ID                   = CDS/P/2MASS/H
hips_doi             = 10.26093/cds/aladin/2thy-66
creator_did          = ivo://CDS/P/2MASS/H
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hips_sampling        = bilinear
hips_skyval_method   = SKYVAL
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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
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moc_time_range       = 1
moc_order            = 9
obs_initial_ra       = 266.40499479
obs_initial_dec      = -28.936173970
obs_initial_fov      = 0.11451621372724685
TIMESTAMP            = 1699689866896
,
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
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hips_sampling        = bilinear
hips_skyval_method   = SKYVAL
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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
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obs_regime           = Infrared
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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
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hips_status_1        = public mirror clonableOnce
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moc_type             = stmoc
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,
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hips_doi             = 10.26093/cds/aladin/2ea3-abw
creator_did          = ivo://CDS/P/2MASS/K
hips_initial_ra      = 266.40499479
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hips_sampling        = bilinear
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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
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hips_order_min       = 0
hips_tile_width      = 512
dataproduct_type     = image
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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
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em_min               = 2.015E-6
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hips_pixel_scale     = 2.236E-4
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moc_sky_fraction     = 1
hips_estsize         = 4706425658
hips_creation_date   = 2013-01-14T09:45Z
hipsgen_date         = 2020-08-04T10:56Z
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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
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obs_initial_fov      = 0.11451621372724685
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,
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
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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. (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         = Aladin/HipsGen v11.023
hips_version         = 1.4
hips_release_date    = 2021-02-24T03:22Z
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
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hips_rgb_green       = 2MASSh [1.0 20.0 100.0 Log]
hips_rgb_blue        = 2MASS J [-0.5 20.0 40.0 Log]
moc_sky_fraction     = 1
hips_estsize         = 75160788
hipsgen_date         = 2020-10-01T09:28Z
hipsgen_params       = inRed=Hips-K2 inBlue=Hips-J2 inGreen=Hips-H out=Hips-Color5 creator_did=ivo://CDS-test/P/2MASS/Color skyval=SKYVAL "fitskeys=ORDATE SCANNO SCANDIR" maxthread=64 hips_frame=equatorial "cmRed=-0.5 20 40 log" "cmBlue=-0.5 20 40 log" "cmGreen=1 20 100 log" color=jpeg RGB
hips_creation_date   = 2012-02-24T12:43Z
hips_tile_format     = jpeg
hipsgen_date_1       = 2020-10-12T12:49Z
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hips_hierarchy       = median
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
hips_service_url_2   = https://casda.csiro.au/hips/2MASS/Color
hips_status_2        = public mirror unclonable
hips_service_url_3   = https://irsa.ipac.caltech.edu/data/hips/CDS/2MASS/Color
hips_status_3        = public mirror unclonable
hips_service_url_4   = https://healpix.ias.u-psud.fr/CDS_P_2MASS_color
hips_status_4        = public mirror unclonable
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moc_time_order       = 25
moc_time_range       = 1
moc_order            = 9
obs_initial_ra       = 266.40499479
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obs_initial_fov      = 0.11451621372724685
TIMESTAMP            = 1711279617991
,
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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)
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hips_order           = 5
hips_frame           = equatorial
hips_tile_width      = 512
hips_tile_format     = png jpeg
dataproduct_type     = image
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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
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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
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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            = 1711279428544
,
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            = 1701982996993
,
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            = 1712902101704
,
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            = 1701982997197
,
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            = 1701982997329
,
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            = 1701982998717
,
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 ŕ partir des gravures du moine cartographe Vincenzo Coronelli.
obs_copyright        = Jean-Pierre Rosenkranz, Bibliothčque 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            = 1696351649854
,
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            = 1699603388664
,
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            = 1701983071905
,
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            = 1702506004592
,
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            = 1701983072053
,
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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            = 1691097259681
,
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            = 1696351647298
,
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            = 1696351647618
,
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            = 1696351637226
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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            = 1696351647098
,
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)
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hips_creator         = Boch T. (CDS)
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hips_copyright       = © Université de Strasbourg - CNRS. All rights reserved
obs_copyright        = © Université de Strasbourg - CNRS. All rights reserved
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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
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hips_creation_date   = 2023-01-30T07:50Z
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hips_copyright       = © Université de Strasbourg - CNRS. All rights reserved
obs_copyright        = © Université de Strasbourg - CNRS. All rights reserved
hips_initial_fov     = 58.63230142835039
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hips_service_url     = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/Infrared
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hips_copyright       = © Université de Strasbourg - CNRS. All rights reserved
obs_copyright        = © Université de Strasbourg - CNRS. All rights reserved
hips_initial_fov     = 58.63230142835039
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hips_creation_date   = 2023-01-30T07:50Z
hips_service_url     = https://alasky.cds.unistra.fr/ancillary/simbad-biblio/Nebula
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hips_copyright       = © Université de Strasbourg - CNRS. All rights reserved
obs_copyright        = © Université de Strasbourg - CNRS. All rights reserved
hips_initial_fov     = 58.63230142835039
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hips_initial_dec     = +0
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hips_copyright       = © Université de Strasbourg - CNRS. All rights reserved
obs_copyright        = © Université de Strasbourg - CNRS. All rights reserved
hips_initial_fov     = 58.63230142835039
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hips_initial_dec     = +0
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hips_copyright       = © Université de Strasbourg - CNRS. All rights reserved
obs_copyright        = © Université de Strasbourg - CNRS. All rights reserved
hips_initial_fov     = 58.63230142835039
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hips_initial_dec     = +0
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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            = 1696438180162
,
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            = 1701983035141
,
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            = 1701982998873
,
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            = 1711279618819
,
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            = 1701983439243
,
ID                   = CDS/P/EGRET/Dif/100-150
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            = 1691097205133
,
ID                   = CDS/P/EGRET/Dif/1000-2000
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            = 1691097205181
,
ID                   = CDS/P/EGRET/Dif/150-300
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            = 1691097205225
,
ID                   = CDS/P/EGRET/Dif/2000-4000
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            = 1691097205289
,
ID                   = CDS/P/EGRET/Dif/30-50
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            = 1691097205341
,
ID                   = CDS/P/EGRET/Dif/300-500
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            = 1691097205389
,
ID                   = CDS/P/EGRET/Dif/4000-10000
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            = 1691097205441
,
ID                   = CDS/P/EGRET/Dif/50-70
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            = 1691097205489
,
ID                   = CDS/P/EGRET/Dif/500-1000
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            = 1691097205537
,
ID                   = CDS/P/EGRET/Dif/70-100
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            = 1691097205589
,
ID                   = CDS/P/EGRET/inf100
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            = 1691097205653
,
ID                   = CDS/P/EGRET/sup100
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            = 1691097205709
,
ID                   = CDS/P/Fermi/3
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            = 1696351581890
,
ID                   = CDS/P/Fermi/4
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            = 1696351581962
,
ID                   = CDS/P/Fermi/5
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            = 1696351582026
,
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]
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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
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dataproduct_subtype  = color
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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
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moc_time_order       = 25
moc_time_range       = 1
moc_order            = 3
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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
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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
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moc_order            = 3
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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_service_url     = https://alasky.cds.unistra.fr/GALEX/GR6-03-2014/AIS-FD
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.
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hips_pixel_bitpix    = -32
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hipsgen_params       = out=/asd-volumes/sc1-asd-volume10/GALEX/GR6-03-2014/AIS-FD UPDATE
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hips_status_1        = public mirror clonableOnce
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hips_status_2        = public mirror unclonable
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moc_order            = 8
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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
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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_service_url     = https://alasky.cds.unistra.fr/GALEX/GR6-03-2014/AIS-ND
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.
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hipsgen_params       = out=/asd-volumes/sc1-asd-volume10/GALEX/GR6-03-2014/AIS-ND UPDATE
hips_service_url_1   = https://alaskybis.cds.unistra.fr/GALEX/GR6-03-2014/AIS-ND
hips_status_1        = public mirror clonableOnce
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hips_status_2        = public mirror unclonable
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obs_collection       = GALEX Allsky Imaging Survey (AIS) colored
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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
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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
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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.
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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
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hips_status_2        = public mirror unclonable
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hips_status_3        = public mirror unclonable
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hips_copyright       = CNRS/Unistra
obs_title            = GALEXGR6_7 FUV
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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
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hips_version         = 1.4
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hips_frame           = equatorial
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hips_tile_format     = png fits
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hips_service_url_1   = https://alaskybis.cds.unistra.fr/GALEX/GALEXGR6_7_FUV
hips_status_1        = public mirror clonableOnce
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hips_doi             = 10.26093/cds/aladin/20ag-p3d
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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
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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
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obs_copyright        = STScI (NASA)
obs_copyright_url    = https://www.stsci.edu/copyright
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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
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obs_copyright        = STScI (NASA)
obs_copyright_url    = https://www.stsci.edu/copyright
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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/
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hips_status          = public master clonableOnce
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hips_status_1        = public mirror clonableOnce
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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/
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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/
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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/
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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
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,
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
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,
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            = 1696351628930
,
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
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,
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            = 1691097206373
,
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/ships_creator         = Buga M. (CDS)
hips_copyright       = CNRS/Unistra
obs_ack              = Benjamin Winkel, bwinkel(at)mpifr.de
prov_progenitor      = VizieR Service, CDS (ftp : J/A+A/594/A116/)
bib_reference        = 2016A&A...594A.116H
bib_reference_url    = https://ui.adsabs.harvard.edu/?#abs/2016A%26A...594A.116H
t_min                = 54812
t_max                = 56293
obs_regime           = Radio
em_min               = 0.21
em_max               = 0.21
hips_builder         = Aladin/HipsGen v10.125
hips_version         = 1.4
hips_release_date    = 2019-05-22T05:04Z
hips_frame           = galactic
hips_order           = 3
hips_tile_width      = 128
hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_bitpix    = -32
hips_pixel_cut       = 2.286E20 2.056E22
hips_data_range      = -1.433E22 3.660E22
hips_pixel_scale     = 0.05726
dataproduct_type     = image
moc_sky_fraction     = 1
hips_estsize         = 72690
hipsgen_date         = 2017-06-12T13:36Z
hips_initial_fov     = 120.0
hips_initial_ra      = 266.4168166
hips_initial_dec     = -29.0078249
hipsgen_params       = in=NHI_only_HPX.fits ivorn=ivo://CDS/P/HI4PI
hips_creation_date   = 2017-06-12T13:36Z
hipsgen_date_1       = 2017-06-12T13:36Z
hipsgen_params_1     = in=NHI_only_HPX.fits ivorn=ivo://CDS/P/HI4PI
hips_order_min       = 0
hipsgen_date_2       = 2019-05-22T05:04Z
hipsgen_params_2     = out=/asd-volumes/sc1-asd-volume6/HI4PI/P_HI4PI_NHI UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/HI4PI/P_HI4PI_NHI
hips_service_url_1   = https://alaskybis.cds.unistra.fr/HI4PI/P_HI4PI_NHI
hips_status_1        = public mirror clonableOnce
hips_service_url_2   = https://casda.csiro.au/hips/HI4PI/P_HI4PI_NHI
hips_status_2        = public mirror unclonable
hips_service_url_3   = http://skies.esac.esa.int/HI4PI
hips_status_3        = public mirror unclonable
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 8
obs_initial_ra       = 266.4168166
obs_initial_dec      = -29.0078249
obs_initial_fov      = 0.2290324274544937
TIMESTAMP            = 1706687273621
,
ID                   = CDS/P/HLA/H
hips_doi             = 10.26093/cds/aladin/2qxh-p7g
creator_did          = ivo://CDS/P/HLA/H
prov_did             = ivo://cadc.nrc.ca/hla
obs_collection       = HLA-H
obs_title            = HLA-H : F160W
obs_description      = The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F160W filter between the beginning of the mission  to the 4th of October 2014.The 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.  The Hubble Legacy Archive (HLA) is designed to optimize science from the Hubble Space Telescope by providing online, enhanced Hubble products and advanced browsing capabilities. The HLA is a joint project of the Space Telescope Science Institute (STScI), the Space Telescope European Coordinating Facility (ST-ECF), and the Canadian Astronomy Data Centre (CADC). Currently we have enhanced image products for ACS, WFPC2, WFC3, and NICMOS, extracted spectra from NICMOS and ACS grism observations.  The enhanced data products were generated from the standard HST pipeline products. The ACS, WFPC2, and WFC3, and NICMOS images have been combined using MultiDrizzle, are aligned north up , and, except for WFC3, have been astrometrically corrected when possible (for approximately 80% of the cases).  All HLA-produced images are in units of electrons/second, which for WFPC2 and NICMOS differs from calibration pipeline products; photometric zeropoints must be adjusted to reflect the units used.
