipsgen_date_125 = 2024-06-26T09:39Z hipsgen_params_125 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394780 CONCAT hipsgen_date_126 = 2024-06-26T09:40Z hipsgen_params_126 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394792 CONCAT hipsgen_date_127 = 2024-06-26T09:40Z hipsgen_params_127 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394807 CONCAT hipsgen_date_128 = 2024-06-26T09:40Z hipsgen_params_128 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394821 CONCAT hipsgen_date_129 = 2024-06-26T09:40Z hipsgen_params_129 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394834 CONCAT hipsgen_date_130 = 2024-06-26T09:40Z hipsgen_params_130 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394846 CONCAT hipsgen_date_131 = 2024-06-26T09:41Z hipsgen_params_131 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394857 CONCAT hipsgen_date_132 = 2024-06-26T09:41Z hipsgen_params_132 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394870 CONCAT hipsgen_date_133 = 2024-06-26T09:41Z hipsgen_params_133 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394884 CONCAT hipsgen_date_134 = 2024-06-26T09:41Z hipsgen_params_134 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394893 CONCAT hipsgen_date_135 = 2024-06-26T09:41Z hipsgen_params_135 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394904 CONCAT hipsgen_date_136 = 2024-06-26T09:42Z hipsgen_params_136 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394914 CONCAT hipsgen_date_137 = 2024-06-26T09:42Z hipsgen_params_137 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394924 CONCAT hipsgen_date_138 = 2024-06-26T09:42Z hipsgen_params_138 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394937 CONCAT hipsgen_date_139 = 2024-06-26T09:42Z hipsgen_params_139 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394948 CONCAT hipsgen_date_140 = 2024-06-26T09:42Z hipsgen_params_140 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394958 CONCAT hipsgen_date_141 = 2024-06-26T09:42Z hipsgen_params_141 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394969 CONCAT hipsgen_date_142 = 2024-06-26T09:43Z hipsgen_params_142 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394979 CONCAT hipsgen_date_143 = 2024-06-26T09:43Z hipsgen_params_143 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394989 CONCAT hipsgen_date_144 = 2024-06-26T09:43Z hipsgen_params_144 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719394998 CONCAT hipsgen_date_145 = 2024-06-26T09:43Z hipsgen_params_145 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719395006 CONCAT hipsgen_date_146 = 2024-06-26T09:43Z hipsgen_params_146 = out=hips/CDS_P_JWST_EPO in=hips/CDS_P_JWST_EPO/AddsHips1719395014 CONCAT hipsgen_date_147 = 2024-06-26T09:43Z hipsgen_params_147 = out=hips/CDS_P_JWST_EPO id=CDS/P/JWST/EPO CLEANWEIGHT hips_service_url = https://alasky.cds.unistra.fr/JWST-outreach/CDS_P_JWST_EPO hips_progenitor_url = https://alasky.cds.unistra.fr/JWST-outreach/CDS_P_JWST_EPO/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/JWST-outreach/CDS_P_JWST_EPO hips_status_1 = public mirror clonableOnce moc_type = smoc moc_sky_fraction = 8.338E-6 moc_order = 14 obs_initial_ra = 274.732621 obs_initial_dec = -13.8452489 obs_initial_fov = 0.003578631678976464 TIMESTAMP = 1723788087529 ID = CDS/P/JWST/F115W hips_doi = 10.26093/cds/aladin/32j1-j07 creator_did = ivo://CDS/P/JWST/F115W hips_creator = Durand D. (CDS) hips_copyright = CNRS/Unistra obs_title = JWST F115W (beta) obs_collection = JWST obs_description = The JWST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all JWST observations done in obs_ack = This work is based [in part] on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. t_min = 59632.6192776682 t_max = 60056.3072676736 obs_regime = Infrared client_category = Image/Infrared/JWST moc_sky_fraction = 1.426E-5 hips_builder = Aladin/HipsGen v12.044 hips_version = 1.4 hips_frame = equatorial hips_order = 14 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 3.5834580 hips_initial_dec = -30.3882779 hips_initial_fov = 0.09933 hips_pixel_scale = 6.989E-6 s_pixel_scale = 8.701E-6 dataproduct_type = image hipsgen_date = 2023-05-05T10:14Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=F115W -in=/data-test-iscsi/d.durand/2023A/JWST/F115W.extract -id=CDS/P/JWST/F115W -blank=0 -order=14 -mocOrder=17 -out=/data-test-iscsi/d.durand/2023A/JWST/F115W.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwriteTile treeMean hips_tile_format = png fits hips_pixel_cut = 0.1391 0.7523 hips_data_range = -24.96 71.96 hips_release_date = 2023-05-05T14:42Z hips_estsize = 83565421 hips_nb_tiles = 140370 hips_check_code = png:66199641 fits:1067565097 hips_service_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_F115W hips_progenitor_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_F115W/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/JWST/CDS_P_JWST_F115W hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 17 obs_initial_ra = 3.5834580 obs_initial_dec = -30.3882779 obs_initial_fov = 4.47328959872058E-4 TIMESTAMP = 1721288491682 ID = CDS/P/JWST/F150W hips_doi = 10.26093/cds/aladin/2znx-54y creator_did = ivo://CDS/P/JWST/F150W hips_creator = Durand D. (CDS) hips_copyright = CNRS/Unistra obs_title = JWST F150W (beta) obs_collection = JWST obs_description = The JWST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all JWST observations done in obs_ack = This work is based [in part] on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. t_min = 59612.2992469815 t_max = 60056.9805759028 obs_regime = Infrared client_category = Image/Infrared/JWST moc_sky_fraction = 1.798E-5 hips_builder = Aladin/HipsGen v12.044 hips_version = 1.4 hips_frame = equatorial hips_order = 14 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 53.1604685 hips_initial_dec = -27.7843480 hips_initial_fov = 0.08565 hips_pixel_scale = 6.989E-6 s_pixel_scale = 8.586E-6 dataproduct_type = image hipsgen_date = 2023-05-05T10:19Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=F150W -in=/data-test-iscsi/d.durand/2023A/JWST/F150W.extract -id=CDS/P/JWST/F150W -blank=0 -order=14 -mocOrder=17 -out=/data-test-iscsi/d.durand/2023A/JWST/F150W.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwrite treeMean hips_tile_format = png fits hipsgen_date_1 = 2023-05-05T10:19Z hips_release_date = 2023-05-05T16:06Z hips_creation_date = 2023-05-05T14:07Z hips_estsize = 105893663 hips_nb_tiles = 182122 hips_check_code = png:158007384 fits:1035360949 hipsgen_params_1 = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=F150W -in=/data-test-iscsi/d.durand/2023A/JWST/F150W.extract -id=CDS/P/JWST/F150W -blank=0 -order=14 -mocOrder=17 -out=/data-test-iscsi/d.durand/2023A/JWST/F150W.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_service_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_F150W hips_progenitor_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_F150W/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/JWST/CDS_P_JWST_F150W hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 17 obs_initial_ra = 53.1604685 obs_initial_dec = -27.7843480 obs_initial_fov = 4.47328959872058E-4 TIMESTAMP = 1721288491734 ID = CDS/P/JWST/F200W hips_doi = 10.26093/cds/aladin/2nj1-ycv creator_did = ivo://CDS/P/JWST/F200W hips_creator = Durand D. (CDS) hips_copyright = CNRS/Unistra obs_title = JWST F200W (beta) obs_collection = JWST obs_description = The JWST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all JWST observations done in obs_ack = This work is based [in part] on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. t_min = 59612.306330673 t_max = 60057.0065484722 obs_regime = Infrared client_category = Image/Infrared/JWST moc_sky_fraction = 1.022E-5 hips_builder = Aladin/HipsGen v12.044 hips_version = 1.4 hips_frame = equatorial hips_order = 14 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 233.7384332 hips_initial_dec = +23.5032246 hips_initial_fov = 0.08569 hips_pixel_scale = 6.989E-6 s_pixel_scale = 8.540E-6 dataproduct_type = image hipsgen_date = 2023-05-05T16:36Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=F200W -in=/data-test-iscsi/d.durand/2023A/JWST/F200W.extract -id=CDS/P/JWST/F200W -blank=0 -order=14 -mocOrder=17 -out=/data-test-iscsi/d.durand/2023A/JWST/F200W.