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ID                   = CDS/B/gcvs/gcvs_cat
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obs_description      = The XMM-Newton Observation log (2024-11-04)
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moc_access_url       = https://alasky.unistra.fr/footprints/tables/vizier/B_xmm_xmmlog/MOC?nside=2048
bib_reference        = 2002yCat....102009X
obs_description_url  = https://cdsarc.u-strasbg.fr/viz-bin/cat/B/xmm
obs_copyright_url    = https://cdsarc.u-strasbg.fr/viz-bin/cat/B/xmm
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obs_collection       = GALFA-HI Narrow
obs_title            = GALFA-HI Narrow
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prov_progenitor      = GALFA-HI Data Archive
obs_copyright_url    = https://purcell.ssl.berkeley.edu
bib_reference        = 2011ApJS..194...20P
bib_reference_url    = http://cdsads.u-strasbg.fr/abs/2011ApJS..194...20P
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obs_title            = GALFAHI Narrow DR2
obs_collection       = GALFAHI Narrow DR2
obs_description      = The Galactic Arecibo L-Band Feed Array H I (GALFA-H I) survey data release 2 (DR2) covers the 21 cm hyperfine transition of Galactic H I from -650 to 650 km s-1, with 0.184 km s-1 channel spacing, 4' angular resolution, and 150 mK rms noise per 1 km s-1 velocity channel. DR2 covers the entirety of the sky available from the William E. Gordon 305 m antenna at Arecibo, from decl. -1deg17' to decl. + 37deg57' across all R.A.: 4 steradians or 32% of the sky. DR2 differs in a number of ways from data release 1, which was released in 2011. DR2 is built from a largely separate set of observations from DR1, which were taken in a much more consistent mode. This consistency, coupled with more careful attention to systematics and more advanced data reduction algorithms, leads to a much higher-quality DR2 data product. We present three data sets for public use: H I data cubes, far-sidelobe stray-radiation-corrected column density maps, and results of the Rolling Hough Transform linear feature detection algorithm.
hips_creator         = Buga M. (CDS)
hips_copyright       = CNRS/Unistra
obs_ack              = We use data from Galactic ALFA HI (GALFA HI) survey data set obtained with the Arecibo L-band Feed Array (ALFA) on the Arecibo 305m telescope. The Arecibo Observatory is operated by SRI International under a cooperative agreement with the National Science Foundation (AST-1100968), and in alliance with Ana G. Mendez-Universidad Metropolitana, and the Universities Space Research Association. The GALFA HI surveys have been funded by the NSF through grants to Columbia University, the University of Wisconsin, and the University of California.
prov_progenitor      = GALFA-HI Data Archive
bib_reference        = 2018ApJS..234....2P
bib_reference_url    = https://ui.adsabs.harvard.edu/?#abs/2018ApJS..234....2P
obs_copyright        = Regents of the University of Calfornia
obs_copyright_url    = https://purcell.ssl.berkeley.edu/
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hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_cut       = 1.5 30
hips_data_range      = -8.004 87.15
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dataproduct_type     = cube
hips_cube_depth      = 2048
hips_cube_firstframe  = 1024
data_cube_crpix3     = 1024.5
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hipsgen_date_1       = 2018-04-11T00:19Z
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hipsgen_date_4       = 2018-04-12T21:38Z
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hipsgen_date_5       = 2019-05-22T07:24Z
hipsgen_params_5     = out=/asd-volumes/sc1-asd-volume6/GALFAHI/GALFAHI-Narrow-DR2 UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/GALFAHI/GALFAHI-Narrow-DR2
hips_progenitor_url  = https://alasky.cds.unistra.fr/GALFAHI/GALFAHI-Narrow-DR2/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/GALFAHI/GALFAHI-Narrow-DR2
hips_status_1        = public mirror clonableOnce
client_category      = Cube
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creator_did          = ivo://CDS/C/GALFAHI/Wide/DR2
obs_title            = GALFAHI Wide DR2
obs_collection       = GALFAHI Wide DR2
obs_description      = The Galactic Arecibo L-Band Feed Array H I (GALFA-H I) survey data release 2 (DR2) covers the 21 cm hyperfine transition of Galactic H I from -650 to 650 km s-1, with 0.184 km s-1 channel spacing, 4' angular resolution, and 150 mK rms noise per 1 km s-1 velocity channel. DR2 covers the entirety of the sky available from the William E. Gordon 305 m antenna at Arecibo, from decl. -1deg17' to decl. + 37deg57' across all R.A.: 4 steradians or 32% of the sky. DR2 differs in a number of ways from data release 1, which was released in 2011. DR2 is built from a largely separate set of observations from DR1, which were taken in a much more consistent mode. This consistency, coupled with more careful attention to systematics and more advanced data reduction algorithms, leads to a much higher-quality DR2 data product. We present three data sets for public use: H I data cubes, far-sidelobe stray-radiation-corrected column density maps, and results of the Rolling Hough Transform linear feature detection algorithm.