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. "
hips_initial_fov     = 0.04893
hips_initial_ra      = 99.2681117
hips_initial_dec     = -75.3142555
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
prov_progenitor      = Canadian Astronomy Data Centre
t_min                = 50611.07373843
t_max                = 58020.25996528
obs_regime           = Infrared
client_category      = Image/Infrared/HST/HLA
em_min               = 1.3939e-06
em_max               = 1.8094e-06
hips_builder         = Aladin/HipsGen v12.044
hips_version         = 1.4
hips_release_date    = 2023-03-07T17:11Z
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       = -0.1 0.22
hips_data_range      = -15.58 46.75
hips_pixel_scale     = 1.397E-5
s_pixel_scale        = 2.5E-5
dataproduct_type     = image
moc_sky_fraction     = 3.290E-4
hipsgen_date         = 2018-04-11T15:08Z
hipsgen_params       = -maxThread=25 "-hips_creator=CADC (Daniel Durand)" -obs_title=H -in=filter_H_extract -force -blank=0 "-fitskeys=DSNAME INSTRUME OPT_ELE DETECTOR TIME_EXP PROP_ID PRODTYPE TARGNAME NMEMBERS OBS_DATE T_MIN T_MAX WAVE_MIN WAVE_MAX" -hips_order=13 -mocOrder=16 -out=filter_H_hips "-hips_pixel_cut=-0.1 0.22" -live -creator_did=CDS/P/HST/H
hips_creation_date   = 2018-04-11T15:08Z
hipsgen_date_1       = 2018-04-11T17:21Z
hipsgen_params_1     = -maxThread=25 "-hips_creator=CADC (Daniel Durand)" -obs_title=H -in=filter_H_extract -force -blank=0 "-fitskeys=DSNAME INSTRUME OPT_ELE DETECTOR TIME_EXP PROP_ID PRODTYPE TARGNAME NMEMBERS OBS_DATE T_MIN T_MAX WAVE_MIN WAVE_MAX" -hips_order=13 -mocOrder=16 -out=filter_H_hips "-hips_pixel_cut=-0.1 0.22" -live -creator_did=CDS/P/HST/H
hipsgen_date_2       = 2019-05-07T11:28Z
hipsgen_params_2     = out=/asd-volumes/sc1-asd-volume8/HLA-hips/filter_H_hips UPDATE
hipsgen_date_3       = 2023-03-07T17:11Z
hipsgen_params_3     = verbose=7 out=/var/www/HLA-hips/filter_H_hips "pixelCut=11% 99.9% byRegion log" maxThread=8 PNG
hips_service_url     = https://alasky.cds.unistra.fr/HLA-hips/filter_H_hips
hips_progenitor_url  = https://alasky.cds.unistra.fr/HLA-hips/filter_H_hips/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/HLA-hips/filter_H_hips
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 41
moc_time_range       = 14528
moc_order            = 13
obs_initial_ra       = 99.2681117
obs_initial_dec      = -75.3142555
obs_initial_fov      = 0.007157263357952928
TIMESTAMP            = 1702419525120
,
ID                   = CDS/P/HLA/I
hips_doi             = 10.26093/cds/aladin/3cdz-t36
creator_did          = ivo://CDS/P/HLA/I
prov_did             = ivo://cadc.nrc.ca/hla
obs_collection       = HLA-I
obs_title            = HLA-I : F814W, F791W, F785LP and F775W
obs_description      = The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC 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 the 4th of October 2014.The 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.  The Hubble Legacy Archive (HLA) is designed to optimize science from the Hubble Space Telescope by providing online, enhanced Hubble products and advanced browsing capabilities. The HLA is a joint project of the Space Telescope Science Institute (STScI), the Space Telescope European Coordinating Facility (ST-ECF), and the Canadian Astronomy Data Centre (CADC). Currently we have enhanced image products for ACS, WFPC2, WFC3, and NICMOS, extracted spectra from NICMOS and ACS grism observations.  The enhanced data products were generated from the standard HST pipeline products. The ACS, WFPC2, and WFC3, and NICMOS images have been combined using MultiDrizzle, are aligned north up , and, except for WFC3, have been astrometrically corrected when possible (for approximately 80% of the cases).  All HLA-produced images are in units of electrons/second, which for WFPC2 and NICMOS differs from calibration pipeline products; photometric zeropoints must be adjusted to reflect the units used.
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. "
hips_initial_fov     = 0.06216
hips_initial_ra      = 189.25342
hips_initial_dec     = +26.10801
hips_pixel_bitpix    = -32
data_pixel_bitpix    = -32
hips_sampling        = bilinear
hips_overlay         = mean
hips_hierarchy       = median
hips_creator         = Durand D. (CDS)
prov_progenitor      = Canadian Astronomy Data Centre
t_min                = 47280.00018518
t_max                = 58024.13143519
obs_regime           = Optical
client_category      = Image/Optical/HST/HLA
em_min               = 6.90e-07
em_max               = 9.829e-07
hips_builder         = Aladin/HipsGen v12.044
hips_version         = 1.4
hips_release_date    = 2023-03-08T23:46Z
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 0.12
hips_data_range      = -24.9 74.68
hips_pixel_scale     = 1.397E-5
s_pixel_scale        = 1.100E-5
dataproduct_type     = image
moc_sky_fraction     = 0.001473
hipsgen_date         = 2018-04-16T16:11Z
hipsgen_params       = -maxThread=25 "-hips_creator=CADC (Daniel Durand)" -obs_title=I -in=filter_I_extract -force -blank=0 "-fitskeys=DSNAME INSTRUME OPT_ELE DETECTOR TIME_EXP PROP_ID PRODTYPE TARGNAME NMEMBERS OBS_DATE T_MIN T_MAX WAVE_MIN WAVE_MAX" -hips_order=13 -mocOrder=16 -out=filter_I_hips "-hips_pixel_cut=0.0 0.12" -live -creator_did=CDS/P/HST/I
hips_creation_date   = 2018-04-16T16:11Z
hipsgen_date_1       = 2018-04-17T09:32Z
hipsgen_params_1     = -maxThread=25 "-hips_creator=CADC (Daniel Durand)" -obs_title=I -in=filter_I_extract -force -blank=0 "-fitskeys=DSNAME INSTRUME OPT_ELE DETECTOR TIME_EXP PROP_ID PRODTYPE TARGNAME NMEMBERS OBS_DATE T_MIN T_MAX WAVE_MIN WAVE_MAX" -hips_order=13 -mocOrder=16 -out=filter_I_hips "-hips_pixel_cut=0.0 0.12" -live -creator_did=CDS/P/HST/I
hipsgen_date_2       = 2019-05-07T11:29Z
hipsgen_params_2     = out=/asd-volumes/sc1-asd-volume8/HLA-hips/filter_I_hips UPDATE
hipsgen_date_3       = 2023-03-08T23:46Z
hipsgen_params_3     = out=/var/www/HLA-hips/filter_I_hips "pixelCut=11% 99.9% byRegion log" PNG
hips_service_url     = https://alasky.cds.unistra.fr/HLA-hips/filter_I_hips
hips_progenitor_url  = https://alasky.cds.unistra.fr/HLA-hips/filter_I_hips/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/HLA-hips/filter_I_hips
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 41
moc_time_range       = 27439
moc_order            = 13
obs_initial_ra       = 189.25342
obs_initial_dec      = +26.10801
obs_initial_fov      = 0.007157263357952928
TIMESTAMP            = 1702505973396
,
ID                   = CDS/P/HLA/R
hips_doi             = 10.26093/cds/aladin/19bm-8ca
creator_did          = ivo://CDS/P/HLA/R
prov_did             = ivo://cadc.nrc.ca/hla
obs_collection       = HLA-R
obs_title            = HLA-R : F702W and F675W
obs_description      = The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F702W  and F675W filters between the beginning of the mission  to the 4th of October 2014.The 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.  The Hubble Legacy Archive (HLA) is designed to optimize science from the Hubble Space Telescope by providing online, enhanced Hubble products and advanced browsing capabilities. The HLA is a joint project of the Space Telescope Science Institute (STScI), the Space Telescope European Coordinating Facility (ST-ECF), and the Canadian Astronomy Data Centre (CADC). Currently we have enhanced image products for ACS, WFPC2, WFC3, and NICMOS, extracted spectra from NICMOS and ACS grism observations.  The enhanced data products were generated from the standard HST pipeline products. The ACS, WFPC2, and WFC3, and NICMOS images have been combined using MultiDrizzle, are aligned north up , and, except for WFC3, have been astrometrically corrected when possible (for approximately 80% of the cases).  All HLA-produced images are in units of electrons/second, which for WFPC2 and NICMOS differs from calibration pipeline products; photometric zeropoints must be adjusted to reflect the units used.
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. "
hips_initial_fov     = 0.05972
hips_initial_ra      = 176.43196
hips_initial_dec     = +49.76079
hips_pixel_bitpix    = -32
data_pixel_bitpix    = -32
hips_sampling        = bilinear
hips_overlay         = mean
hips_hierarchy       = median
hips_creator         = Durand D. (CDS)
prov_progenitor      = Canadian Astronomy Data Centre
t_min                = 49376.20922454
t_max                = 54950.16472222
obs_regime           = Optical
client_category      = Image/Optical/HST/HLA
em_min               = 6.1256e-07
em_max               = 7.792e-07
hips_builder         = Aladin/HipsGen v12.044
hips_version         = 1.4
hips_release_date    = 2023-03-09T10:33Z
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 0.12
hips_data_range      = -18.57 49.47
hips_pixel_scale     = 1.397E-5
s_pixel_scale        = 2.777E-5
dataproduct_type     = image
moc_sky_fraction     = 1.565E-4
hipsgen_date         = 2018-04-14T06:03Z
hipsgen_params       = -maxThread=25 "-hips_creator=CADC (Daniel Durand)" -obs_title=R -in=filter_R_extract -force -blank=0 "-fitskeys=DSNAME INSTRUME OPT_ELE DETECTOR TIME_EXP PROP_ID PRODTYPE TARGNAME NMEMBERS OBS_DATE T_MIN T_MAX WAVE_MIN WAVE_MAX" -hips_order=13 -mocOrder=16 -out=filter_R_hips "-hips_pixel_cut=0.0 0.12" -live -creator_did=CDS/P/HST/R
hips_creation_date   = 2018-04-14T06:03Z
hipsgen_date_1       = 2018-04-14T06:48Z
hipsgen_params_1     = -maxThread=25 "-hips_creator=CADC (Daniel Durand)" -obs_title=R -in=filter_R_extract -force -blank=0 "-fitskeys=DSNAME INSTRUME OPT_ELE DETECTOR TIME_EXP PROP_ID PRODTYPE TARGNAME NMEMBERS OBS_DATE T_MIN T_MAX WAVE_MIN WAVE_MAX" -hips_order=13 -mocOrder=16 -out=filter_R_hips "-hips_pixel_cut=0.0 0.12" -live -creator_did=CDS/P/HST/R
hipsgen_date_2       = 2019-05-07T11:30Z
hipsgen_params_2     = out=/asd-volumes/sc1-asd-volume8/HLA-hips/filter_R_hips UPDATE
hipsgen_date_3       = 2023-03-09T10:33Z
hipsgen_params_3     = out=/var/www/HLA-hips/filter_R_hips "pixelCut=11% 99.9% byRegion log" PNG
hips_service_url     = https://alasky.cds.unistra.fr/HLA-hips/filter_R_hips
hips_progenitor_url  = https://alasky.cds.unistra.fr/HLA-hips/filter_R_hips/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/HLA-hips/filter_R_hips
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 41
moc_time_range       = 2650
moc_order            = 13
obs_initial_ra       = 176.43196
obs_initial_dec      = +49.76079
obs_initial_fov      = 0.007157263357952928
TIMESTAMP            = 1702678762927
,
ID                   = CDS/P/HLA/U
hips_doi             = 10.26093/cds/aladin/36dx-d19
creator_did          = ivo://CDS/P/HLA/U
prov_did             = ivo://cadc.nrc.ca/hla
obs_collection       = HLA-U
obs_title            = HLA-U : F336W, F330W, F300W, F275W
obs_description      = The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC 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 the 4th of October 2014.The 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.  The Hubble Legacy Archive (HLA) is designed to optimize science from the Hubble Space Telescope by providing online, enhanced Hubble products and advanced browsing capabilities. The HLA is a joint project of the Space Telescope Science Institute (STScI), the Space Telescope European Coordinating Facility (ST-ECF), and the Canadian Astronomy Data Centre (CADC). Currently we have enhanced image products for ACS, WFPC2, WFC3, and NICMOS, extracted spectra from NICMOS and ACS grism observations.  The enhanced data products were generated from the standard HST pipeline products. The ACS, WFPC2, and WFC3, and NICMOS images have been combined using MultiDrizzle, are aligned north up , and, except for WFC3, have been astrometrically corrected when possible (for approximately 80% of the cases).  All HLA-produced images are in units of electrons/second, which for WFPC2 and NICMOS differs from calibration pipeline products; photometric zeropoints must be adjusted to reflect the units used.