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwriteTile treeMean hips_release_date = 2023-05-05T19:11Z hips_tile_format = png fits hips_creation_date = 2023-05-05T18:02Z hips_estsize = 63286871 hips_nb_tiles = 111420 hips_check_code = png:3218719029 fits:737322526 hips_service_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_F200W hips_progenitor_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_F200W/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/JWST/CDS_P_JWST_F200W hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 17 obs_initial_ra = 233.7384332 obs_initial_dec = +23.5032246 obs_initial_fov = 4.47328959872058E-4 TIMESTAMP = 1721288491802 ID = CDS/P/JWST/F210M hips_doi = 10.26093/cds/aladin/1br0-tpp creator_did = ivo://CDS/P/JWST/F210M hips_creator = Durand D. (CDS) hips_copyright = CNRS/Unistra obs_title = JWST F210M (beta) obs_collection = JWST obs_description = The JWST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all JWST observations done in obs_ack = This work is based [in part] on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. obs_regime = Infrared client_category = Image/Infrared/JWST moc_sky_fraction = 2.066E-6 hips_builder = Aladin/HipsGen v12.044 hips_version = 1.4 hips_frame = equatorial hips_order = 14 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 89.9412 hips_initial_dec = -65.81183 hips_initial_fov = 0.00362 hips_pixel_scale = 6.989E-6 s_pixel_scale = 8.508E-6 dataproduct_type = image hipsgen_date = 2023-05-05T16:36Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=F210M -in=/data-test-iscsi/d.durand/2023A/JWST/F210M.extract -id=CDS/P/JWST/F210M -blank=0 -order=14 -mocOrder=17 -out=/data-test-iscsi/d.durand/2023A/JWST/F210M.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwriteTile treeMean hips_release_date = 2023-05-05T18:13Z hips_tile_format = png fits hips_pixel_cut = -2.962 3077 hips_data_range = -36747 110196 hips_creation_date = 2023-05-05T17:45Z hips_estsize = 12799678 hips_nb_tiles = 22220 hips_check_code = png:3142953536 fits:4009463526 hips_service_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_F210M hips_progenitor_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_F210M/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/JWST/CDS_P_JWST_F210M hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 17 obs_initial_ra = 89.9412 obs_initial_dec = -65.81183 obs_initial_fov = 4.47328959872058E-4 TIMESTAMP = 1721288491858 ID = CDS/P/JWST/F212N hips_doi = 10.26093/cds/aladin/3yby-pfe creator_did = ivo://CDS/P/JWST/F212N hips_creator = Durand D. (CDS) hips_copyright = CNRS/Unistra obs_title = JWST F212N (beta) obs_collection = JWST obs_description = The JWST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all JWST observations done in obs_ack = This work is based [in part] on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. t_min = 59612.8332408199 t_max = 60040.9079674769 obs_regime = Infrared client_category = Image/Infrared/JWST moc_sky_fraction = 5.449E-6 hips_builder = Aladin/HipsGen v12.044 hips_version = 1.4 hips_frame = equatorial hips_order = 14 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 159.36613 hips_initial_dec = -69.65746 hips_initial_fov = 0.03717 hips_pixel_scale = 6.989E-6 s_pixel_scale = 8.458E-6 dataproduct_type = image hipsgen_date = 2023-05-05T23:33Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=F212N -in=/data-test-iscsi/d.durand/2023A/JWST/F212N.extract -id=CDS/P/JWST/F212N -blank=0 -order=14 -mocOrder=17 -out=/data-test-iscsi/d.durand/2023A/JWST/F212N.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwriteTile treeMean hips_release_date = 2023-05-06T02:33Z hips_tile_format = png fits hips_pixel_cut = -0.2945 2.795 hips_data_range = -23.35 55.74 hips_creation_date = 2023-05-06T01:28Z hips_estsize = 31439366 hips_nb_tiles = 51716 hips_check_code = png:322815795 fits:677351810 hips_service_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_F212N hips_progenitor_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_F212N/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/JWST/CDS_P_JWST_F212N hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 17 obs_initial_ra = 159.36613 obs_initial_dec = -69.65746 obs_initial_fov = 4.47328959872058E-4 TIMESTAMP = 1721288491910 ID = CDS/P/JWST/F444W hips_doi = 10.26093/cds/aladin/3pjx-jwz creator_did = ivo://CDS/P/JWST/F444W hips_creator = Durand D. (CDS) hips_copyright = CNRS/Unistra obs_title = JWST F444W (beta) obs_collection = JWST obs_description = The JWST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all JWST observations done in obs_ack = This work is based [in part] on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. t_min = 59612.3063306736 t_max = 60056.9652907292 obs_regime = Infrared client_category = Image/Infrared/JWST moc_sky_fraction = 1.703E-5 hips_builder = Aladin/HipsGen v12.044 hips_version = 1.4 hips_frame = equatorial hips_order = 14 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 83.82 hips_initial_dec = -5.39 hips_initial_fov = 0.085 hips_pixel_scale = 6.989E-6 s_pixel_scale = 1.750E-5 dataproduct_type = image hipsgen_date = 2023-05-05T23:34Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=F444W -in=/data-test-iscsi/d.durand/2023A/JWST/F444W.extract -id=CDS/P/JWST/F444W -blank=0 -order=14 -mocOrder=17 -out=/data-test-iscsi/d.durand/2023A/JWST/F444W.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwriteTile treeMean hips_release_date = 2023-05-06T02:45Z hips_tile_format = png fits hips_pixel_cut = -0.1063 0.3471 hips_data_range = -1.334 1.57 hips_creation_date = 2023-05-06T01:58Z hips_estsize = 92515477 hips_nb_tiles = 169066 hips_check_code = png:1859473588 fits:1288804405 hips_service_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_F444W hips_progenitor_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_F444W/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/JWST/CDS_P_JWST_F444W hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 17 obs_initial_ra = 83.82 obs_initial_dec = -5.39 obs_initial_fov = 4.47328959872058E-4 TIMESTAMP = 1721288491966 ID = CDS/P/JWST/F480M hips_doi = 10.26093/cds/aladin/1ykm-3m5 creator_did = ivo://CDS/P/JWST/F480M hips_creator = Durand D. (CDS) hips_copyright = CNRS/Unistra obs_title = JWST F480M (beta) obs_collection = JWST obs_description = The JWST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all JWST observations done in obs_ack = This work is based [in part] on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. t_min = 59612.8332400792 t_max = 60051.9467064236 obs_regime = Infrared client_category = Image/Infrared/JWST moc_sky_fraction = 5.694E-6 hips_builder = Aladin/HipsGen v12.044 hips_version = 1.4 hips_frame = equatorial hips_order = 14 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 53.1586337 hips_initial_dec = -27.7828882 hips_initial_fov = 0.03632 hips_pixel_scale = 6.989E-6 s_pixel_scale = 1.750E-5 dataproduct_type = image hipsgen_date = 2023-05-06T07:26Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=F480M -in=/data-test-iscsi/d.durand/2023A/JWST/F480M.extract -id=CDS/P/JWST/F480M -blank=0 -order=14 -mocOrder=17 -out=/data-test-iscsi/d.durand/2023A/JWST/F480M.