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. "
hips_initial_fov     = 0.0553
hips_initial_ra      = 11.15706
hips_initial_dec     = +41.81818
hips_pixel_bitpix    = -32
data_pixel_bitpix    = -32
hips_sampling        = bilinear
hips_overlay         = mean
hips_hierarchy       = median
hips_creator         = Durand D. (CDS)
prov_progenitor      = Canadian Astronomy Data Centre
t_min                = 49406.59325231
t_max                = 58023.28240741
obs_regime           = UV
client_category      = Image/UV/HST/HLA
em_min               = 2.432e-07
em_max               = 3.70e-7
hips_builder         = Aladin/HipsGen v10.123
hips_version         = 1.4
hips_release_date    = 2019-05-07T11:32Z
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      = -23.47 70.33
hips_pixel_scale     = 1.397E-5
s_pixel_scale        = 1.100E-5
dataproduct_type     = image
dataproduct_subtype  = live
moc_sky_fraction     = 4.011E-4
hips_estsize         = 473017499
hipsgen_date         = 2018-04-12T18:07Z
hipsgen_params       = -maxThread=25 "-hips_creator=CADC (Daniel Durand)" -obs_title=U -in=filter_U_extract -force -blank=0 "-fitskeys=DSNAME INSTRUME OPT_ELE DETECTOR TIME_EXP PROP_ID PRODTYPE TARGNAME NMEMBERS OBS_DATE T_MIN T_MAX WAVE_MIN WAVE_MAX" -hips_order=13 -mocOrder=16 -out=filter_U_hips "-hips_pixel_cut=0.0 0.15" -live -creator_did=CDS/P/HST/U
hips_creation_date   = 2018-04-12T18:07Z
hipsgen_date_1       = 2018-04-12T21:14Z
hipsgen_params_1     = -maxThread=25 "-hips_creator=CADC (Daniel Durand)" -obs_title=U -in=filter_U_extract -force -blank=0 "-fitskeys=DSNAME INSTRUME OPT_ELE DETECTOR TIME_EXP PROP_ID PRODTYPE TARGNAME NMEMBERS OBS_DATE T_MIN T_MAX WAVE_MIN WAVE_MAX" -hips_order=13 -mocOrder=16 -out=filter_U_hips "-hips_pixel_cut=0.0 0.15" -live -creator_did=CDS/P/HST/U
hipsgen_date_2       = 2019-05-07T11:32Z
hipsgen_params_2     = out=/asd-volumes/sc1-asd-volume8/HLA-hips/filter_U_hips UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/HLA-hips/filter_U_hips
hips_progenitor_url  = https://alasky.cds.unistra.fr/HLA-hips/filter_U_hips/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/HLA-hips/filter_U_hips
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 41
moc_time_range       = 11428
moc_order            = 13
obs_initial_ra       = 11.15706
obs_initial_dec      = +41.81818
obs_initial_fov      = 0.007157263357952928
TIMESTAMP            = 1702678763515
,
ID                   = CDS/P/HLA/V
creator_did          = ivo://CDS/P/HLA/V
prov_did             = ivo://cadc.nrc.ca/hla
obs_collection       = HLA-V
obs_title            = HLA-V : F555W, F547M, F569W
obs_description      = The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F555W, F547M and F569W filters between the beginning of the mission  to the 4th of October 2014.The 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.  The Hubble Legacy Archive (HLA) is designed to optimize science from the Hubble Space Telescope by providing online, enhanced Hubble products and advanced browsing capabilities. The HLA is a joint project of the Space Telescope Science Institute (STScI), the Space Telescope European Coordinating Facility (ST-ECF), and the Canadian Astronomy Data Centre (CADC). Currently we have enhanced image products for ACS, WFPC2, WFC3, and NICMOS, extracted spectra from NICMOS and ACS grism observations.  The enhanced data products were generated from the standard HST pipeline products. The ACS, WFPC2, and WFC3, and NICMOS images have been combined using MultiDrizzle, are aligned north up , and, except for WFC3, have been astrometrically corrected when possible (for approximately 80% of the cases).  All HLA-produced images are in units of electrons/second, which for WFPC2 and NICMOS differs from calibration pipeline products; photometric zeropoints must be adjusted to reflect the units used.
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. "
hips_initial_fov     = 0.06082
hips_initial_ra      = 186.44899
hips_initial_dec     = +33.53609
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/Universite de Strasbourg
prov_progenitor      = Canadian Astronomy Data Centre
t_min                = 47280.00018518
t_max                = 58024.83653935
obs_regime           = Optical
client_category      = Image/Optical/HST/HLA
em_min               = 4.417e-07
em_max               = 6.591e-07
hips_builder         = Aladin/HipsGen v12.060
hips_version         = 1.4
hips_release_date    = 2023-06-30T15:17Z
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      = -2.169 5.853
hips_pixel_scale     = 1.397E-5
s_pixel_scale        = 1.100E-5
dataproduct_type     = image
moc_sky_fraction     = 3.957E-4
hipsgen_date         = 2018-04-13T10:59Z
hipsgen_params       = -maxThread=25 "-hips_creator=CADC (Daniel Durand)" -obs_title=V -in=filter_V_extract -force -blank=0 "-fitskeys=DSNAME INSTRUME OPT_ELE DETECTOR TIME_EXP PROP_ID PRODTYPE TARGNAME NMEMBERS OBS_DATE T_MIN T_MAX WAVE_MIN WAVE_MAX" -hips_order=13 -mocOrder=16 -out=filter_V_hips "-hips_pixel_cut=0.0 0.15" -live -creator_did=CDS/P/HST/V
hips_creation_date   = 2018-04-13T10:59Z
hipsgen_date_1       = 2018-04-13T13:51Z
hipsgen_params_1     = -maxThread=25 "-hips_creator=CADC (Daniel Durand)" -obs_title=V -in=filter_V_extract -force -blank=0 "-fitskeys=DSNAME INSTRUME OPT_ELE DETECTOR TIME_EXP PROP_ID PRODTYPE TARGNAME NMEMBERS OBS_DATE T_MIN T_MAX WAVE_MIN WAVE_MAX" -hips_order=13 -mocOrder=16 -out=filter_V_hips "-hips_pixel_cut=0.0 0.15" -live -creator_did=CDS/P/HST/V
hipsgen_date_2       = 2019-05-07T11:32Z
hipsgen_params_2     = out=/asd-volumes/sc1-asd-volume8/HLA-hips/filter_V_hips UPDATE
hipsgen_date_3       = 2023-06-30T13:44Z
hipsgen_params_3     = out=/var/www/HLA-hips/filter_V_hips PNG
hipsgen_date_4       = 2023-06-30T15:17Z
hipsgen_params_4     = out=/var/www/HLA-hips/filter_V_hips mode=median PNG
hips_service_url     = https://alasky.cds.unistra.fr/HLA-hips/filter_V_hips
hips_progenitor_url  = https://alasky.cds.unistra.fr/HLA-hips/filter_V_hips/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/HLA-hips/filter_V_hips
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 41
moc_time_range       = 8084
moc_order            = 13
obs_initial_ra       = 186.44899
obs_initial_dec      = +33.53609
obs_initial_fov      = 0.007157263357952928
TIMESTAMP            = 1696956485373
,
ID                   = CDS/P/HLA/Y
creator_did          = ivo://CDS/P/HLA/Y
prov_did             = ivo://cadc.nrc.ca/hla
obs_collection       = HLA-Y
obs_title            = HLA-Y : F110W and F105W
obs_description      = The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F110W and F105W filters between the beginning of the mission  to the 4th of October 2014.The 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.  The Hubble Legacy Archive (HLA) is designed to optimize science from the Hubble Space Telescope by providing online, enhanced Hubble products and advanced browsing capabilities. The HLA is a joint project of the Space Telescope Science Institute (STScI), the Space Telescope European Coordinating Facility (ST-ECF), and the Canadian Astronomy Data Centre (CADC). Currently we have enhanced image products for ACS, WFPC2, WFC3, and NICMOS, extracted spectra from NICMOS and ACS grism observations.  The enhanced data products were generated from the standard HST pipeline products. The ACS, WFPC2, and WFC3, and NICMOS images have been combined using MultiDrizzle, are aligned north up, and, except for WFC3, have been astrometrically corrected when possible (for approximately 80% of the cases).  All HLA-produced images are in units of electrons/second, which for WFPC2 and NICMOS differs from calibration pipeline products; photometric zeropoints must be adjusted to reflect the units used.
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. "
hips_initial_fov     = 0.04985
hips_initial_ra      = 64.1384
hips_initial_dec     = -24.11368
hips_pixel_bitpix    = -32
data_pixel_bitpix    = -32
hips_sampling        = bilinear
hips_overlay         = overlayMean mergeOverwrite treeMean
hips_hierarchy       = median
hips_creator         = Durand D. (CDS)
prov_progenitor      = Canadian Astronomy Data Centre
t_min                = 50624.87065972
t_max                = 58023.60008102
obs_regime           = Infrared
client_category      = Image/Infrared/HST/HLA
em_min               = 8.4225e-07
em_max               = 1.42975e-06
hips_builder         = Aladin/HipsGen v12.060
hips_version         = 1.4
hips_release_date    = 2023-07-03T08:44Z
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 0.8
hips_data_range      = -207.2 622.5
hips_pixel_scale     = 1.397E-5
s_pixel_scale        = 2.499E-5
dataproduct_type     = image
moc_sky_fraction     = 2.011E-4
hipsgen_date         = 2018-04-14T07:33Z
hipsgen_params       = -maxThread=25 "-hips_creator=CADC (Daniel Durand)" -obs_title=Y -in=filter_Y_extract -force -blank=0 "-fitskeys=DSNAME INSTRUME OPT_ELE DETECTOR TIME_EXP PROP_ID PRODTYPE TARGNAME NMEMBERS OBS_DATE T_MIN T_MAX WAVE_MIN WAVE_MAX" -hips_order=13 -mocOrder=16 -out=filter_Y_hips "-hips_pixel_cut=0.0 0.8" -live -creator_did=CDS/P/HST/Y
hips_creation_date   = 2018-04-14T07:33Z
hipsgen_date_1       = 2018-04-14T08:46Z
hipsgen_params_1     = -maxThread=25 "-hips_creator=CADC (Daniel Durand)" -obs_title=Y -in=filter_Y_extract -force -blank=0 "-fitskeys=DSNAME INSTRUME OPT_ELE DETECTOR TIME_EXP PROP_ID PRODTYPE TARGNAME NMEMBERS OBS_DATE T_MIN T_MAX WAVE_MIN WAVE_MAX" -hips_order=13 -mocOrder=16 -out=filter_Y_hips "-hips_pixel_cut=0.0 0.8" -live -creator_did=CDS/P/HST/Y
hipsgen_date_2       = 2019-05-07T08:52Z
hipsgen_params_2     = out=/asd-volumes/sc1-asd-volume8/HLA-hips/filter_Y_hips UPDATE
hipsgen_date_3       = 2019-05-07T09:36Z
hipsgen_params_3     = out=/asd-volumes/sc1-asd-volume8/HLA-hips/filter_Y_hips UPDATE
hipsgen_date_4       = 2023-07-03T08:36Z
hipsgen_params_4     = out=/var/www/HLA-hips/filter_Y_hips TREE
hipsgen_date_5       = 2023-07-03T08:44Z
hipsgen_params_5     = out=/var/www/HLA-hips/filter_Y_hips TREE
hips_service_url     = https://alasky.cds.unistra.fr/HLA-hips/filter_Y_hips
hips_progenitor_url  = https://alasky.cds.unistra.fr/HLA-hips/filter_Y_hips/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/HLA-hips/filter_Y_hips
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 41
moc_time_range       = 8871
moc_order            = 13
obs_initial_ra       = 64.1384
obs_initial_dec      = -24.11368
obs_initial_fov      = 0.007157263357952928
TIMESTAMP            = 1696956485713
,
ID                   = CDS/P/HLA/wideUV
creator_did          = ivo://CDS/P/HLA/wideUV
prov_did             = ivo://cadc.nrc.ca/hla
obs_collection       = HLA-wideUV
obs_title            = HLA-wideUV : F255W, F250W, F225W, F220W and F218W
obs_description      = The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC 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 the 4th of October 2014.The 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.  The Hubble Legacy Archive (HLA) is designed to optimize science from the Hubble Space Telescope by providing online, enhanced Hubble products and advanced browsing capabilities. The HLA is a joint project of the Space Telescope Science Institute (STScI), the Space Telescope European Coordinating Facility (ST-ECF), and the Canadian Astronomy Data Centre (CADC). Currently we have enhanced image products for ACS, WFPC2, WFC3, and NICMOS, extracted spectra from NICMOS and ACS grism observations.  The enhanced data products were generated from the standard HST pipeline products. The ACS, WFPC2, and WFC3, and NICMOS images have been combined using MultiDrizzle, are aligned north up , and, except for WFC3, have been astrometrically corrected when possible (for approximately 80% of the cases).  All HLA-produced images are in units of electrons/second, which for WFPC2 and NICMOS differs from calibration pipeline products; photometric zeropoints must be adjusted to reflect the units used.