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwriteTile treeMean hips_release_date = 2023-05-06T09:22Z hips_tile_format = png fits hips_pixel_cut = 0.2751 61.99 hips_data_range = -726.7 2070 hips_creation_date = 2023-05-06T09:12Z hips_estsize = 30810328 hips_nb_tiles = 55520 hips_check_code = png:4233275037 fits:3057106928 hips_service_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_F480M hips_progenitor_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_F480M/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/JWST/CDS_P_JWST_F480M hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 17 obs_initial_ra = 53.1586337 obs_initial_dec = -27.7828882 obs_initial_fov = 4.47328959872058E-4 TIMESTAMP = 1721288492026 ID = CDS/P/JWST/First-Images hips_initial_fov = 0.10547 hips_initial_ra = 338.99754 hips_initial_dec = +33.96049 creator_did = ivo://CDS/P/JWST/First-Images client_category = Image/Infrared/JWST hips_overlay = mean hips_hierarchy = median hips_creator = Boch T. (CDS) hips_copyright = CNRS/Unistra obs_title = JWST First Images obs_collection = JWST obs_description = First images of JWST, hipsilized by CDS. I. NASA's James Webb Space Telescope has produced the deepest and sharpest infrared image of the distant universe to date. Known as Webb's First Deep Field, this image of galaxy cluster SMACS 0723 is overflowing with detail. This deep field, taken by Webb's Near-Infrared Camera (NIRCam), is a composite made from images at different wavelengths, totaling 12.5 hour. II. What looks much like craggy mountains on a moonlit evening is actually the edge of a nearby, young, star-forming region NGC 3324 in the Carina Nebula. Captured in infrared light by the Near-Infrared Camera (NIRCam) on NASA's James Webb Space Telescope, this image reveals previously obscured areas of star birth. III. An enormous mosaic of Stephan's Quintet is the largest image to date from NASA's James Webb Space Telescope, covering about one-fifth of the Moon's diameter. The visual grouping of five galaxies was captured by Webb's Near-Infrared Camera (NIRCam) and Mid-Infrared Instrument (MIRI). IV. The Southern Ring Nebula in near-infrared light. V. The image of the Cartwheel and its companion galaxies, a composite from Webb's NIRCam and MIRI. obs_ack = NASA, ESA, CSA, and STScI obs_ack_url = https://www.nasa.gov/webbfirstimages prov_progenitor = https://webbtelescope.org/news/first-images obs_copyright = NASA, ESA, CSA, and STScI obs_copyright_url = https://webbtelescope.org/copyright t_min = 59700 t_max = 59761 obs_regime = Infrared em_min = 6e-7 em_max = 2.8e-5 hips_builder = Aladin/HipsGen v11.914 hips_version = 1.4 hips_release_date = 2022-08-03T08:46Z hips_frame = equatorial hips_order = 14 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png hips_pixel_scale = 6.989E-6 s_pixel_scale = 8.789E-6 dataproduct_type = image moc_sky_fraction = 6.398E-7 hipsgen_date = 2022-07-13T10:30Z hipsgen_params = in=stephan/stsci_2022-034a_12000.jpg creator_did=CDS/P/JWST/Stephans-Quintet/NIRCam+MIRI addendum_id = CDS/P/JWST/Southern-Ring-Nebula/NIRCam addendum_id = CDS/P/JWST/Cartwheel/NIRCam+MIRI hips_creation_date = 2022-07-13T10:30Z hipsgen_date_1 = 2022-07-29T10:37Z hipsgen_params_1 = in=CDS_P_JWST_Southern-Ring-Nebula_NIRCam out=CDS_P_JWST_Stephans-Quintet_NIRCam+MIRI CONCAT dataproduct_subtype = color hipsgen_date_2 = 2022-08-03T08:46Z hipsgen_params_2 = in=CDS_P_JWST_Cartwheel_NIRCam+MIRI out=CDS_P_JWST_First_Images CONCAT hips_service_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_First_Images hips_progenitor_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_First_Images/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/JWST/CDS_P_JWST_First_Images hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 14 obs_initial_ra = 338.99754 obs_initial_dec = +33.96049 obs_initial_fov = 0.003578631678976464 TIMESTAMP = 1721288491622 ID = CDS/P/JWST/OPEN hips_doi = 10.26093/cds/aladin/pg0c-rj creator_did = ivo://CDS/P/JWST/OPEN hips_creator = Durand D. (CDS) hips_copyright = CNRS/Unistra obs_title = JWST OPEN (beta) obs_collection = JWST obs_description = The JWST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all JWST observations done in obs_ack = This work is based [in part] on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. obs_regime = Infrared client_category = Image/Infrared/JWST moc_sky_fraction = 8.269E-7 hips_builder = Aladin/HipsGen v12.044 hips_version = 1.4 hips_frame = equatorial hips_order = 14 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_initial_ra = 80.00003 hips_initial_dec = -69.61116 hips_initial_fov = 0.04021 hips_pixel_scale = 6.989E-6 s_pixel_scale = 1.889E-5 dataproduct_type = image hipsgen_date = 2023-05-06T07:27Z hipsgen_params = -maxThread=35 "-creator=CDS (Daniel Durand)" -title=OPEN -in=/data-test-iscsi/d.durand/2023A/JWST/OPEN.extract -id=CDS/P/JWST/OPEN -blank=0 -order=14 -mocOrder=17 -out=/data-test-iscsi/d.durand/2023A/JWST/OPEN.hips "-pixelCut=9% 99.9% byRegion log" "-fitskeys=DSNAME INSTRUME OPT_ELE T_MIN T_MAX TIME_EXP WAVE_MIN WAVE_MAX PROP_ID TARGNAME OBS_DATE URLPATH URLPREV" hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = overlayMean mergeOverwriteTile treeMean hips_release_date = 2023-05-06T10:39Z hips_tile_format = png fits hips_pixel_cut = 0.3488 19.58 hips_data_range = -59.43 101.7 hips_creation_date = 2023-05-06T10:34Z hips_estsize = 5215464 hips_nb_tiles = 9144 hips_check_code = png:1173925588 fits:738895196 hips_service_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_OPEN hips_progenitor_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_OPEN/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/JWST/CDS_P_JWST_OPEN hips_status_1 = public mirror clonableOnce moc_type = smoc moc_order = 17 obs_initial_ra = 80.00003 obs_initial_dec = -69.61116 obs_initial_fov = 4.47328959872058E-4 TIMESTAMP = 1721288492086 ID = CDS/P/JWST/Southern-Ring-Nebula/NIRCam hips_initial_fov = 0.04027 hips_initial_ra = 151.75593 hips_initial_dec = -40.43597 creator_did = ivo://CDS/P/JWST/Southern-Ring-Nebula/NIRCam client_category = Image/Infrared/JWST hips_overlay = mean hips_hierarchy = median hips_creator = Boch T. (CDS) hips_copyright = CNRS/Unistra obs_title = Southern Ring Nebula obs_collection = JWST obs_description = Southern Ring Nebula in near-infrared light from NASA's Webb Telescope. Hipsilized by CDS. obs_ack = NASA, ESA, CSA, and STScI obs_ack_url = https://www.nasa.gov/webbfirstimages prov_progenitor = https://webbtelescope.org/news/first-images obs_copyright = NASA, ESA, CSA, and STScI obs_copyright_url = https://webbtelescope.org/copyright t_min = 59700 t_max = 59761 obs_regime = Infrared em_min = 6e-7 em_max = 5e-6 hips_builder = Aladin/HipsGen v11.071 hips_version = 1.4 hips_release_date = 2022-07-13T12:40Z hips_frame = equatorial hips_order = 14 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png hips_pixel_scale = 6.989E-6 s_pixel_scale = 8.329E-6 dataproduct_type = image dataproduct_subtype = color moc_sky_fraction = 4.563E-8 hips_estsize = 15828 hipsgen_date = 2022-07-13T12:40Z hipsgen_params = in=ring/jwst-ring.png creator_did=CDS/P/JWST/Southern-Ring-Nebula/NIRCam hips_service_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_Southern-Ring-Nebula_NIRCam hips_progenitor_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_Southern-Ring-Nebula_NIRCam/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/JWST/CDS_P_JWST_Southern-Ring-Nebula_NIRCam hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 14 obs_initial_ra = 151.75593 obs_initial_dec = -40.43597 obs_initial_fov = 0.003578631678976464 TIMESTAMP = 1721288491022 ID = CDS/P/JWST/Stephans-Quintet/MIRI hips_initial_fov = 0.07465 hips_initial_ra = 339.00606 hips_initial_dec = +33.95971 creator_did = ivo://CDS/P/JWST/Stephans-Quintet/MIRI client_category = Image/Infrared/JWST hips_overlay = mean hips_hierarchy = median hips_creator = Boch T. (CDS) hips_copyright = CNRS/Unistra obs_title = Stephans Quintet MIRI obs_collection = JWST obs_description = An enormous mosaic of Stephan's Quintet is the largest image to date from NASA's James Webb Space Telescope, covering about one-fifth of the Moon's diameter. It contains over 150 million pixels and is constructed from almost 1,000 separate image files. The visual grouping of five galaxies was captured by Webb's Mid-Infrared Instrument (MIRI). Hipsilized by CDS. obs_ack = NASA, ESA, CSA, and STScI obs_ack_url = https://www.nasa.gov/webbfirstimages prov_progenitor = https://webbtelescope.org/news/first-images obs_copyright = NASA, ESA, CSA, and STScI obs_copyright_url = https://webbtelescope.org/copyright t_min = 59700 t_max = 59761 obs_regime = Infrared em_min = 5e-6 em_max = 2.8e-5 hips_builder = Aladin/HipsGen v11.071 hips_version = 1.4 hips_release_date = 2022-07-13T13:02Z hips_frame = equatorial hips_order = 12 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png hips_pixel_scale = 2.795E-5 s_pixel_scale = 3.054E-5 dataproduct_type = image dataproduct_subtype = color moc_sky_fraction = 1.788E-7 hips_estsize = 3894 hipsgen_date = 2022-07-13T13:02Z hipsgen_params = in=quintet-MIRI/jwst-stephan-miri.png creator_did=CDS/P/JWST/Stephans-Quintet/MIRI hips_service_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_Stephans-Quintet_MIRI hips_progenitor_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_Stephans-Quintet_MIRI/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/JWST/CDS_P_JWST_Stephans-Quintet_MIRI hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 12 obs_initial_ra = 339.00606 obs_initial_dec = +33.95971 obs_initial_fov = 0.014314526715905856 TIMESTAMP = 1721288491090 ID = CDS/P/JWST/Stephans-Quintet/NIRCam+MIRI hips_initial_fov = 0.10547 hips_initial_ra = 338.99754 hips_initial_dec = +33.96049 creator_did = ivo://CDS/P/JWST/Stephans-Quintet/NIRCam+MIRI client_category = Image/Infrared/JWST hips_overlay = mean hips_hierarchy = median hips_creator = Boch T. (CDS) hips_copyright = CNRS/Unistra obs_title = Stephans-Quintet NIRCam+MIRI obs_collection = JWST obs_description = An enormous mosaic of Stephan's Quintet is the largest image to date from NASA's James Webb Space Telescope, covering about one-fifth of the Moon's diameter. It contains over 150 million pixels and is constructed from almost 1,000 separate image files. The visual grouping of five galaxies was captured by Webb's Near-Infrared Camera (NIRCam) and Mid-Infrared Instrument (MIRI). Hipslized by CDS. obs_ack = NASA, ESA, CSA, and STScI obs_ack_url = https://www.nasa.gov/webbfirstimages prov_progenitor = https://webbtelescope.org/news/first-images obs_copyright = NASA, ESA, CSA, and STScI obs_copyright_url = https://webbtelescope.org/copyright t_min = 59700 t_max = 59761 obs_regime = Infrared em_min = 6e-7 em_max = 2.8e-5 hips_builder = Aladin/HipsGen v11.071 hips_version = 1.4 hips_release_date = 2022-07-13T10:30Z hips_frame = equatorial hips_order = 14 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png hips_pixel_scale = 6.989E-6 s_pixel_scale = 8.789E-6 dataproduct_type = image dataproduct_subtype = color moc_sky_fraction = 2.800E-7 hips_estsize = 32335 hipsgen_date = 2022-07-13T10:30Z hipsgen_params = in=stephan/stsci_2022-034a_12000.jpg creator_did=CDS/P/JWST/Stephans-Quintet/NIRCam+MIRI hips_service_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_Stephans-Quintet_NIRCam+MIRI hips_progenitor_url = https://alasky.cds.unistra.fr/JWST/CDS_P_JWST_Stephans-Quintet_NIRCam+MIRI/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/JWST/CDS_P_JWST_Stephans-Quintet_NIRCam+MIRI hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 14 obs_initial_ra = 338.99754 obs_initial_dec = +33.96049 obs_initial_fov = 0.003578631678976464 TIMESTAMP = 1721288491146 ID = CDS/P/Jupiter/PIA07782 client_category = Solar system/Jupiter hips_initial_fov = 180 hips_initial_ra = 0 hips_initial_dec = +0 creator_did = ivo://CDS/P/Jupiter/PIA07782 hips_overlay = mean hips_hierarchy = median obs_title = Jupiter PIA07782 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T07:01Z hips_frame = jupiter hips_body = jupiter hips_order = 3 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = jpeg hips_pixel_scale = 0.01431 s_pixel_scale = 0.1 dataproduct_type = image moc_sky_fraction = 1 hips_estsize = 18357 hipsgen_date = 2018-01-13T19:00Z hipsgen_params = "in=D:\\Planet\\JupiterPIA07782" "out=D:\\Planet\\Jupiter2HiPS" color=true creator_did=CDS/P/Jupiter/PIA07782 -f INDEX TILES hips_creation_date = 2018-01-13T19:01Z hips_order_min = 0 dataproduct_subtype = color hipsgen_date_1 = 2019-05-21T07:01Z hipsgen_params_1 = out=/asd-volumes/sc1-asd-volume6/Planets/CDS_P_Jupiter_PIA07782 UPDATE hips_service_url = https://alasky.cds.unistra.fr/Planets/CDS_P_Jupiter_PIA07782 hips_service_url_1 = https://alaskybis.cds.unistra.fr/Planets/CDS_P_Jupiter_PIA07782 hips_status_1 = public mirror clonableOnce client_application = AladinDesktopBeta>=10.040 AladinDesktop>=11.125 moc_type = smoc moc_order = 3 obs_initial_ra = 0 obs_initial_dec = +0 obs_initial_fov = 7.3290376785437985 TIMESTAMP = 1721288466674 ID = CDS/P/KiDS/DR5/color-gri hips_initial_ra = 50.32083 hips_initial_dec = -27.1722 hips_initial_fov = 0.3 creator_did = ivo://CDS/P/KiDS/DR5/color-gri hips_creator = Kuijken K. (KiDS team) obs_title = KiDS color gri obs_collection = KiDS prov_progenitor = ESO Science Archive obs_description = The Kilo-Degree Survey (KiDS) covers 1346 square degrees of sky in u,g,r,i bands, and was primarily designed for weak gravitational lensing studies. It used the OmegaCAM instrument on the VLT Survey Telescope on Paranal, and took data between 2011 and 2019. These colour images are from the final data release, DR5, and are being made available pre-publication. Description of the data reduction procedures can be found in the DR4 release paper, and will be updated, together with the corresponding FITS files, in due course. bib_reference = 2019A&A...625A...2K bib_reference_url = https://doi.org/10.1051/0004-6361/201834918 obs_copyright = All data in the ESO archive retain ESO's copyright, and are distributed according to the terms of the Creative Commons Attribution 4.0 International license (CC BY 4.0). obs_copyright_url = http://archive.eso.org/cms/eso-data-access-policy.html t_min = 55782 t_max = 58690 obs_regime = Optical em_min = 3.91271e-7 em_max = 8.74145e-7 client_category = Image/Optical/KiDS hips_builder = Aladin/HipsGen v12.055 hips_version = 1.4 hips_release_date = 2023-05-03T13:16Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_pixel_scale = 5.591E-5 dataproduct_type = image hips_rgb_red = i [lupton min=-1.5E-12 scale=3.75E9 Q=100.0] hips_rgb_green = r [lupton min=-2.0E-12 scale=5.0E9 Q=100.0] hips_rgb_blue = g [lupton min=-3.0E-12 scale=7.5E9 Q=100.0] hipsgen_date = 2023-03-27T12:57Z hipsgen_params = -maxthread=16 mode=keeptile inred=iHiPS ingreen=rHiPS inblue=gHiPS color=png luptonM=-1.5e-12/-2e-12/-3e-12 luptonS=3.75e9/5e9/7.5e9 luptonQ=100 out=griHiPS id=KiDS/gri RGB hips_creation_date = 2023-03-27T12:57Z hips_overlay = overlayMean mergeOverwriteTile treeMedian hips_tile_format = png moc_sky_fraction = 0.03263 hips_estsize = 1132970166 hips_nb_tiles = 2196061 dataproduct_subtype = color hips_check_code = png:1146781870 hips_service_url = https://alasky.cds.unistra.fr/KiDS/CDS_P_KiDS_DR5_color-gri hips_service_url_1 = https://alaskybis.cds.unistra.fr/KiDS/CDS_P_KiDS_DR5_color-gri hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 50.32083 obs_initial_dec = -27.1722 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288495282 ID = CDS/P/KiDS/DR5/color-ug hips_initial_ra = 50.32083 hips_initial_dec = -27.1722 hips_initial_fov = 0.3 creator_did = ivo://CDS/P/KiDS/DR5/color-ug hips_creator = Kuijken K. (KiDS team) obs_title = KiDS color ug obs_collection = KiDS prov_progenitor = ESO Science Archive obs_description = The Kilo-Degree Survey (KiDS) covers 1346 square degrees of sky in u,g,r,i bands, and was primarily designed for weak gravitational lensing studies. It used the OmegaCAM instrument on the VLT Survey Telescope on Paranal, and took data between 2011 and 2019. These colour images are from the final data release, DR5, and are being made available pre-publication. Description of the data reduction procedures can be found in the DR4 release paper, and will be updated, together with the corresponding FITS files, in due course. bib_reference = 2019A&A...625A...2K bib_reference_url = https://doi.org/10.1051/0004-6361/201834918 obs_copyright = All data in the ESO archive retain ESO's copyright, and are distributed according to the terms of the Creative Commons Attribution 4.0 International license (CC BY 4.0). obs_copyright_url = http://archive.eso.org/cms/eso-data-access-policy.html t_min = 55798 t_max = 58690 obs_regime = Optical em_min = 3.20744e-7 em_max = 5.57293e-7 client_category = Image/Optical/KiDS hips_builder = Aladin/HipsGen v12.055 hips_version = 1.4 hips_release_date = 2023-05-03T15:13Z hips_frame = equatorial hips_order = 10 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_pixel_scale = 1.118E-4 dataproduct_type = image hips_rgb_red = g [lupton min=-1.0E-12 scale=1.0E10 Q=100.0] hips_rgb_blue = u [lupton min=-3.0E-12 scale=3.0E10 Q=100.0] hipsgen_date = 2023-03-27T13:07Z hipsgen_params = -maxthread=5 mode=keeptile -order=10 inred=gHiPS inblue=uHiPS color=png luptonM=-1e-12//-3e-12 luptonS=1e10//3e10 luptonQ=100 out=ugHiPS id=KiDS/ug RGB hips_creation_date = 2023-03-27T13:07Z hips_overlay = overlayMean mergeOverwriteTile treeMedian hips_tile_format = png moc_sky_fraction = 0.03286 hips_estsize = 280700059 hips_nb_tiles = 554594 dataproduct_subtype = color hips_check_code = png:795716704 hips_service_url = https://alasky.cds.unistra.fr/KiDS/CDS_P_KiDS_DR5_color-ug hips_service_url_1 = https://alaskybis.cds.unistra.fr/KiDS/CDS_P_KiDS_DR5_color-ug hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 10 obs_initial_ra = 50.32083 obs_initial_dec = -27.1722 obs_initial_fov = 0.057258106863623426 TIMESTAMP = 1721288495202 ID = CDS/P/KiDZ/DR5/color-gri hips_initial_ra = 33.6611000 hips_initial_dec = -4.5704999 hips_initial_fov = 0.15 creator_did = ivo://CDS/P/KiDZ/DR5/color-gri hips_creator = Kuijken K. (KiDS team) obs_title = KiDZ color gri obs_collection = KiDS prov_progenitor = ESO Science Archive obs_description = The KiDZ data are complementary to the main Kilo-Degree (KIDS) survey, and specifically target fields with extensive deep spectroscopy. They are primarily intended for the calibration of photometric redshifts of galaxies. bib_reference = 2019A&A...625A...2K bib_reference_url = https://doi.org/10.1051/0004-6361/201834918 obs_copyright = All data in the ESO archive retain ESO?s copyright, and are distributed according to the terms of the Creative Commons Attribution 4.0 International license (CC BY 4.0). obs_copyright_url = http://archive.eso.org/cms/eso-data-access-policy.html t_min = 55782 t_max = 58690 obs_regime = Optical em_min = 3.91271e-7 em_max = 8.74145e-7 client_category = Image/Optical/KiDS hips_builder = Aladin/HipsGen v12.055 hips_version = 1.4 hips_release_date = 2023-05-11T12:50Z hips_frame = equatorial hips_order = 11 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_pixel_scale = 5.591E-5 dataproduct_type = image hips_rgb_red = kidz-i [lupton min=-1.5E-12 scale=3.75E9 Q=100.0] hips_rgb_green = kidz-r [lupton min=-2.0E-12 scale=5.0E9 Q=100.0] hips_rgb_blue = kidz-g [lupton min=-3.0E-12 scale=7.5E9 Q=100.0] hipsgen_date = 2023-04-25T14:45Z hipsgen_params = -maxthread=20 mode=keeptile inred=ziHiPS ingreen=zrHiPS inblue=zgHiPS color=png luptonM=-1.5e-12/-2e-12/-3e-12 luptonS=3.75e9/5e9/7.5e9 luptonQ=100 out=zgriHiPS id=KiDZ/gri RGB hips_creation_date = 2023-04-25T14:45Z hips_overlay = overlayMean mergeOverwriteTile treeMedian hips_tile_format = png moc_sky_fraction = 5.795E-4 hips_estsize = 19291674 hips_nb_tiles = 39708 dataproduct_subtype = color hips_check_code = png:3446861131 hips_service_url = https://alasky.cds.unistra.fr/KiDS/CDS_P_KiDZ_DR5_color-gri hips_service_url_1 = https://alaskybis.cds.unistra.fr/KiDS/CDS_P_KiDZ_DR5_color-gri hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 11 obs_initial_ra = 33.6611000 obs_initial_dec = -4.5704999 obs_initial_fov = 0.028629053431811713 TIMESTAMP = 1721288495418 ID = CDS/P/KiDZ/DR5/color-ug hips_initial_ra = 33.6611000 hips_initial_dec = -4.5704999 hips_initial_fov = 0.15 creator_did = ivo://CDS/P/KiDZ/DR5/color-ug hips_creator = Kuijken K. (KiDS team) obs_title = KiDZ color ug obs_collection = KiDS prov_progenitor = ESO Science Archive obs_description = The KiDZ data are complementary to the main Kilo-Degree (KIDS) survey, and specifically target fields with extensive deep spectroscopy. They are primarily intended for the calibration of photometric redshifts of galaxies. bib_reference = 2019A&A...625A...2K bib_reference_url = https://doi.org/10.1051/0004-6361/201834918 obs_copyright = All data in the ESO archive retain ESO?s copyright, and are distributed according to the terms of the Creative Commons Attribution 4.0 International license (CC BY 4.0). obs_copyright_url = http://archive.eso.org/cms/eso-data-access-policy.html t_min = 55798 t_max = 58690 obs_regime = Optical em_min = 3.20744e-7 em_max = 5.57293e-7 client_category = Image/Optical/KiDS hips_builder = Aladin/HipsGen v12.055 hips_version = 1.4 hips_release_date = 2023-05-11T12:53Z hips_frame = equatorial hips_order = 10 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_pixel_scale = 1.118E-4 dataproduct_type = image hips_rgb_red = kidz-g [lupton min=-1.0E-12 scale=1.0E10 Q=100.0] hips_rgb_blue = kidz-u [lupton min=-3.0E-12 scale=3.0E10 Q=100.0] hipsgen_date = 2023-04-25T13:22Z hipsgen_params = -maxthread=5 mode=keeptile -order=10 inred=zgHiPS inblue=zuHiPS color=png luptonM=-1e-12//-3e-12 luptonS=1e10//3e10 luptonQ=100 out=zugHiPS id=KiDZ/ug RGB hips_creation_date = 2023-04-25T13:22Z hips_overlay = overlayMean mergeOverwriteTile treeMedian hips_tile_format = png moc_sky_fraction = 6.170E-4 hips_estsize = 4802502 hips_nb_tiles = 10836 dataproduct_subtype = color hips_check_code = png:717930885 hips_service_url = https://alasky.cds.unistra.fr/KiDS/CDS_P_KiDZ_DR5_color-ug hips_service_url_1 = https://alaskybis.cds.unistra.fr/KiDS/CDS_P_KiDZ_DR5_color-ug hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 10 obs_initial_ra = 33.6611000 obs_initial_dec = -4.5704999 obs_initial_fov = 0.057258106863623426 TIMESTAMP = 1721288495350 ID = CDS/P/MAMA/ColorEJ client_category = Image/Optical/MAMA creator_did = ivo://CDS/P/MAMA/ColorEJ obs_title = MAMA color composition (posse,srcj) obs_collection = MAMA Color obs_description = During the eighties and nineties, several thousands original photographic plates had been digitized with the MAMA microdensitometer and calibrated to meet the specific objectives of a number of national and international projects in a variety of scientific domains: clusters of galaxies, samples of quasar candidates, young stellar objects, variable stars, stellar populations in the solar neighbourhood, tidal effects on open and globular clusters, microlensing. More recently, our team (Observatoire de Paris) has undertaken digitizing and making available to the astronomical community three atlases: ESO-R and southern part of POSSI-E in