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. "
hips_initial_fov     = 0.06916
hips_initial_ra      = 53.13447
hips_initial_dec     = -27.73647
hips_pixel_bitpix    = -32
data_pixel_bitpix    = -32
hips_sampling        = bilinear
hips_overlay         = mean
hips_hierarchy       = median
hips_creator         = Durand D. (CDS)
prov_progenitor      = Canadian Astronomy Data Centre
t_min                = 49386.08491898
t_max                = 58023.27571759
obs_regime           = UV
client_category      = Image/UV/HST/HLA
em_min               = 1.85e-07
em_max               = 3.40e-07
hips_builder         = Aladin/HipsGen v10.123
hips_version         = 1.4
hips_release_date    = 2019-05-07T11:33Z
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      = -0.5027 1.487
hips_pixel_scale     = 1.397E-5
s_pixel_scale        = 1.100E-5
dataproduct_type     = image
dataproduct_subtype  = live
moc_sky_fraction     = 1.028E-4
hips_estsize         = 121616040
hipsgen_date         = 2018-04-15T09:19Z
hipsgen_params       = -maxThread=25 "-hips_creator=CADC (Daniel Durand)" -obs_title=wideUV -in=filter_wideUV_extract -force -blank=0 "-fitskeys=DSNAME INSTRUME OPT_ELE DETECTOR TIME_EXP PROP_ID PRODTYPE TARGNAME NMEMBERS OBS_DATE T_MIN T_MAX WAVE_MIN WAVE_MAX" -hips_order=13 -mocOrder=16 -out=filter_wideUV_hips "-hips_pixel_cut=0.0 0.15" -live -creator_did=CDS/P/HST/wideUV
hips_creation_date   = 2018-04-15T09:19Z
hipsgen_date_1       = 2018-04-15T10:00Z
hipsgen_params_1     = -maxThread=25 "-hips_creator=CADC (Daniel Durand)" -obs_title=wideUV -in=filter_wideUV_extract -force -blank=0 "-fitskeys=DSNAME INSTRUME OPT_ELE DETECTOR TIME_EXP PROP_ID PRODTYPE TARGNAME NMEMBERS OBS_DATE T_MIN T_MAX WAVE_MIN WAVE_MAX" -hips_order=13 -mocOrder=16 -out=filter_wideUV_hips "-hips_pixel_cut=0.0 0.15" -live -creator_did=CDS/P/HST/wideUV
hipsgen_date_2       = 2019-05-07T11:33Z
hipsgen_params_2     = out=/asd-volumes/sc1-asd-volume8/HLA-hips/filter_wideUV_hips UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/HLA-hips/filter_wideUV_hips
hips_progenitor_url  = https://alasky.cds.unistra.fr/HLA-hips/filter_wideUV_hips/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/HLA-hips/filter_wideUV_hips
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 41
moc_time_range       = 2334
moc_order            = 13
obs_initial_ra       = 53.13447
obs_initial_dec      = -27.73647
obs_initial_fov      = 0.007157263357952928
TIMESTAMP            = 1696956485497
,
ID                   = CDS/P/HLA/wideV
creator_did          = ivo://CDS/P/HLA/wideV
prov_did             = ivo://cadc.nrc.ca/hla
obs_collection       = HLA-wideV
obs_title            = HLA-wideV : F606W and F600LP
obs_description      = The HST-HLA Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand from CADC and distributed by CDS. It sets together all HST observations done in F606W and F600LP filters between the beginning of the mission  to the 4th of October 2014.The 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.  The Hubble Legacy Archive (HLA) is designed to optimize science from the Hubble Space Telescope by providing online, enhanced Hubble products and advanced browsing capabilities. The HLA is a joint project of the Space Telescope Science Institute (STScI), the Space Telescope European Coordinating Facility (ST-ECF), and the Canadian Astronomy Data Centre (CADC). Currently we have enhanced image products for ACS, WFPC2, WFC3, and NICMOS, extracted spectra from NICMOS and ACS grism observations.  The enhanced data products were generated from the standard HST pipeline products. The ACS, WFPC2, and WFC3, and NICMOS images have been combined using MultiDrizzle, are aligned north up, and, except for WFC3, have been astrometrically corrected when possible (for approximately 80% of the cases).  All HLA-produced images are in units of electrons/second, which for WFPC2 and NICMOS differs from calibration pipeline products; photometric zeropoints must be adjusted to reflect the units used.
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. "
hips_initial_fov     = 0.06202
hips_initial_ra      = 189.25321
hips_initial_dec     = +26.10809
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/Universite de Strasbourg
prov_progenitor      = Canadian Astronomy Data Centre
t_min                = 49378.38978009
t_max                = 58025.70430556
obs_regime           = Optical
client_category      = Image/Optical/HST/HLA
em_min               = 4.70e-07
em_max               = 9.96e-07
hips_builder         = Aladin/HipsGen v10.123
hips_version         = 1.4
hips_release_date    = 2019-05-07T11:33Z
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      = -33.81 101.4
hips_pixel_scale     = 1.397E-5
s_pixel_scale        = 1.100E-5
dataproduct_type     = image
dataproduct_subtype  = live
moc_sky_fraction     = 0.001113
hips_estsize         = 1312269055
hipsgen_date         = 2018-04-14T16:18Z
hipsgen_params       = -maxThread=25 "-hips_creator=CADC (Daniel Durand)" -obs_title=wideV -in=filter_wideV_extract -force -blank=0 "-fitskeys=DSNAME INSTRUME OPT_ELE DETECTOR TIME_EXP PROP_ID PRODTYPE TARGNAME NMEMBERS OBS_DATE T_MIN T_MAX WAVE_MIN WAVE_MAX" -hips_order=13 -mocOrder=16 -out=filter_wideV_hips "-hips_pixel_cut=0.0 0.15" -live -creator_did=CDS/P/HST/wideV
hips_creation_date   = 2018-04-14T16:18Z
hipsgen_date_1       = 2018-04-15T07:50Z
hipsgen_params_1     = PNG GZIP DETAILS -maxThread=25 "-hips_creator=CADC (Daniel Durand)" -obs_title=wideV -in=filter_wideV_extract -blank=0 "-fitskeys=DSNAME INSTRUME OPT_ELE DETECTOR TIME_EXP PROP_ID PRODTYPE TARGNAME NMEMBERS OBS_DATE T_MIN T_MAX WAVE_MIN WAVE_MAX" -hips_order=13 -mocOrder=16 -out=filter_wideV_hips "-hips_pixel_cut=0.0 0.15" -live -creator_did=CDS/P/HST/wideV
hipsgen_date_2       = 2019-05-07T11:33Z
hipsgen_params_2     = out=/asd-volumes/sc1-asd-volume8/HLA-hips/filter_wideV_hips UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/HLA-hips/filter_wideV_hips
hips_progenitor_url  = https://alasky.cds.unistra.fr/HLA-hips/filter_wideV_hips/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/HLA-hips/filter_wideV_hips
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 41
moc_time_range       = 22129
moc_order            = 13
obs_initial_ra       = 189.25321
obs_initial_dec      = +26.10809
obs_initial_fov      = 0.007157263357952928
TIMESTAMP            = 1696956485597
,
ID                   = CDS/P/HSCLA/2016/g
hips_initial_fov     = 8.0
hips_initial_ra      = 153.1149759
hips_initial_dec     = -1.8160131
creator_did          = ivo://CDS/P/HSCLA/2016/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       = CNRS/Universite de Strasbourg
obs_title            = HSCLA 2016 g
obs_collection       = HSCLA 2016
obs_description      = Hyper Suprime-Cam Legacy Archive (HSCLA) is a public archive of processed, science-ready data from HSC taken as part of PI-based programs. The 2016 release includes data taken through 2016 and the total data volume increased significantly. Now, the total area of 3400 square degrees is covered in at least one filter and as many as 770 million sources are detected and measured. The data processed here are from 800 hours of observations executed under good conditions. Also, the overall data quality is improved thanks to updates in the processing pipeline.
obs_ack              = This HiPS is based on data from the Hyper Suprime-Cam Legacy Archive (HSCLA), which is operated by the Subaru Telescope. The original data in HSCLA was collected at the Subaru Telescope and retrieved from the HSC data archive system, which is operated by the Subaru Telescope and Astronomy Data Center at National Astronomical Observatory of Japan. The Subaru Telescope is honored and grateful for the opportunity of observing the Universe from Maunakea, which has the cultural, historical and natural significance in Hawaii.
prov_progenitor      = HSCLA directory tree: https://hscla.mtk.nao.ac.jp/archive/files/
bib_reference        = 2021PASJ...73..735T
bib_reference_url    = https://ui.adsabs.harvard.edu/abs/2021PASJ...73..735T/abstract
obs_copyright_url    = https://hscla.mtk.nao.ac.jp/doc/acknowledgement-hscla2016/
client_category      = Image/Optical/HSCLA
obs_regime           = Optical
em_min               = 3.84e-7
em_max               = 5.7e-7
hips_builder         = Aladin/HipsGen v11.071
hips_version         = 1.4
hips_release_date    = 2022-08-04T23:42Z
hips_frame           = equatorial
hips_order           = 12
hips_order_min       = 0
hips_tile_width      = 512
hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_cut       = -0.01 4.5
hips_data_range      = -46.22 138.1
hips_pixel_scale     = 2.795E-5
s_pixel_scale        = 4.666E-5
dataproduct_type     = image
moc_sky_fraction     = 0.03167
hips_estsize         = 9385988804
hipsgen_date         = 2022-07-16T10:38Z
hipsgen_params       = creator_did=CDS/P/HSCLA/2016/g in=data/HSC-G out=/data-test-iscsi/boch/HSCLA/ tiles
hips_creation_date   = 2022-07-16T10:38Z
hipsgen_date_1       = 2022-08-04T23:42Z
hipsgen_params_1     = creator_did=CDS/P/HSCLA/2016/g in=data/HSC-G out=/data-test-iscsi/boch/HSCLA/ "hips_pixel_cut=-0.01 4.5 asinh" png
hips_service_url     = https://alasky.cds.unistra.fr/HSCLA/CDS_P_HSCLA_2016_g
hips_progenitor_url  = https://alasky.cds.unistra.fr/HSCLA/CDS_P_HSCLA_2016_g/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/HSCLA/CDS_P_HSCLA_2016_g
hips_status_1        = public mirror clonableOnce
moc_type             = smoc
moc_order            = 12
obs_initial_ra       = 153.1149759
obs_initial_dec      = -1.8160131
obs_initial_fov      = 0.014314526715905856
TIMESTAMP            = 1696351652430
,
ID                   = CDS/P/HSCLA/2016/i
hips_initial_fov     = 30.0
hips_initial_ra      = 5.7646419
hips_initial_dec     = +35.73979206
creator_did          = ivo://CDS/P/HSCLA/2016/i
hips_pixel_bitpix    = -32
data_pixel_bitpix    = -32
hips_sampling        = bilinear
hips_overlay         = mean
hips_hierarchy       = median
hips_creator         = Boch T. (CDS)
hips_copyright       = CNRS/Universite de Strasbourg
obs_title            = HSCLA 2016 i
obs_collection       = HSCLA 2016
obs_description      = Hyper Suprime-Cam Legacy Archive (HSCLA) is a public archive of processed, science-ready data from HSC taken as part of PI-based programs. The 2016 release includes data taken through 2016 and the total data volume increased significantly. Now, the total area of 3400 square degrees is covered in at least one filter and as many as 770 million sources are detected and measured. The data processed here are from 800 hours of observations executed under good conditions. Also, the overall data quality is improved thanks to updates in the processing pipeline.
obs_ack              = This HiPS is based on data from the Hyper Suprime-Cam Legacy Archive (HSCLA), which is operated by the Subaru Telescope. The original data in HSCLA was collected at the Subaru Telescope and retrieved from the HSC data archive system, which is operated by the Subaru Telescope and Astronomy Data Center at National Astronomical Observatory of Japan. The Subaru Telescope is honored and grateful for the opportunity of observing the Universe from Maunakea, which has the cultural, historical and natural significance in Hawaii.
prov_progenitor      = HSCLA directory tree: https://hscla.mtk.nao.ac.jp/archive/files/
bib_reference        = 2021PASJ...73..735T
bib_reference_url    = https://ui.adsabs.harvard.edu/abs/2021PASJ...73..735T/abstract
obs_copyright_url    = https://hscla.mtk.nao.ac.jp/doc/acknowledgement-hscla2016/
client_category      = Image/Optical/HSCLA
obs_regime           = Optical
em_min               = 6.503e-7
em_max               = 8.9992e-7
hips_builder         = Aladin/HipsGen v11.071
hips_version         = 1.4
hips_release_date    = 2022-10-28T20:08Z
hips_frame           = equatorial
hips_order           = 12
hips_order_min       = 0
hips_tile_width      = 512
hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_scale     = 2.795E-5
s_pixel_scale        = 4.666E-5
dataproduct_type     = image
moc_sky_fraction     = 0.0281
hips_estsize         = 8328779542
hipsgen_date         = 2022-10-26T06:17Z
hipsgen_params       = creator_did=CDS/P/HSCLA/2016/r in=data/HSC-I out=/data-test-iscsi/boch/HSCLA/ tiles
hips_creation_date   = 2022-10-26T06:17Z
hips_pixel_cut       = -0.01 8.5
hipsgen_date_1       = 2022-10-28T20:08Z
hipsgen_params_1     = creator_did=CDS/P/HSCLA/2016/i in=data/HSC-I out=/data-test-iscsi/boch/HSCLA/ "hips_pixel_cut=-0.01 8.5 asinh" method=MEAN png
hips_service_url     = https://alasky.cds.unistra.fr/HSCLA/CDS_P_HSCLA_2016_i
hips_service_url_1   = https://alaskybis.cds.unistra.fr/HSCLA/CDS_P_HSCLA_2016_i
hips_status_1        = public mirror clonableOnce
moc_type             = smoc
moc_order            = 12
obs_initial_ra       = 5.7646419
obs_initial_dec      = +35.73979206
obs_initial_fov      = 0.014314526715905856
TIMESTAMP            = 1696351652574
,
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            = 1696956480121
,
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            = 1696956480629
,
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
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            = 1704925137205
,
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            = 1696956481709
,
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            = 1696956482365
,
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            = 1696956482617
,
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            = 1696956482981
,
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            = 1696956481361
,
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            = 1696956482749
,
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            = 1696956482873
,
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            = 1696351583822
,
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            = 1696351583710
,
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            = 1711279449388
,
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            = 1701291897171
,
ID                   = CDS/P/Mellinger/color
creator_did          = ivo://CDS/P/Mellinger/color
obs_collection       = Mellinger color
obs_title            = Mellinger color optical survey
obs_description      = Using a portable low-cost CCD camera system, 70 fields (each covering 40deg x 27deg) were imaged over a time span of 22 months from dark-sky locations in South Africa, Texas, and Michigan. The fields were photometrically calibrated against standard catalog stars. Using sky background data from the Pioneer 10 and 11 space probes, gradients resulting from artificial light pollution, airglow, and zodiacal light were eliminated, while the large-scale galactic and extragalactic background resulting from unresolved sources was preserved. The 648 megapixel image is a valuable educational tool, being able to fully utilize the resolution and dynamic range of modern full-dome planetarium projection systems.