the R band, SRC-J in the B band. hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra obs_ack = The project is conducted in partnership with the VO Paris Data Centre and the ALADIN group (CDS). prov_progenitor = VO Paris Data Centre bib_reference = 1988CRJS....9..122A bib_reference_url = http://adsabs.harvard.edu/abs/1988CRJS....9..122A obs_copyright = Observatoire de Paris obs_copyright_url = https://www.obspm.fr/mentions-legales.html?lang=en t_min = 41683 t_max = 46796 obs_regime = Optical em_min = 3.95E-7 em_max = 6.9E-7 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T06:24Z hips_frame = equatorial hips_order = 10 hips_tile_width = 512 hips_status = public master clonableOnce hips_pixel_scale = 1.118E-4 dataproduct_type = image hips_rgb_red = MAMA posse [263.91565582133546 NaN 1693.6855231833124 Linear] hips_rgb_blue = MAMA srcj [324.90647318898084 NaN 2206.099081736764 Linear] moc_sky_fraction = 0.3012 hips_estsize = 450964692 hipsgen_date = 2017-12-19T16:39Z hips_initial_fov = 1.1 hips_initial_ra = 274.5795184 hips_initial_dec = -11.8228963 hipsgen_params = inRed=/var/www/MAMA/CDS_P_MAMA_posse inBlue=/var/www/MAMA/CDS_P_MAMA_srcj "cmRed=0.2328 1.494" "cmBlue=0.2866 1.946" out=HIPS_MAMA_color_posse_srcj_new creator_did=CDS/P/MAMA/posse/Color region=/home/buga/CDS_P_MAMA_posse_MOC.fits color=png maxthread=16 RGB hips_creation_date = 2017-12-19T16:39Z hips_hierarchy = median hips_tile_format = png hipsgen_date_1 = 2017-12-20T16:11Z hipsgen_params_1 = inRed=/var/www/MAMA/CDS_P_MAMA_posse inBlue=/var/www/MAMA/CDS_P_MAMA_srcj "cmRed=0.2328 1.494" "cmBlue=0.2866 1.946" out=HIPS_MAMA_color_posse_srcj_new creator_did=CDS/P/MAMA/posse/Color region=/home/buga/CDS_P_MAMA_posse_MOC.fits color=png maxthread=16 RGB hips_order_min = 0 dataproduct_subtype = color hipsgen_date_2 = 2019-05-21T06:24Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/MAMA/CDS_P_MAMA_color_posse_srcj UPDATE hips_service_url = https://alasky.cds.unistra.fr/MAMA/CDS_P_MAMA_color_posse_srcj hips_service_url_1 = https://alaskybis.cds.unistra.fr/MAMA/CDS_P_MAMA_color_posse_srcj hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 10 obs_initial_ra = 274.5795184 obs_initial_dec = -11.8228963 obs_initial_fov = 0.057258106863623426 TIMESTAMP = 1721288464350 ID = CDS/P/MAMA/posse creator_did = ivo://CDS/P/MAMA/posse obs_collection = MAMA posse obs_title = MAMA posse obs_description = During the eighties and nineties, several thousands original photographic plates had been digitized with the MAMA microdensitometer and calibrated to meet the specific objectives of a number of national and international projects in a variety of scientific domains: clusters of galaxies, samples of quasar candidates, young stellar objects, variable stars, stellar populations in the solar neighbourhood, tidal effects on open and globular clusters, microlensing. More recently, our team (Observatoire de Paris) has undertaken digitizing and making available to the astronomical community three atlases: ESO-R and southern part of POSSI-E in the R band, SRC-J in the B band. obs_ack = The project is conducted in partnership with the VO Paris Data Centre and the ALADIN group (CDS). prov_progenitor = VO Paris Data Centre bib_reference = 1988CRJS....9..122A bib_reference_url = http://adsabs.harvard.edu/abs/1988CRJS....9..122A obs_copyright = Observatoire de Paris obs_copyright_url = https://www.obspm.fr/mentions-legales.html?lang=en t_min = 41683 t_max = 46796 obs_regime = Optical em_min = 6.1E-7 em_max = 6.9E-7 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T06:34Z hips_frame = equatorial hips_order = 10 hips_tile_width = 512 client_category = Image/Optical/MAMA hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = 0.2328 1.494 hips_data_range = -0.6691 2.286 hips_initial_ra = 274.6998723 hips_initial_dec = -13.8206118 hips_initial_fov = 2.5 hips_pixel_scale = 1.118E-4 s_pixel_scale = 1.865E-4 dataproduct_type = image moc_sky_fraction = 0.3012 hips_estsize = 2863914789 hipsgen_date = 2016-07-09T19:09Z hipsgen_params = in=posse out=HIPS_posse fov=true skyval=true border=100 ivorn=ivo://CDS/P/MAMA/posse Publisher=M.Buga [CDS] INDEX TILES DETAILS hips_creation_date = 2016-07-09T19:09Z hipsgen_date_1 = 2016-09-12T21:38Z hipsgen_params_1 = in=posse out=HIPS_posse ivorn=ivo://CDS/P/MAMA/posse Publisher=M.Buga [CDS] PNG hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra hips_order_min = 0 hips_pixel_bitpix = 16 hipsgen_date_2 = 2019-05-21T06:34Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/MAMA/CDS_P_MAMA_posse UPDATE hips_service_url = https://alasky.cds.unistra.fr/MAMA/CDS_P_MAMA_posse hips_progenitor_url = https://alasky.cds.unistra.fr/MAMA/CDS_P_MAMA_posse/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/MAMA/CDS_P_MAMA_posse hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 10 obs_initial_ra = 274.6998723 obs_initial_dec = -13.8206118 obs_initial_fov = 0.057258106863623426 TIMESTAMP = 1721288464590 ID = CDS/P/MAMA/srcj creator_did = ivo://CDS/P/MAMA/srcj obs_collection = MAMA srcj obs_title = MAMA srcj obs_description = During the eighties and nineties, several thousands original photographic plates had been digitized with the MAMA microdensitometer and calibrated to meet the specific objectives of a number of national and international projects in a variety of scientific domains: clusters of galaxies, samples of quasar candidates, young stellar objects, variable stars, stellar populations in the solar neighbourhood, tidal effects on open and globular clusters, microlensing. More recently, our team (Observatoire de Paris) has undertaken digitizing and making available to the astronomical community three atlases: ESO-R and southern part of POSSI-E in the R band, SRC-J in the B band. hips_pixel_bitpix = 16 data_pixel_bitpix = 16 hips_sampling = bilinear hips_skyval = hips_estimation hips_overlay = border_fading hips_hierarchy = median hips_creator = Buga M. (CDS) hips_copyright = CNRS/Unistra obs_ack = The project is conducted in partnership with the VO Paris Data Centre and the ALADIN group (CDS). prov_progenitor = VO Paris Data Centre bib_reference = 1988CRJS....9..122A bib_reference_url = http://adsabs.harvard.edu/abs/1988CRJS....9..122A obs_copyright = Observatoire de Paris obs_copyright_url = https://www.obspm.fr/mentions-legales.html?lang=en t_min = 41683 t_max = 46796 obs_regime = Optical em_min = 3.95E-7 em_max = 5.4E-7 hips_builder = Aladin/HipsGen v10.125 hips_version = 1.4 hips_release_date = 2019-05-21T06:26Z hips_frame = equatorial hips_order = 10 hips_tile_width = 512 client_category = Image/Optical/MAMA hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = 0.2937 2.08 hips_data_range = -0.9121 3.551 hips_initial_ra = 160.9123191 hips_initial_dec = -59.7706835 hips_initial_fov = 4.5 hips_pixel_scale = 1.118E-4 s_pixel_scale = 1.864E-4 dataproduct_type = image moc_sky_fraction = 0.5241 hips_estsize = 4984548162 hips_creation_date = 2016-06-19T14:24Z hipsgen_date = 2016-06-19T14:24Z hipsgen_params = in=srcj out=HIPS_srcj fov=true skyval=true border=2000 ivorn=ivo://CDS/P/MAMA/srcj Publisher="M.Buga [CDS] INDEX TILES DETAILS hipsgen_date_1 = 2016-06-30T05:19Z hipsgen_params_1 = in=srcj out=HIPS_srcj fov=true skyval=true border=2000 ivorn=ivo://CDS/P/MAMA/srcj Publisher="M.Buga [CDS]" PNG hips_order_min = 0 hipsgen_date_2 = 2019-05-21T06:26Z hipsgen_params_2 = out=/asd-volumes/sc1-asd-volume6/MAMA/CDS_P_MAMA_srcj UPDATE hips_service_url = https://alasky.cds.unistra.fr/MAMA/CDS_P_MAMA_srcj hips_progenitor_url = https://alasky.cds.unistra.fr/MAMA/CDS_P_MAMA_srcj/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/MAMA/CDS_P_MAMA_srcj hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 10 obs_initial_ra = 160.9123191 obs_initial_dec = -59.7706835 obs_initial_fov = 0.057258106863623426 TIMESTAMP = 1721288464430 ID = CDS/P/MATLAS/color hips_initial_fov = 0.4 hips_initial_ra = 29.8068442 hips_initial_dec = 18.9546447 creator_did = ivo://CDS/P/MATLAS/color hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = mean hips_creator = Boch T. (CDS) hips_copyright = CNRS / Universite de Strasbourg obs_title = MATLAS color (filters i, r, g) obs_collection = MATLAS obs_description = MATLAS (Mass Assembly of early-Type GaLAxies with their fine Structures) investigates the mass assembly of Early-Type Galaxies (ETGs) and the build-up of their scaling relations, with extremely deep optical images. The stellar populations in the outermost regions of ETGs, the fine structures (tidal tails, stellar stream, and shells) around them, the Globular Cluster (GCs) and dwarf satellites, preserve a record of past merger events and more generally of the evolution and transformation of galaxies. The MATLAS color HiPS has been generated from i, r, g HiPS. obs_ack = MATLAS collaboration bib_reference = 2020MNRAS.498.2138B bib_reference_url = https://ui.adsabs.harvard.edu/abs/2020MNRAS.498.2138B/ obs_copyright = Duc/ObAS/AIM/CFHT obs_copyright_url = http://obas-matlas.u-strasbg.fr/ t_min = 54858 t_max = 57196 obs_regime = Optical em_min = 3.93888e-7 em_max = 8.63094e-7 client_category = Image/Optical/MATLAS hips_builder = Aladin/HipsGen v11.025 hips_version = 1.4 hips_release_date = 2020-12-15T13:17Z hips_frame = equatorial hips_order = 12 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png hips_pixel_scale = 0.229 s_pixel_scale = 5.164E-5 dataproduct_type = image dataproduct_subtype = color moc_sky_fraction = 0.007406 hips_estsize = 8 hipsgen_date = 2020-12-11T09:27Z hipsgen_params = tiles hips_creation_date = 2020-12-11T09:27Z hipsgen_date_1 = 2020-12-11T17:24Z hipsgen_params_1 = tiles hipsgen_date_2 = 2020-12-13T14:53Z hipsgen_params_2 = tiles hipsgen_date_3 = 2020-12-15T09:32Z hipsgen_params_3 = out=old_hips/CDS_P_MATLAS_color ALLSKY hipsgen_date_4 = 2020-12-15T09:33Z hipsgen_params_4 = out=old_hips/CDS_P_MATLAS_color tree hipsgen_date_5 = 2020-12-15T09:43Z hipsgen_params_5 = out=old_hips/CDS_P_MATLAS_color tree hipsgen_date_6 = 2020-12-15T09:44Z hipsgen_params_6 = out=old_hips/CDS_P_MATLAS_color allsky hipsgen_date_7 = 2020-12-15T09:44Z hipsgen_params_7 = out=old_hips/CDS_P_MATLAS_color allsky hipsgen_date_8 = 2020-12-15T11:04Z hipsgen_params_8 = out=old_hips/CDS_P_MATLAS_color ALLSKY hipsgen_date_9 = 2020-12-15T11:05Z hipsgen_params_9 = out=old_hips/CDS_P_MATLAS_color verbose=4 ALLSKY hipsgen_date_10 = 2020-12-15T11:06Z hipsgen_params_10 = out=old_hips/CDS_P_MATLAS_color verbose=4 ALLSKY hipsgen_date_11 = 2020-12-15T13:14Z hipsgen_params_11 = out=old_hips/CDS_P_MATLAS_color verbose=4 ALLSKY -f hipsgen_date_12 = 2020-12-15T13:17Z hipsgen_params_12 = out=old_hips/CDS_P_MATLAS_color color=png ALLSKY hips_service_url = https://alasky.cds.unistra.fr/MATLAS/CDS_P_MATLAS_color hips_service_url_1 = https://alaskybis.cds.unistra.fr/MATLAS/CDS_P_MATLAS_color hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 12 obs_initial_ra = 29.8068442 obs_initial_dec = 18.9546447 obs_initial_fov = 0.014314526715905856 TIMESTAMP = 1721288489382 ID = CDS/P/MATLAS/g hips_initial_fov = 0.4 hips_initial_ra = 29.8068442 hips_initial_dec = 18.9546447 creator_did = ivo://CDS/P/MATLAS/g hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = mean hips_creator = Boch T. (CDS) hips_copyright = CNRS / Universite de Strasbourg obs_title = MATLAS g obs_collection = MATLAS obs_description = MATLAS (Mass Assembly of early-Type GaLAxies with their fine Structures) investigates the mass assembly of Early-Type Galaxies (ETGs) and the build-up of their scaling relations, with extremely deep optical images. The stellar populations in the outermost regions of ETGs, the fine structures (tidal tails, stellar stream, and shells) around them, the Globular Cluster (GCs) and dwarf satellites, preserve a record of past merger events and more generally of the evolution and transformation of galaxies. obs_ack = MATLAS collaboration bib_reference = 2020MNRAS.498.2138B bib_reference_url = https://ui.adsabs.harvard.edu/abs/2020MNRAS.498.2138B/ obs_copyright = Duc/ObAS/AIM/CFHT obs_copyright_url = http://obas-matlas.u-strasbg.fr/ t_min = 54858 t_max = 57184 obs_regime = Optical em_min = 3.93888e-7 em_max = 5.57092e-7 client_category = Image/Optical/MATLAS hips_builder = Aladin/HipsGen v11.025 hips_version = 1.4 hips_release_date = 2020-12-29T19:22Z hips_frame = equatorial hips_order = 12 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = fits png hips_pixel_cut = -0.5 200 hips_data_range = -3472 8483 hips_pixel_scale = 2.795E-5 s_pixel_scale = 5.164E-5 dataproduct_type = image moc_sky_fraction = 0.007461 hips_estsize = 2211375805 hipsgen_date = 2020-12-15T07:13Z hipsgen_params = tiles hips_creation_date = 2020-12-15T07:13Z hipsgen_date_1 = 2020-12-15T07:19Z hipsgen_params_1 = png hipsgen_date_2 = 2020-12-15T07:21Z hipsgen_params_2 = tiles hipsgen_date_3 = 2020-12-29T11:42Z hipsgen_params_3 = png -f hips_service_url = https://alasky.cds.unistra.fr/MATLAS/CDS_P_MATLAS_g hips_service_url_1 = https://alaskybis.cds.unistra.fr/MATLAS/CDS_P_MATLAS_g hips_status_1 = public mirror clonableOnce TIMESTAMP = 1721288489142 ID = CDS/P/MATLAS/i hips_initial_fov = 0.4 hips_initial_ra = 29.8068442 hips_initial_dec = 18.9546447 creator_did = ivo://CDS/P/MATLAS/i hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = mean hips_creator = Boch T. (CDS) hips_copyright = CNRS / Universite de Strasbourg obs_title = MATLAS i obs_collection = MATLAS obs_description = MATLAS (Mass Assembly of early-Type GaLAxies with their fine Structures) investigates the mass assembly of Early-Type Galaxies (ETGs) and the build-up of their scaling relations, with extremely deep optical images. The stellar populations in the outermost regions of ETGs, the fine structures (tidal tails, stellar stream, and shells) around them, the Globular Cluster (GCs) and dwarf satellites, preserve a record of past merger events and more generally of the evolution and transformation of galaxies. obs_ack = MATLAS collaboration bib_reference = 2020MNRAS.498.2138B bib_reference_url = https://ui.adsabs.harvard.edu/abs/2020MNRAS.498.2138B/ obs_copyright = Duc/ObAS/AIM/CFHT obs_copyright_url = http://obas-matlas.u-strasbg.fr/ t_min = 54949 t_max = 57169 obs_regime = Optical em_min = 6.91151e-7 em_max = 8.63094e-7 client_category = Image/Optical/MATLAS hips_builder = Aladin/HipsGen v11.025 hips_version = 1.4 hips_release_date = 2020-12-30T06:05Z hips_frame = equatorial hips_order = 12 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = fits png hips_pixel_cut = -0.5 200 hips_data_range = -7252 21266 hips_pixel_scale = 2.795E-5 s_pixel_scale = 5.193E-5 dataproduct_type = image moc_sky_fraction = 0.003943 hips_estsize = 1168594490 hipsgen_date = 2020-12-16T13:03Z hipsgen_params = tiles -f hips_creation_date = 2020-12-16T13:03Z hipsgen_date_1 = 2020-12-30T02:55Z hipsgen_params_1 = png -f hips_service_url = https://alasky.cds.unistra.fr/MATLAS/CDS_P_MATLAS_i hips_service_url_1 = https://alaskybis.cds.unistra.fr/MATLAS/CDS_P_MATLAS_i hips_status_1 = public mirror clonableOnce TIMESTAMP = 1721288489330 ID = CDS/P/MATLAS/r hips_initial_fov = 0.4 hips_initial_ra = 29.8068442 hips_initial_dec = 18.9546447 creator_did = ivo://CDS/P/MATLAS/r hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = mean hips_creator = Boch T. (CDS) hips_copyright = CNRS / Universite de Strasbourg obs_title = MATLAS r obs_collection = MATLAS obs_description = MATLAS (Mass Assembly of early-Type GaLAxies with their fine Structures) investigates the mass assembly of Early-Type Galaxies (ETGs) and the