prov_progenitor      = Axel Mellinger
bib_reference        = 2009PASP..121.1180M
bib_reference_url    = http://adsabs.harvard.edu/cgi-bin/nph-bib_query?db_key=AST&bibcode=2009PASP..121.1180M
obs_copyright        = Copyright 2000-2017 Axel Mellinger. All rights reserved.
obs_copyright_url    = http://www.milkywaysky.com/
client_category      = Image/Optical
client_sort_key      = 03-03
hips_creation_date   = 2010-07-12T00:00Z
hips_release_date    = 2019-05-05T06:40Z
hips_builder         = Aladin/HipsGen v10.123
hips_creator         = Boch T. (CDS)
hips_version         = 1.4
hips_order           = 4
hips_frame           = galactic
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/MellingerRGB/Moc.fits
hips_status          = public master clonableOnce
hips_copyright       = CNRS/Unistra
t_min                = 54374
t_max                = 55044
obs_regime           = Optical
em_min               = 4e-7
em_max               = 8e-7
hips_pixel_scale     = 0.007157
hips_initial_fov     = 360.0
hips_initial_ra      = 266.4168166
hips_initial_dec     = -29.0078249
hips_order_min       = 0
dataproduct_subtype  = color
moc_sky_fraction     = 1
hips_estsize         = 36707
hipsgen_date         = 2019-05-05T06:40Z
hipsgen_params       = out=/asd-volumes/sc1-asd-volume10/MellingerRGB UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/MellingerRGB
hips_service_url_1   = https://alaskybis.cds.unistra.fr/MellingerRGB
hips_status_1        = public mirror clonableOnce
hips_service_url_2   = https://healpix.ias.u-psud.fr/CDS_P_Mellinger_color
hips_status_2        = public mirror unclonable
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 4
obs_initial_ra       = 266.4168166
obs_initial_dec      = -29.0078249
obs_initial_fov      = 3.6645188392718993
TIMESTAMP            = 1711279430632
,
ID                   = CDS/P/NEOWISER/Color
creator_did          = ivo://CDS/P/NEOWISER/Color
obs_collection       = NEOWISER W2-W1
obs_title            = NEOWISER color  Red (W2) , Blue (W1)
obs_description      = The NEOWISE project is the asteroid-hunting portion of the Wide-field Infrared Survey Explorer (WISE) mission. Funded by NASA's Planetary Science Division, NEOWISE harvests measurements of asteroids and comets from the WISE images and provides a rich archive for searching WISE data for solar system objects. Here we update our full-depth coadds by folding in the most recently published year of W1/W2 exposures released by NEOWISER. These new single-frame data were acquired between 2015 December 13 and 2016 December 13, and became public in 2017 June. In the present work, we simply re-ran the latest unWISE coaddition code (Meisner et al. 2017a) on inputs including this additional year of publicly available NEOWISER frames. The resulting set of full-depth coadds uniformly incorporates all publicly available W1 and W2 exposures, with observation dates ranging from 2010 January 7 to 2016 December 13. The inputs consisted of ~ 10.5 million frames per band, totaling ~ 140 terabytes of single-exposure pixel data.
hips_creator         = Buga M. (CDS)
hips_copyright       = CNRS/Unistra
obs_ack              = This publication also makes use of data products from NEOWISE, which is a project of the Jet Propulsion Laboratory/California Institute of Technology, funded by the Planetary Science Division of the National Aeronautics and Space Administration
prov_progenitor      = IPAC/NASA
bib_reference        = 2014ApJ...792...30M
bib_reference_url    = https://ui.adsabs.harvard.edu/abs/2014ApJ...792...30M/abstract
obs_copyright        = University of Massachusetts & IPAC/Caltech
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prov_progenitor      = IPAC/NASA
bib_reference        = 2014ApJ...792...30M
bib_reference_url    = https://ui.adsabs.harvard.edu/abs/2014ApJ...792...30M/abstract
obs_copyright        = University of Massachusetts & IPAC/Caltech
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prov_progenitor      = IPAC/NASA
bib_reference        = 2014ApJ...792...30M
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obs_copyright        = Copyright 2009 Associated Universities, Inc. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.
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obs_ack              = Any papers using observational material taken with NRAO instruments (Karl G. Jansky Very Large Array or otherwise) or papers where a significant portion of the work was done at NRAO, should include the following acknowledgement to NRAO and NSF:
prov_progenitor      = NRAO
bib_reference        = 1998AJ....115.1693C
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obs_description      = The Planck mission will collect and characterise radiation from the Cosmic Microwave Background (CMB) using sensitive radio receivers operating at extremely low temperatures. These receivers will determine the black body equivalent temperature of the background radiation and will be capable of distinguishing temperature variations of about one microkelvin. These measurements will be used to produce the best ever maps of anisotropies in the CMB radiation field.
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ID                   = CDS/P/PLANCK/R2/HFI143
creator_did          = ivo://CDS/P/PLANCK/R2/HFI143
obs_collection       = PLANCK R2 HFI143
obs_title            = PLANCK R2 nominal frequency HFI map 143Ghz
obs_description      = The Planck mission will collect and characterise radiation from the Cosmic Microwave Background (CMB) using sensitive radio receivers operating at extremely low temperatures. These receivers will determine the black body equivalent temperature of the background radiation and will be capable of distinguishing temperature variations of about one microkelvin. These measurements will be used to produce the best ever maps of anisotropies in the CMB radiation field.
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obs_description      = Planck is ESA's mission to observe the first light in the Universe. Planck was launched on 14 May 2009, and the minimum requirement for success was for the spacecraft to complete two whole surveys of the sky. In the end, Planck worked perfectly for 30 months, about twice the span originally required, and completed five full-sky surveys with both instruments. Able to work at slightly higher temperatures than HFI, the Low Frequency Instrument (LFI) continued to survey the sky for a large part of 2013, providing even more data to improve the Planck final results. Planck was turned off on 23 October 2013. The high-quality data the mission has produced will continue to be scientifically explored in the years to come.
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hips_initial_ra      = 266.4150089
hips_initial_dec     = -29.0061110
creator_did          = ivo://CDS/P/QUIJOTE/DR1/MFI/P/19GHz
hips_creator         = QUIJOTE collaboration
hips_copyright       = CNRS/Unistra
obs_title            = QUIJOTE MFI DR1 19GHz Polarization
obs_collection       = QUIJOTE MFI DR1
obs_description      = The QUIJOTE (Q-U-I JOint TEnerife) CMB Experiment is a scientific collaboration between the Instituto de Astrofisica de Canarias (Tenerife, Spain), the Instituto de Fisica de Cantabria (Santander, Spain), the Departamento de Ingenieria de COMunicaciones (Santander, Spain), the Jodrell Bank Observatory (Manchester, UK), the Cavendish Laboratory (Cambridge, UK), and the IDOM company (Spain). It started operations in November 2012, and it consists in two telescopes and three instruments dedicated to measure the polarization of the microwave sky in the frequency range between 10 GHz and 40GHz, and at angular scales of one degree. We present QUIJOTE intensity and polarization maps in four frequency bands centred around 11, 13, 17 and 19 GHz, and covering approximately 30 000 deg2, including most of the Northern sky region. These maps result from 9 000 hours of observations taken between May 2013 and June 2018 with the first QUIJOTE instrument (MFI), and have angular resolutions of around one degree, and sensitivities in polarization within the range 35-40 microkelvin per 1-degree beam, being a factor 2-4 worse in intensity.
obs_ack              = Please acknowledge the use of the QUIJOTE MFI wide survey data products by: citing the main QUIJOTE MFI wide survey paper ( Rubino-Martin et al. 2023 ), and if using derived products, the relevant associated paper(s); and adding an acknowledgment statement: "Some of the presented results are based on observations obtained with the QUIJOTE experiment ( http://research.iac.es/proyecto/quijote )".
prov_progenitor      = https://research.iac.es/proyecto/quijote/pages/en/data/mfi-wide-survey.php
bib_reference        = 2023MNRAS.519.3383R
bib_reference_url    = https://ui.adsabs.harvard.edu/abs/2023MNRAS.519.3383R
obs_copyright_url    = https://research.iac.es/proyecto/quijote/pages/en/data/mfi-wide-survey.php
obs_regime           = Radio
em_min               = 0.01578947368
em_max               = 0.01578947368
client_category      = Image/Radio/QUIJOTE/DR1/Polarization
hips_builder         = Aladin/HipsGen v11.024
hips_version         = 1.4
hips_release_date    = 2023-01-14T09:34Z
hips_frame           = galactic
hips_order           = 3
hips_order_min       = 0
hips_tile_width      = 64
hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_bitpix    = -32
hips_pixel_cut       = 0.003608 1.692
hips_data_range      = -3.556 10.67
hips_pixel_scale     = 1.832
dataproduct_type     = image
moc_sky_fraction     = 1
hips_estsize         = 8
hips_creation_date   = 2023-01-14T09:32Z
hips_service_url     = https://alasky.cds.unistra.fr/QUIJOTE/DR1/MFI/CDS_P_QUIJOTE_DR1_MFI_P_19GHz
hips_service_url_1   = https://alaskybis.cds.unistra.fr/QUIJOTE/DR1/MFI/CDS_P_QUIJOTE_DR1_MFI_P_19GHz
hips_status_1        = public mirror clonableOnce
moc_type             = smoc
moc_order            = 7
obs_initial_ra       = 266.4150089
obs_initial_dec      = -29.0061110
obs_initial_fov      = 0.4580648549089874
TIMESTAMP            = 1695746875674
,
ID                   = CDS/P/RASS
creator_did          = ivo://CDS/P/RASS
obs_collection       = RASS
obs_title            = ROSAT X-Ray All-Sky Survey
obs_description      = The ROSAT All-Sky X-ray Survey was obtained during 1990/1991 using the ROSAT Position Sensitive Proportional Counter (PSPC) in combination with the ROSAT X-ray Telescope (XRT).
obs_copyright        = Distributed by MPE - HEALPixed by CDS
obs_copyright_url    = http://www.mpe.mpg.de/xray/home.php
client_category      = Image/X/ROSAT
client_sort_key      = 01-02
hips_creation_date   = 2014-03-29T13:46Z
hips_release_date    = 2019-05-05T06:52Z
hips_builder         = Aladin/HipsGen v10.123
hips_creator         = Fernique P. (CDS)
hips_version         = 1.4
hips_order           = 4
hips_frame           = equatorial
hips_tile_width      = 512
hips_tile_format     = jpeg fits
dataproduct_type     = image
moc_access_url       = http://alasky.u-strasbg.fr/RASS/Moc.fits
hips_status          = public master clonableOnce
hips_initial_fov     = 100.0
hips_initial_ra      = 266.4168166
hips_initial_dec     = -29.0078249
hips_copyright       = CNRS/Unistra
prov_progenitor      = NASA/HEASARC
bib_reference        = 1999A&A...349..389V
bib_reference_url    = http://simbad.u-strasbg.fr/simbad/sim-ref?bibcode=1999A%26A...349..389V&simbo=on
t_min                = 48058
t_max                = 48602
obs_regime           = X-ray
em_min               = 5.1660e-10
em_max               = 1.2398e-8
hips_pixel_scale     = 0.007157
moc_sky_fraction     = 1
hips_estsize         = 2247318
hips_order_min       = 0
hips_pixel_bitpix    = 16
hipsgen_date         = 2019-05-05T06:52Z
hipsgen_params       = out=/asd-volumes/sc1-asd-volume10/RASS UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/RASS
hips_service_url_1   = https://alaskybis.cds.unistra.fr/RASS
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 4
obs_initial_ra       = 266.4168166
obs_initial_dec      = -29.0078249
obs_initial_fov      = 3.6645188392718993
TIMESTAMP            = 1696351585354
,
ID                   = CDS/P/ROSATWFC/F1
creator_did          = ivo://CDS/P/ROSATWFC/F1
obs_collection       = ROSAT WFC F1 (15-27 PHz)
obs_title            = ROSAT Wide Field Camera F1 (15-27 PHz)
obs_description      = During 1990-91 the Wide Field Camera (WFC), on the ROSAT satellite, performed the first all-sky surveys at EUV wavelengths. The surrey was conducted in two wavebands, S1 and S2, with passbands covering the ranges 60-140 A and 110-200 A. It was fully imaging, with effective spatial resolution of about 3 arcmin full width at half maximum (FWHM), and point source location accuracy of typically better than 1 arcmin.
obs_ack              = University of Leiscester - obtained through SkyView NASA/HEASARC
prov_progenitor      = SkyView NASA/HEASARC
bib_reference        = 1995AdSpR..16R..69M
bib_reference_url    = http://adsabs.harvard.edu/abs/1995AdSpR..16R..69M
obs_copyright        = University of Leicester used by permission (no restrictions on not for profit use)
obs_copyright_url    = http://skyview.gsfc.nasa.gov/current/cgi/survey.pl
t_min                = 57427.500000
t_max                = 48257.500000
obs_regime           = UV
em_min               = 1.1103e-8
em_max               = 1.9986e-8
hips_builder         = Aladin/HipsGen v10.125
hips_version         = 1.4
hips_release_date    = 2019-05-20T15:06Z
hips_creator         = Buga M. (CDS)
hips_frame           = equatorial
hips_order           = 3
hips_tile_width      = 512
hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_bitpix    = -32
data_pixel_bitpix    = -32
hips_hierarchy       = mean
hips_pixel_cut       = -1 10
hips_data_range      = -1 170
hips_initial_ra      = 28.93525
hips_initial_dec     = -16.04479
hips_initial_fov     = 2.66672
hips_pixel_scale     = 0.01431
s_pixel_scale        = 0.01667
dataproduct_type     = image
moc_sky_fraction     = 0.9714
hips_estsize         = 1098298
hipsgen_date         = 2016-02-09T15:40Z
hipsgen_params       = in=WFCF1 out=WFCF1HiPS_1 ivorn=ivo://CDS.Aladin/P/ROSAT-WFC-F2 Publisher=M.Buga [CDS] -pixelcut=-1 10 -pixelRange=-1 170 INDEX TILES PNG DETAILS
hips_creation_date   = 2016-02-09T15:40Z
hipsgen_date_1       = 2016-02-09T15:40Z
hipsgen_params_1     = in=WFCF1 out=WFCF1HiPS_1 ivorn=ivo://CDS.Aladin/P/ROSAT-WFC-F2 Publisher=M.Buga [CDS] -pixelcut=-1 10 -pixelRange=-1 170 INDEX TILES PNG DETAILS
client_category      = Image/UV/ROSATWFC
client_sort_key      = 02-xx
hips_order_min       = 0
hipsgen_date_2       = 2019-05-20T15:06Z
hipsgen_params_2     = out=/asd-volumes/sc1-asd-volume6/ROSATWFC-new/ROSAT-WFC1 UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/ROSATWFC-new/ROSAT-WFC1
hips_progenitor_url  = https://alasky.cds.unistra.fr/ROSATWFC-new/ROSAT-WFC1/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/ROSATWFC-new/ROSAT-WFC1
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 8
obs_initial_ra       = 28.93525
obs_initial_dec      = -16.04479
obs_initial_fov      = 0.2290324274544937
TIMESTAMP            = 1696351623606
,
ID                   = CDS/P/ROSATWFC/F2
creator_did          = ivo://CDS/P/ROSATWFC/F2
obs_collection       = ROSAT-WFC-F2 (21-50 PHz)
obs_title            = ROSAT Wide Field Camera F2 (21-50 PHz)
obs_description      = obs_description      = During 1990-91 the Wide Field Camera (WFC), on the ROSAT satellite, performed the first all-sky surveys at EUV wavelengths. The surrey was conducted in two wavebands, S1 and S2, with passbands covering the ranges 60-140 A and 110-200 A. It was fully imaging, with effective spatial resolution of about 3 arcmin full width at half maximum (FWHM), and point source location accuracy of typically better than 1 arcmin.
obs_ack              = University of Leiscester - obtained through SkyView NASA/HEASARC
prov_progenitor      = SkyView NASA/HEASARC
bib_reference        = 1995AdSpR..16R..69M
bib_reference_url    = http://adsabs.harvard.edu/abs/1995AdSpR..16R..69M
obs_copyright        = University of Leicester used by permission (no restrictions on not for profit use)
obs_copyright_url    = http://skyview.gsfc.nasa.gov/current/cgi/survey.pl
t_min                = 57427.500000
t_max                = 48257.500000
obs_regime           = UV
em_min               = 5.9958e-9
em_max               = 1.4276e-8
hips_builder         = Aladin/HipsGen v10.125
hips_version         = 1.4
hips_release_date    = 2019-05-20T15:06Z
hips_creator         = Buga M. (CDS)
hips_frame           = equatorial
hips_order           = 3
hips_tile_width      = 512
hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_bitpix    = -32
data_pixel_bitpix    = -32
hips_hierarchy       = mean
hips_pixel_cut       = -1 10
hips_data_range      = -1 170
hips_initial_ra      = 4.07769
hips_initial_dec     = -22.3285
hips_initial_fov     = 2.66672
hips_pixel_scale     = 0.01431
s_pixel_scale        = 0.01667
dataproduct_type     = image
moc_sky_fraction     = 0.9714
hips_estsize         = 1098298
hipsgen_date         = 2016-02-09T15:19Z
hipsgen_params       = in=WFCF2 out=WFCF2HiPS_1 ivorn=ivo://CDS.Aladin/P/ROSAT-WFC-F2 Publisher=M.Buga [CDS] -pixelcut=-1 10 -pixelRange=-1 170 INDEX TILES PNG DETAILS
hips_creation_date   = 2016-02-09T15:19Z
hipsgen_date_1       = 2016-02-09T15:19Z
hipsgen_params_1     = in=WFCF2 out=WFCF2HiPS_1 ivorn=ivo://CDS.Aladin/P/ROSAT-WFC-F2 Publisher=M.Buga [CDS] -pixelcut=-1 10 -pixelRange=-1 170 INDEX TILES PNG DETAILS
client_category      = Image/UV/ROSATWFC
client_sort_key      = 02-xx
hips_order_min       = 0
hipsgen_date_2       = 2019-05-20T15:06Z
hipsgen_params_2     = out=/asd-volumes/sc1-asd-volume6/ROSATWFC-new/ROSAT-WFC2 UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/ROSATWFC-new/ROSAT-WFC2
hips_progenitor_url  = https://alasky.cds.unistra.fr/ROSATWFC-new/ROSAT-WFC2/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/ROSATWFC-new/ROSAT-WFC2
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 8
obs_initial_ra       = 4.07769
obs_initial_dec      = -22.3285
obs_initial_fov      = 0.2290324274544937
TIMESTAMP            = 1696351623686
,
ID                   = CDS/P/ROSATWFC/color
creator_did          = ivo://CDS/P/ROSATWFC/color
obs_collection       = ROSAT color
obs_title            = ROSAT Wide Field Camera Color composition
obs_description      = During 1990-91 the Wide Field Camera (WFC), on the ROSAT satellite, performed the first all-sky surveys at EUV wavelengths. The surrey was conducted in two wavebands, S1 and S2, with passbands covering the ranges 60-140 A and 110-200 A. It was fully imaging, with effective spatial resolution of about 3 arcmin full width at half maximum (FWHM), and point source location accuracy of typically better than 1 arcmin.
obs_ack              = University of Leiscester - obtained through SkyView NASA/HEASARC
prov_progenitor      = SkyView NASA/HEASARC
bib_reference        = 1995AdSpR..16R..69M
bib_reference_url    = http://adsabs.harvard.edu/abs/1995AdSpR..16R..69M
obs_copyright        = University of Leicester used by permission (no restrictions on not for profit use)
obs_copyright_url    = http://skyview.gsfc.nasa.gov/current/cgi/survey.pl
t_min                = 57427.500000
t_max                = 48257.500000
obs_regime           = UV
em_min               = 5.9958e-9
em_max               = 1.9986e-8
hips_builder         = Aladin/HipsGen v10.125
hips_version         = 1.4
hips_release_date    = 2019-05-20T15:05Z
hips_creator         = Buga M. (CDS)
hips_frame           = equatorial
hips_order           = 3
hips_tile_width      = 512
hips_status          = public master clonableOnce
hips_hierarchy       = mean
hips_pixel_scale     = 0.01431
dataproduct_type     = image
hips_rgb_red         = ROSAT-WFC-F1 [-1.0 NaN 10.0 Linear]
hips_rgb_blue        = ROSAT-WFC-F2 [-1.0 NaN 10.0 Linear]
moc_sky_fraction     = 0.9714
hips_estsize         = 27532
hipsgen_date         = 2016-01-28T16:11Z
hipsgen_params       = inRed=WFCF1HiPS inBlue=WFCF2HiPS out=HIPSColor Publisher=M.Buga [CDS]
hips_creation_date   = 2016-01-28T16:11Z
hips_tile_format     = png
hipsgen_date_1       = 2016-01-28T16:13Z
hipsgen_params_1     = inRed=WFCF1HiPS inBlue=WFCF2HiPS out=HIPSColor Publisher=M.Buga [CDS]
client_category      = Image/UV/ROSATWFC
client_sort_key      = 02-xx
hips_initial_fov     = 58.63230142835039
hips_initial_ra      = 0
hips_initial_dec     = +0
hips_order_min       = 0
dataproduct_subtype  = color
hipsgen_date_2       = 2019-05-20T15:05Z
hipsgen_params_2     = out=/asd-volumes/sc1-asd-volume6/ROSATWFC-new/ROSAT-WFC-color UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/ROSATWFC-new/ROSAT-WFC-color
hips_service_url_1   = https://alaskybis.cds.unistra.fr/ROSATWFC-new/ROSAT-WFC-color
hips_status_1        = public mirror clonableOnce
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            = 1696351623534
,
ID                   = CDS/P/SCUBA/450em
creator_did          = ivo://CDS/P/SCUBA/450em
obs_collection       = SCUBA 450em
obs_title            = SCUBA 450um emission maps
obs_description      = SCUBA, the Submillimetre Common-User Bolometer Array, built by the Royal Observatory Edinburgh for the James Clerk Maxwell Telescope, is the most versatile and powerful of a new generation of submillimetre cameras. It combines a sensitive dual-waveband imaging array with a three-band photometer, and is sky-background-limited by the emission from the Mauna Kea atmosphere at all observing wavelengths from 350 um to 2 mm.
obs_copyright_url    = http://www.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/community/scubalegacy
prov_progenitor      = CADC - HEALPixed by CDS
client_category      = Image/Radio/SCUBA
client_sort_key      = 05-01-03
hips_release_date    = 2019-05-05T06:53Z
hips_creator         = CDS
hips_version         = 1.4
hips_order           = 8
hips_frame           = equatorial
hips_tile_width      = 512
hips_tile_format     = jpeg fits
dataproduct_type     = image
moc_access_url       = http://alasky.u-strasbg.fr/SCUBA/Scuba450ALLSKY/Moc.fits
hips_status          = public master clonableOnce
hips_initial_fov     = 0.2290324274544937
hips_initial_ra      = 45.0
hips_initial_dec     = 0.14920792779581243
hips_copyright       = CNRS/Unistra
bib_reference        = 1999MNRAS.303..659H
bib_reference_url    = http://simbad.u-strasbg.fr/simbad/sim-ref?bibcode=1999MNRAS.303..659H&simbo=on
obs_copyright        = SCUBA Legacy
t_min                = 50569
t_max                = 50874
obs_regime           = Radio
em_min               = 4.5E-4
em_max               = 4.5E-4
hips_builder         = Aladin/HipsGen v10.123
hips_pixel_bitpix    = -32
hips_pixel_scale     = 4.473E-4
moc_sky_fraction     = 0.003081
hips_estsize         = 70829943
hipsgen_date         = 2017-07-28T13:40Z
hipsgen_params       = -notouch out=Scuba450ALLSKY UPDATE
hips_creation_date   = 2012-10-11T11:10Z
hips_order_min       = 0
hipsgen_date_1       = 2019-05-05T06:53Z
hipsgen_params_1     = out=/asd-volumes/sc1-asd-volume10/SCUBA/Scuba450ALLSKY UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/SCUBA/Scuba450ALLSKY
hips_service_url_1   = https://alaskybis.cds.unistra.fr/SCUBA/Scuba450ALLSKY
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 8
obs_initial_ra       = 45.0
obs_initial_dec      = 0.14920792779581243
obs_initial_fov      = 0.2290324274544937
TIMESTAMP            = 1691097208641
,
ID                   = CDS/P/SCUBA/850em
creator_did          = ivo://CDS/P/SCUBA/850em
obs_collection       = SCUBA 850em
obs_title            = SCUBA 850um emission maps
obs_description      = SCUBA, the Submillimetre Common-User Bolometer Array, built by the Royal Observatory Edinburgh for the James Clerk Maxwell Telescope, is the most versatile and powerful of a new generation of submillimetre cameras. It combines a sensitive dual-waveband imaging array with a three-band photometer, and is sky-background-limited by the emission from the Mauna Kea atmosphere at all observing wavelengths from 350 um to 2 mm.