build-up of their scaling relations, with extremely deep optical images. The stellar populations in the outermost regions of ETGs, the fine structures (tidal tails, stellar stream, and shells) around them, the Globular Cluster (GCs) and dwarf satellites, preserve a record of past merger events and more generally of the evolution and transformation of galaxies. obs_ack = MATLAS collaboration bib_reference = 2020MNRAS.498.2138B bib_reference_url = https://ui.adsabs.harvard.edu/abs/2020MNRAS.498.2138B/ obs_copyright = Duc/ObAS/AIM/CFHT obs_copyright_url = http://obas-matlas.u-strasbg.fr/ t_min = 54858 t_max = 57196 obs_regime = Optical em_min = 5.61481e-7 em_max = 7.21806e-7 client_category = Image/Optical/MATLAS hips_builder = Aladin/HipsGen v11.025 hips_version = 1.4 hips_release_date = 2020-12-30T02:53Z hips_frame = equatorial hips_order = 12 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_pixel_cut = -0.5 200 hips_data_range = -5303 12718 hips_pixel_scale = 2.795E-5 s_pixel_scale = 5.164E-5 dataproduct_type = image hipsgen_date = 2020-12-15T08:39Z hipsgen_params = "region=7/54047,7/54090" tiles hips_creation_date = 2020-12-15T08:39Z hips_tile_format = fits png moc_sky_fraction = 0.007488 hips_estsize = 2219339149 hipsgen_date_1 = 2020-12-15T13:24Z hipsgen_params_1 = tiles hipsgen_date_2 = 2020-12-15T13:28Z hipsgen_params_2 = tiles hipsgen_date_3 = 2020-12-15T23:58Z hipsgen_params_3 = tiles -f hipsgen_date_4 = 2020-12-29T19:27Z hipsgen_params_4 = png -f hips_service_url = https://alasky.cds.unistra.fr/MATLAS/CDS_P_MATLAS_r hips_service_url_1 = https://alaskybis.cds.unistra.fr/MATLAS/CDS_P_MATLAS_r hips_status_1 = public mirror clonableOnce TIMESTAMP = 1721288489230 ID = CDS/P/MSX/A hips_initial_fov = 25 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 creator_did = ivo://CDS/P/MSX/A client_category = Image/Infrared/MSX hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = mean hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = MSX A (8.28 um) obs_collection = MSX obs_description = Midcourse Space Experiment (MSX) obs_ack = This research made use of data products from the Midcourse Space Experiment. Processing of the data was funded by the Ballistic Missile Defense Organization with additional support from NASA Office of Space Science. This research has also made use of the NASA/ IPAC Infrared Science Archive, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. prov_progenitor = https://irsa.ipac.caltech.edu/data/MSX/images/ bib_reference = 1997AAS...191.5005P obs_copyright_url = https://irsa.ipac.caltech.edu/Missions/msx.html t_min = 50221.5 t_max = 50499.5 obs_regime = Infrared em_min = 5.972142e-6 em_max = 11.085209e-6 hips_builder = Aladin/HipsGen v11.025 hips_version = 1.4 hips_release_date = 2020-11-25T08:38Z hips_frame = equatorial hips_order = 7 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = 1.0E-9 5.0E-5 hips_data_range = -7.491E-5 2.180E-4 hips_pixel_scale = 8.946E-4 s_pixel_scale = 0.001667 dataproduct_type = image moc_sky_fraction = 0.1454 hips_estsize = 42091333 hipsgen_date = 2020-11-25T08:37Z hipsgen_params = TILES hips_creation_date = 2020-11-25T08:37Z hipsgen_date_1 = 2020-11-25T08:38Z hipsgen_params_1 = PNG hips_service_url = https://alasky.cds.unistra.fr/MSX/CDS_P_MSX_A hips_progenitor_url = https://alasky.cds.unistra.fr/MSX/CDS_P_MSX_A/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/MSX/CDS_P_MSX_A hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 7 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288488322 ID = CDS/P/MSX/C hips_initial_fov = 25 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 creator_did = ivo://CDS/P/MSX/C client_category = Image/Infrared/MSX hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = mean hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = MSX C (12.13 um) obs_collection = MSX obs_description = Midcourse Space Experiment (MSX) obs_ack = This research made use of data products from the Midcourse Space Experiment. Processing of the data was funded by the Ballistic Missile Defense Organization with additional support from NASA Office of Space Science. This research has also made use of the NASA/ IPAC Infrared Science Archive, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. prov_progenitor = https://irsa.ipac.caltech.edu/data/MSX/images/ bib_reference = 1997AAS...191.5005P obs_copyright_url = https://irsa.ipac.caltech.edu/Missions/msx.html t_min = 50221.5 t_max = 50499.5 obs_regime = Infrared em_min = 10.987116e-6 em_max = 13.338167e-6 hips_builder = Aladin/HipsGen v11.025 hips_version = 1.4 hips_release_date = 2020-11-25T09:15Z hips_frame = equatorial hips_order = 7 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = 1.0E-9 5.0E-5 hips_data_range = -2.025E-5 2.196E-5 hips_pixel_scale = 8.946E-4 s_pixel_scale = 0.001667 dataproduct_type = image moc_sky_fraction = 0.1457 hips_estsize = 42159056 hipsgen_date = 2020-11-25T09:14Z hipsgen_params = TILES hips_creation_date = 2020-11-25T09:14Z hipsgen_date_1 = 2020-11-25T09:15Z hipsgen_params_1 = PNG hips_service_url = https://alasky.cds.unistra.fr/MSX/CDS_P_MSX_C hips_progenitor_url = https://alasky.cds.unistra.fr/MSX/CDS_P_MSX_C/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/MSX/CDS_P_MSX_C hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 7 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288488382 ID = CDS/P/MSX/D hips_initial_fov = 25 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 creator_did = ivo://CDS/P/MSX/D client_category = Image/Infrared/MSX hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = mean hips_creator = Boch T. (CDS) hips_copyright = CNRS/Universite de Strasbourg obs_title = MSX D (14.65 um) obs_collection = MSX obs_description = Midcourse Space Experiment (MSX) obs_ack = This research made use of data products from the Midcourse Space Experiment. Processing of the data was funded by the Ballistic Missile Defense Organization with additional support from NASA Office of Space Science. This research has also made use of the NASA/ IPAC Infrared Science Archive, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. prov_progenitor = https://irsa.ipac.caltech.edu/data/MSX/images/ bib_reference = 1997AAS...191.5005P obs_copyright_url = https://irsa.ipac.caltech.edu/Missions/msx.html t_min = 50221.5 t_max = 50499.5 obs_regime = Infrared em_min = 13.137137e-6 em_max = 16.205789e-6 hips_builder = Aladin/HipsGen v11.025 hips_version = 1.4 hips_release_date = 2020-11-25T10:47Z hips_frame = equatorial hips_order = 7 hips_order_min = 0 hips_tile_width = 512 hips_status = public master clonableOnce hips_tile_format = png fits hips_pixel_cut = 1.0E-9 5.0E-5 hips_data_range = -3.073E-5 7.325E-5 hips_pixel_scale = 8.946E-4 s_pixel_scale = 0.001667 dataproduct_type = image moc_sky_fraction = 0.1434 hips_estsize = 41520104 hipsgen_date = 2020-11-25T10:47Z hipsgen_params = TILES hips_creation_date = 2020-11-25T10:47Z hipsgen_date_1 = 2020-11-25T10:47Z hipsgen_params_1 = PNG hips_service_url = https://alasky.cds.unistra.fr/MSX/CDS_P_MSX_D hips_progenitor_url = https://alasky.cds.unistra.fr/MSX/CDS_P_MSX_D/HpxFinder hips_service_url_1 = https://alaskybis.cds.unistra.fr/MSX/CDS_P_MSX_D hips_status_1 = public mirror clonableOnce moc_type = stmoc moc_time_order = 25 moc_time_range = 1 moc_order = 7 obs_initial_ra = 266.4168166 obs_initial_dec = -29.0078249 obs_initial_fov = 0.4580648549089874 TIMESTAMP = 1721288488454 ID = CDS/P/MSX/E hips_initial_fov = 25 hips_initial_ra = 266.4168166 hips_initial_dec = -29.0078249 creator_did = ivo://CDS/P/MSX/E client_category = Image/Infrared/MSX hips_pixel_bitpix = -32 data_pixel_bitpix = -32 hips_sampling = bilinear hips_overlay = mean hips_hierarchy = mean hips_creator = Boch T. (CDS) hips_copyright