obs_copyright_url    = http://www.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/community/scubalegacy/
prov_progenitor      = CADC - HEALPixed by CDS
client_category      = Image/Radio/SCUBA
client_sort_key      = 05-01-04
hips_release_date    = 2019-05-05T06:53Z
hips_creator         = CDS
hips_version         = 1.4
hips_order           = 7
hips_frame           = equatorial
hips_tile_width      = 512
hips_tile_format     = jpeg fits
dataproduct_type     = image
moc_access_url       = http://alasky.u-strasbg.fr/SCUBA/Scuba850ALLSKY/Moc.fits
hips_status          = public master clonableOnce
hips_initial_fov     = 0.4580648549089874
hips_initial_ra      = 45.0
hips_initial_dec     = 0.2984168674869415
hips_copyright       = CNRS/Unistra
bib_reference        = 1999MNRAS.303..659H
bib_reference_url    = http://simbad.u-strasbg.fr/simbad/sim-ref?bibcode=1999MNRAS.303..659H&simbo=on
obs_copyright        = SCUBA Legacy
t_min                = 50569
t_max                = 50874
obs_regime           = Radio
em_min               = 8.5E-4
em_max               = 8.5E-4
hips_builder         = Aladin/HipsGen v10.123
hips_pixel_bitpix    = -32
hips_pixel_scale     = 8.946E-4
moc_sky_fraction     = 0.003577
hips_estsize         = 24855081
hipsgen_date         = 2017-07-28T14:16Z
hipsgen_params       = -notouch out=Scuba850ALLSKY UPDATE
hips_creation_date   = 2012-10-11T07:15Z
hips_order_min       = 0
hipsgen_date_1       = 2019-05-05T06:53Z
hipsgen_params_1     = out=/asd-volumes/sc1-asd-volume10/SCUBA/Scuba850ALLSKY UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/SCUBA/Scuba850ALLSKY
hips_service_url_1   = https://alaskybis.cds.unistra.fr/SCUBA/Scuba850ALLSKY
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 8
obs_initial_ra       = 45.0
obs_initial_dec      = 0.2984168674869415
obs_initial_fov      = 0.2290324274544937
TIMESTAMP            = 1691097208705
,
ID                   = CDS/P/SCUBA/850emi
creator_did          = ivo://CDS/P/SCUBA/850emi
obs_collection       = SCUBA 850emi
obs_title            = SCUBA 850um emission maps - extended dataset
obs_description      = SCUBA, the Submillimetre Common-User Bolometer Array, built by the Royal Observatory Edinburgh for the James Clerk Maxwell Telescope, is the most versatile and powerful of a new generation of submillimetre cameras. It combines a sensitive dual-waveband imaging array with a three-band photometer, and is sky-background-limited by the emission from the Mauna Kea atmosphere at all observing wavelengths from 350 um to 2 mm.
obs_copyright_url    = http://www.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/community/scubalegacy/
prov_progenitor      = CADC - HEALPixed by CDS
client_category      = Image/Radio/SCUBA
client_sort_key      = 05-01-05
hips_release_date    = 2019-05-05T06:54Z
hips_creator         = CDS
hips_version         = 1.4
hips_order           = 7
hips_frame           = equatorial
hips_tile_width      = 512
hips_tile_format     = jpeg fits
dataproduct_type     = image
moc_access_url       = http://alasky.u-strasbg.fr/SCUBA/Scuba850eALLSKY/Moc.fits
hips_status          = public master clonableOnce
hips_initial_fov     = 0.4580648549089874
hips_initial_ra      = 45.0
hips_initial_dec     = 0.2984168674869415
hips_copyright       = CNRS/Unistra
bib_reference        = 1999MNRAS.303..659H
bib_reference_url    = http://simbad.u-strasbg.fr/simbad/sim-ref?bibcode=1999MNRAS.303..659H&simbo=on
obs_copyright        = SCUBA Legacy
t_min                = 50569
t_max                = 50874
obs_regime           = Radio
em_min               = 8.5E-4
em_max               = 8.5E-4
hips_builder         = Aladin/HipsGen v10.123
hips_pixel_bitpix    = -32
hips_pixel_scale     = 8.946E-4
moc_sky_fraction     = 0.003953
hips_estsize         = 26891456
hipsgen_date         = 2017-07-28T14:17Z
hipsgen_params       = -notouch out=Scuba850eALLSKY UPDATE
hips_creation_date   = 2012-10-10T10:33Z
hips_order_min       = 0
hipsgen_date_1       = 2019-05-05T06:54Z
hipsgen_params_1     = out=/asd-volumes/sc1-asd-volume10/SCUBA/Scuba850eALLSKY UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/SCUBA/Scuba850eALLSKY
hips_service_url_1   = https://alaskybis.cds.unistra.fr/SCUBA/Scuba850eALLSKY
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 8
obs_initial_ra       = 45.0
obs_initial_dec      = 0.2984168674869415
obs_initial_fov      = 0.2290324274544937
TIMESTAMP            = 1691097208773
,
ID                   = CDS/P/SCUBA2/450em
creator_did          = ivo://CDS/P/SCUBA2/450em
obs_collection       = SCUBA2 450em
obs_title            = SCUBA2 450um
obs_description      = The SCUBA2-450em Hierarchical Progressive Survey (HiPS) has been built from JCMT data via CADC archive and distributed by CDS.It sets together all SCUBA2 observations done in 450 filter between the beginning of the mission to the 1st of November 2014. SCUBA-2: the 10 000 pixel bolometer camera on the James Clerk Maxwell Telescope.
obs_ack              = All publications based on SCUBA2 data should carry the following footnote: "The James Clerk Maxwell Telescope has historically been operated by the Joint Astronomy Centre on behalf of the Science and Technology Facilities Council of the United Kingdom, the National Research Council of Canada and the Netherlands Organisation for Scientific Research.
obs_copyright_url    = http://www.eaobservatory.org/jcmt/contact/
prov_progenitor      = JCMT via CADC - HiPSed by CDS
client_category      = Image/Radio/SCUBA
client_sort_key      = 05-01-01
hips_release_date    = 2019-05-05T06:54Z
hips_builder         = Aladin/HipsGen v10.123
hips_creator         = Fernique P. (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       = -350 1000
hips_data_range      = -1498984 1644385
hips_initial_ra      = 233.74375
hips_initial_dec     = +23.50658
hips_initial_fov     = 0.56612
t_max                = 56962
t_max                = 56930
moc_access_url       = http://alasky.u-strasbg.fr/SCUBA2/Scuba2_450/Moc.fits
hips_progenitor_url  = https://alasky.cds.unistra.fr/SCUBA2/Scuba2_450/HpxFinder
hips_status          = public master clonableOnce
hips_copyright       = CNRS/Unistra
bib_reference        = 2013MNRAS.430.2513H
bib_reference_url    = http://simbad.u-strasbg.fr/simbad/sim-ref?bibcode=2013MNRAS.430.2513H&simbo=on
obs_copyright        = 2014-2017 East Asian Observatory all rights reserved
t_min                = 55228
obs_regime           = Radio
em_min               = 4.5E-4
em_max               = 4.5E-4
hips_pixel_scale     = 2.236E-4
moc_sky_fraction     = 0.02216
hips_estsize         = 204562369
hips_creation_date   = 2014-11-20T11:18Z
hips_order_min       = 0
hips_pixel_bitpix    = -64
hipsgen_date         = 2019-05-05T06:54Z
hipsgen_params       = out=/asd-volumes/sc1-asd-volume10/SCUBA2/Scuba2_450 UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/SCUBA2/Scuba2_450
hips_service_url_1   = https://alaskybis.cds.unistra.fr/SCUBA2/Scuba2_450
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 41
moc_time_range       = 12750
moc_order            = 9
obs_initial_ra       = 233.74375
obs_initial_dec      = +23.50658
obs_initial_fov      = 0.11451621372724685
TIMESTAMP            = 1701291900323
,
ID                   = CDS/P/SCUBA2/850em
creator_did          = ivo://CDS/P/SCUBA2/850em
obs_collection       = SCUBA2 850em
obs_title            = SCUBA2 850um
obs_description      = The SCUBA2-450em Hierarchical Progressive Survey (HiPS) has been built from JCMT data via CADC archive and distributed by CDS.It sets together all SCUBA2 observations done in 450 filter between the beginning of the mission to the 1st of November 2014. SCUBA-2: the 10 000 pixel bolometer camera on the James Clerk Maxwell Telescope.
obs_ack              = All publications based on SCUBA2 data should carry the following footnote: "The James Clerk Maxwell Telescope has historically been operated by the Joint Astronomy Centre on behalf of the Science and Technology Facilities Council of the United Kingdom, the National Research Council of Canada and the Netherlands Organisation for Scientific Research.
obs_copyright_url    = http://www.eaobservatory.org/jcmt/contact/
prov_progenitor      = JCMT via CADC - HiPSed by CDS
client_category      = Image/Radio/SCUBA
client_sort_key      = 05-01-02
hips_release_date    = 2019-05-05T06:55Z
hips_builder         = Aladin/HipsGen v10.123
hips_creator         = Fernique P. (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       = -350 1000
hips_data_range      = -10308 10792
hips_initial_ra      = 70.74095
hips_initial_dec     = +36.127
hips_initial_fov     = 0.53778
t_max                = 56962
t_max                = 56930
moc_access_url       = http://alasky.u-strasbg.fr/SCUBA2/Scuba2_850/Moc.fits
hips_progenitor_url  = https://alasky.cds.unistra.fr/SCUBA2/Scuba2_850/HpxFinder
hips_status          = public master clonableOnce
hips_copyright       = CNRS/Unistra
bib_reference        = 2013MNRAS.430.2513H
bib_reference_url    = http://simbad.u-strasbg.fr/simbad/sim-ref?bibcode=2013MNRAS.430.2513H&simbo=on
obs_copyright        = 2014-2017 East Asian Observatory all rights reserved
t_min                = 55228
obs_regime           = Radio
em_min               = 8.5E-4
em_max               = 8.5E-4
hips_pixel_scale     = 2.236E-4
moc_sky_fraction     = 0.02454
hips_estsize         = 226960936
hips_creation_date   = 2014-11-20T14:19Z
hips_order_min       = 0
hips_pixel_bitpix    = -64
hipsgen_date         = 2019-05-05T06:55Z
hipsgen_params       = out=/asd-volumes/sc1-asd-volume10/SCUBA2/Scuba2_850 UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/SCUBA2/Scuba2_850
hips_service_url_1   = https://alaskybis.cds.unistra.fr/SCUBA2/Scuba2_850
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 41
moc_time_range       = 12742
moc_order            = 9
obs_initial_ra       = 70.74095
obs_initial_dec      = +36.127
obs_initial_fov      = 0.11451621372724685
TIMESTAMP            = 1701291900435
,
ID                   = CDS/P/SDSS9/color
creator_did          = ivo://CDS/P/SDSS9/color
obs_collection       = SDSS9 color
obs_title            = SDSS9 color
obs_description      = The Sloan Digital Sky Survey is a multi-filter imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico, United States. Data collection began in 2000, and the final imaging data release covers over 35% of the sky. This color composition is an CDS alternative to the orignal SLOAN color composition using the g, r an i original DR9 bands with a log transfer function and specifical cuts for each band.
obs_copyright        = SLOAN Digitized Sky Survey - Healpixed by CDS
obs_copyright_url    = http://www.sdss.org/
client_category      = Image/Optical/SDSS
client_sort_key      = 03-02-01
hips_creation_date   = 2013-12-18T09:42Z
hips_release_date    = 2019-05-05T06:57Z
hips_builder         = Aladin/HipsGen v10.123
hips_creator         = Boch T. (CDS)
hips_version         = 1.4
hips_order           = 10
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/SDSS/DR9/color/Moc.fits
hips_status          = public master clonableOnce
hips_initial_fov     = 0.4
hips_initial_ra      = 202.4695750
hips_initial_dec     = 47.1952583
hips_copyright       = CNRS/Unistra
obs_ack              = Sloan Digital Sky Survey
prov_progenitor      = SLOAN - http://www.sdss.org
t_min                = 54466
t_max                = 56899
obs_regime           = Optical
em_min               = 3.782e-7
em_max               = 8.389e-7
hips_pixel_scale     = 1.118E-4
moc_sky_fraction     = 0.3562
hips_estsize         = 54490670
hips_order_min       = 0
dataproduct_subtype  = color
hipsgen_date         = 2019-05-05T06:57Z
hipsgen_params       = out=/asd-volumes/sc1-asd-volume10/SDSS/DR9/color UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/SDSS/DR9/color
hips_progenitor_url  = https://alasky.cds.unistra.fr/SDSS/DR9/color/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/SDSS/DR9/color
hips_status_1        = public mirror clonableOnce
hips_service_url_2   = https://irsa.ipac.caltech.edu/data/hips/CDS/SDSS/DR9/color
hips_status_2        = public mirror unclonable
hips_service_url_3   = https://healpix.ias.u-psud.fr/CDS_P_SDSS9_color
hips_status_3        = public mirror unclonable
hips_service_url_4   = http://skies.esac.esa.int/SDSS9Color
hips_status_4        = public mirror unclonable
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 12
obs_initial_ra       = 202.4695750
obs_initial_dec      = 47.1952583
obs_initial_fov      = 0.014314526715905856
TIMESTAMP            = 1711279621771
,
ID                   = CDS/P/SDSS9/color-alt
creator_did          = ivo://CDS/P/SDSS9/color-alt
obs_collection       = SDSS9 color-alt
obs_title            = SDSS9 color (g, r, i CDS color composition)
obs_description      = The Sloan Digital Sky Survey is a multi-filter imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico, United States. Data collection began in 2000, and the final imaging data release covers over 35% of the sky. This color composition is an CDS alternative to the orignal SLOAN color composition using the g, r an i original DR9 bands with a log transfer function and specifical cuts for each band.
hips_creator         = Fernique P. (CDS)
hips_copyright       = CNRS/Unistra
obs_ack              = Sloan Digital Sky Survey
prov_progenitor      = SLOAN - http://www.sdss.org
obs_copyright        = Sloan Digital Sky Survey
obs_copyright_url    = http://www.sdss.org/collaboration/#image-use
t_min                = 54466
t_max                = 56899
obs_regime           = Optical
client_category      = Image/Optical/SDSS
client_sort_key      = 03-02-00
client_application   = AladinDesktop
em_min               = 3.782e-7
em_max               = 8.389e-7
hips_builder         = Aladin/HipsGen v10.123
hips_version         = 1.4
hips_release_date    = 2019-05-05T14:52Z
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         = SDSS9 i [-16354.450801333003 -16072.227087528408 -15225.555946114624 Log]
hips_rgb_green       = SDSS9 r [-16362.606800614692 -16085.553958118306 -15439.097325626733 Log]
hips_rgb_blue        = SDSS9 g [-13898.937109723462 -12589.426315789473 -11092.842551293488 Log]
moc_sky_fraction     = 0.3562
hips_estsize         = 225482350
hips_creation_date   = 2016-05-24T10:01Z
hips_hierarchy       = first
hips_tile_format     = png
hipsgen_date         = 2016-05-29T00:46Z
hipsgen_params       = maxthread=6 inBlue=band-g inGreen=band-r inRed=band-i out=CDS-color-log cmBlue=0 1.4 3 log cmGreen=0 1.8 6 log cmRed=0 2.5 10 log method=first filter=gauss -f RGB
hips_initial_fov     = 0.014314526715905856
hips_initial_ra      = 45.0
hips_initial_dec     = 0.009325484987964084
hips_order_min       = 0
dataproduct_subtype  = color
hipsgen_date_1       = 2019-05-05T14:52Z
hipsgen_params_1     = out=/asd-volumes/sc1-asd-volume10/SDSS/DR9/color-alt UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/SDSS/DR9/color-alt
hips_service_url_1   = https://alaskybis.cds.unistra.fr/SDSS/DR9/color-alt
hips_status_1        = public mirror clonableOnce
hips_service_url_2   = https://healpix.ias.u-psud.fr/CDS_P_SDSS9_color-alt
hips_status_2        = public mirror unclonable
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 12
obs_initial_ra       = 45.0
obs_initial_dec      = 0.009325484987964084
obs_initial_fov      = 0.014314526715905856
TIMESTAMP            = 1711279432176
,
ID                   = CDS/P/SDSS9/g
creator_did          = ivo://CDS/P/SDSS9/g
obs_collection       = SDSS9 g
obs_title            = SDSS9 band g
obs_description      = The Sloan Digital Sky Survey is a multi-filter imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico, United States. Data Release 9 (DR9) offers the latest data from the Sloan Digital Sky Survey. Data Release 9 is the first release of the spectra from the SDSS-III's Baryon Oscillation Spectroscopic Survey (BOSS), which includes more than 800,000 spectra over 3,300 square degrees of sky, observed with the new 1,000-fiber BOSS spectrograph. Data Release 9 also includes all imaging and spectra from prior SDSS data releases, and provides corrected astrometry for the imaging from Data Release 8.
obs_ack              = Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/. SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University.
obs_copyright        = SLOAN Digitized Sky Survey - Healpixed by CDS
obs_copyright        = Sloan Digital Sky Survey
obs_copyright_url    = http://www.sdss.org/
obs_copyright_url    = http://www.sdss.org/collaboration/#image-use
client_category      = Image/Optical/SDSS
client_sort_key      = 03-02-03
prov_progenitor      = SLOAN
t_min                = 54466
t_max                = 56899
em_min               = 3.782e-7
em_max               = 5.549e-7
hips_builder         = Aladin/HipsGen v10.123
hips_version         = 1.4
hips_release_date    = 2019-05-06T08:37Z
hips_creator         = Boch T. (CDS)
hips_frame           = equatorial
hips_order           = 10
hips_tile_width      = 512
hips_tile_format     = png jpeg fits
hips_pixel_bitpix    = 16
data_pixel_bitpix    = -32
hips_hierarchy       = mean
hips_pixel_cut       = 0 1.8
hips_data_range      = -20.17 49.89
hips_initial_ra      = 0
hips_initial_dec     = +10
hips_initial_fov     = 70
hips_pixel_scale     = 1.118E-4
s_pixel_scale        = 1.099E-4
dataproduct_type     = image
moc_sky_fraction     = 0.3786
hips_estsize         = 3418408328
hips_creation_date   = 2016-01-17T03:25Z
moc_access_url       = http://alasky.u-strasbg.fr/SDSS/DR9/band-g/Moc.fits
hips_status          = public master clonableOnce
hips_copyright       = CNRS/Unistra
obs_regime           = Optical
hips_order_min       = 0
hipsgen_date         = 2019-05-06T08:37Z
hipsgen_params       = out=/asd-volumes/sc1-asd-volume10/SDSS/DR9/band-g UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/SDSS/DR9/band-g
hips_progenitor_url  = https://alasky.cds.unistra.fr/SDSS/DR9/band-g/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/SDSS/DR9/band-g
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 36
moc_time_range       = 813
moc_order            = 8
obs_initial_ra       = 0
obs_initial_dec      = +10
obs_initial_fov      = 0.2290324274544937
TIMESTAMP            = 1696351585922
,
ID                   = CDS/P/SDSS9/i
creator_did          = ivo://CDS/P/SDSS9/i
obs_collection       = SDSS9 i
obs_title            = SDSS9 band i
obs_description      = The Sloan Digital Sky Survey is a multi-filter imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico, United States. Data Release 9 (DR9) offers the latest data from the Sloan Digital Sky Survey. Data Release 9 is the first release of the spectra from the SDSS-III's Baryon Oscillation Spectroscopic Survey (BOSS), which includes more than 800,000 spectra over 3,300 square degrees of sky, observed with the new 1,000-fiber BOSS spectrograph. Data Release 9 also includes all imaging and spectra from prior SDSS data releases, and provides corrected astrometry for the imaging from Data Release 8.
obs_ack              = Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/. SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University.
obs_copyright        = SLOAN Digitized Sky Survey - Healpixed by CDS
obs_copyright_url    = http://www.sdss.org/
client_category      = Image/Optical/SDSS
client_sort_key      = 03-02-05
hips_release_date    = 2019-05-06T08:42Z
hips_builder         = Aladin/HipsGen v10.123
hips_creator         = Boch T. (CDS)
hips_version         = 1.4
hips_order           = 10
hips_frame           = equatorial
hips_tile_width      = 512
hips_tile_format     = png jpeg fits
dataproduct_type     = image
hips_pixel_cut       = 0 6
hips_data_range      = -145.4 435.1
hips_initial_ra      = 0
hips_initial_dec     = +10
hips_initial_fov     = 70
moc_access_url       = http://alasky.u-strasbg.fr/SDSS/DR9/band-i/Moc.fits
hips_progenitor_url  = https://alasky.cds.unistra.fr/SDSS/DR9/band-i/HpxFinder
hips_status          = public master clonableOnce
hips_copyright       = CNRS/Unistra
prov_progenitor      = SLOAN
t_min                = 54466
t_max                = 56899
obs_regime           = Optical
em_min               = 6.689e-7
em_max               = 8.389e-7
hips_pixel_scale     = 1.118E-4
moc_sky_fraction     = 0.3562
hips_estsize         = 3418382846
hips_creation_date   = 2014-12-17T22:14Z
hips_order_min       = 0
hips_pixel_bitpix    = 16
hipsgen_date         = 2019-05-06T08:42Z
hipsgen_params       = out=/asd-volumes/sc1-asd-volume10/SDSS/DR9/band-i UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/SDSS/DR9/band-i
hips_service_url_1   = https://alaskybis.cds.unistra.fr/SDSS/DR9/band-i
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 12
obs_initial_ra       = 0
obs_initial_dec      = +10
obs_initial_fov      = 0.014314526715905856
TIMESTAMP            = 1696351586014
,
ID                   = CDS/P/SDSS9/r
creator_did          = ivo://CDS/P/SDSS9/r
obs_collection       = SDSS9 r
obs_title            = SDSS9 band r
obs_description      = The Sloan Digital Sky Survey is a multi-filter imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico, United States. Data Release 9 (DR9) offers the latest data from the Sloan Digital Sky Survey. Data Release 9 is the first release of the spectra from the SDSS-III's Baryon Oscillation Spectroscopic Survey (BOSS), which includes more than 800,000 spectra over 3,300 square degrees of sky, observed with the new 1,000-fiber BOSS spectrograph. Data Release 9 also includes all imaging and spectra from prior SDSS data releases, and provides corrected astrometry for the imaging from Data Release 8.
obs_ack              = Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/. SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University.
obs_copyright        = SLOAN Digitized Sky Survey - Healpixed by CDS
obs_copyright_url    = http://www.sdss.org/
client_category      = Image/Optical/SDSS
client_sort_key      = 03-02-04
hips_builder         = Aladin/HipsGen v10.123
hips_version         = 1.4
hips_release_date    = 2019-05-05T06:58Z
hips_creator         = Boch T. (CDS)
hips_frame           = equatorial
hips_creation_date   = 2014-02-28T05:53Z
hips_creation_date   = 2015-12-03T05:51Z
hips_order           = 10
hips_tile_width      = 512
hips_tile_format     = png jpeg fits
hips_pixel_bitpix    = 16
data_pixel_bitpix    = -32
dataproduct_type     = image
hips_hierarchy       = mean
hips_pixel_cut       = 0 3
hips_data_range      = -106.6 319.2
hips_initial_ra      = 0
hips_initial_dec     = +10
hips_initial_fov     = 70
hips_pixel_scale     = 1.118E-4
s_pixel_scale        = 1.099E-4
moc_sky_fraction     = 0.3786
hips_estsize         = 3418479528
moc_access_url       = http://alasky.u-strasbg.fr/SDSS/DR9/band-r/Moc.fits
hips_status          = public master clonableOnce
hips_copyright       = CNRS/Unistra
prov_progenitor      = SLOAN
t_min                = 54466
t_max                = 56899
obs_regime           = Optical
em_min               = 5.415e-7
em_max               = 6.989e-7
hips_order_min       = 0
hipsgen_date         = 2019-05-05T06:58Z
hipsgen_params       = out=/asd-volumes/sc1-asd-volume10/SDSS/DR9/band-r UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/SDSS/DR9/band-r
hips_progenitor_url  = https://alasky.cds.unistra.fr/SDSS/DR9/band-r/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/SDSS/DR9/band-r
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 36
moc_time_range       = 815
moc_order            = 8
obs_initial_ra       = 0
obs_initial_dec      = +10
obs_initial_fov      = 0.2290324274544937
TIMESTAMP            = 1696351586102
,
ID                   = CDS/P/SDSS9/u
creator_did          = ivo://CDS/P/SDSS9/u
obs_collection       = SDSS9 u
obs_title            = SDSS9 band u
obs_description      = The Sloan Digital Sky Survey is a multi-filter imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico, United States. Data Release 9 (DR9) offers the latest data from the Sloan Digital Sky Survey. Data Release 9 is the first release of the spectra from the SDSS-III's Baryon Oscillation Spectroscopic Survey (BOSS), which includes more than 800,000 spectra over 3,300 square degrees of sky, observed with the new 1,000-fiber BOSS spectrograph. Data Release 9 also includes all imaging and spectra from prior SDSS data releases, and provides corrected astrometry for the imaging from Data Release 8.
obs_ack              = Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/. SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University.i
obs_copyright        = SLOAN Digitized Sky Survey - Healpixed by CDS
obs_copyright_url    = http://www.sdss.org/
client_category      = Image/Optical/SDSS
client_sort_key      = 03-02-02
hips_release_date    = 2019-05-05T07:02Z
hips_builder         = Aladin/HipsGen v10.123
hips_creator         = Boch T. (CDS)
hips_version         = 1.4
hips_order           = 10
hips_frame           = equatorial
hips_tile_width      = 512
hips_tile_format     = png jpeg fits
dataproduct_type     = image
hips_pixel_cut       = 0 2
hips_data_range      = -17.29 50.93
hips_initial_ra      = 0
hips_initial_dec     = +10
hips_initial_fov     = 70
moc_access_url       = http://alasky.u-strasbg.fr/SDSS/DR9/band-u/Moc.fits
hips_progenitor_url  = https://alasky.cds.unistra.fr/SDSS/DR9/band-u/HpxFinder
hips_status          = public master clonableOnce
hips_copyright       = CNRS/Unistra
prov_progenitor      = SLOAN
t_min                = 54466
t_max                = 56899
obs_regime           = Optical
em_min               = 3.048e-7
em_max               = 4.028e-7
hips_pixel_scale     = 1.118E-4
moc_sky_fraction     = 0.3786
hips_estsize         = 3418487022
hips_creation_date   = 2015-02-11T20:58Z
hips_order_min       = 0
hips_pixel_bitpix    = 16
hipsgen_date         = 2019-05-05T07:02Z