hips_creator         = Buga M. (CDS)
hips_copyright       = CNRS/Unistra
obs_ack              = We use data from Galactic ALFA HI (GALFA HI) survey data set obtained with the Arecibo L-band Feed Array (ALFA) on the Arecibo 305m telescope. The Arecibo Observatory is operated by SRI International under a cooperative agreement with the National Science Foundation (AST-1100968), and in alliance with Ana G. Mendez-Universidad Metropolitana, and the Universities Space Research Association. The GALFA HI surveys have been funded by the NSF through grants to Columbia University, the University of Wisconsin, and the University of California.
prov_progenitor      = GALFA-HI Data Archive
bib_reference        = 2018ApJS..234....2P
bib_reference_url    = https://ui.adsabs.harvard.edu/?#abs/2018ApJS..234....2P
obs_copyright        = Regents of the University of Calfornia
obs_copyright_url    = https://purcell.ssl.berkeley.edu/
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hips_sampling        = bilinear
hips_overlay         = mean
hips_hierarchy       = median
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hips_version         = 1.4
hips_release_date    = 2019-05-21T22:30Z
hips_frame           = equatorial
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hips_tile_width      = 512
hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_cut       = 1.5 30
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s_pixel_scale        = 0.01667
dataproduct_type     = cube
hips_cube_depth      = 2048
hips_cube_firstframe  = 1024
data_cube_crpix3     = 1024.5
data_cube_crval3     = 0.0
data_cube_cdelt3     = 736.1228396
data_cube_bunit3     = null
moc_sky_fraction     = 0.3217
hips_estsize         = 495097856
hipsgen_date         = 2018-04-16T15:35Z
hipsgen_params       = in=GALFA_HI2_W/ out=/data2/buga/HIPS_GALFA_HI2_W creator_did=ivo://CDS/C/GALFAHI/Wide/DR2 verbose=4 "hips_pixel_cut=1.5 30" INDEX TILES PNG DETAILS
hips_creation_date   = 2018-04-16T15:35Z
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hipsgen_params_2     = out=/asd-volumes/sc1-asd-volume6/GALFAHI/GALFAHI-Wide-DR2 UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/GALFAHI/GALFAHI-Wide-DR2
hips_progenitor_url  = https://alasky.cds.unistra.fr/GALFAHI/GALFAHI-Wide-DR2/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/GALFAHI/GALFAHI-Wide-DR2
hips_status_1        = public mirror clonableOnce
client_category      = Cube
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 8
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ID                   = CDS/C/HI4PI/HI
creator_did          = ivo://CDS/C/HI4PI/HI
obs_collection       = HI4PI HI
obs_title            = HI4PI HI survey (individual cubes)
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
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hipsgen_date         = 2017-06-23T16:54Z
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hips_progenitor_url  = https://alasky.cds.unistra.fr/HI4PI/C_HI4PI_HI/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/HI4PI/C_HI4PI_HI
hips_status_1        = public mirror clonableOnce
client_category      = Cube
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moc_time_range       = 1
moc_order            = 8
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,
ID                   = CDS/C/HIPASS
creator_did          = ivo://CDS/C/HIPASS
obs_title            = HIPASS
obs_collection       = HIPASS
obs_description      = The `HI Parkes All Sky Survey' (HIPASS) covers the whole southern sky as well as northern declinations up to +25 degrees. HIPASS commenced in Feb 1997, and the last northern scans were taken in 2002. HIPASS was carried out with the Australia Telescope National Facility's Parkes telescope Parkes 64-m telescope equipped with a novel 21-cm multibeam system. The latter comprises a cooled, 13 beam receiver and digital correlator (Staveley-Smith et al. 1996, Wilson et al. 1997 and Sinclair et al. 1997). The 64 MHz observing band, centred on 1394.5 MHz, was divided into 1024 channels, providing a velocity range of -1280 < cz < 12700 km/s with a channel width of approx. 13.2 km/s and a velocity resolution of 18 km/s. The HIPASS integration time per beam is 450s. After gridding an r.m.s. noise of about 13.3 mJy was achieved in the first set of HIPASS cubes. The observations and techniques used to calibrate and image the data are described in Barnes et al. (2001). The processing algorithms are successfully designed to be statistically robust to the presence of interference signals and are particular to imaging point (or nearly point) sources, not extended emission. Specifically, a major improvement in image quality is obtained by designing a median-gridding algorithm which uses the median estimator in place of the mean estimator. While the average Parkes beam FWHM is 14.3 arcmin, the average gridded HIPASS beam is about 15.5 arcmin. The full data release contains data from 538 data cubes (size: 8o x 8o, 388 over the entire southern sky (DEC < +2o), and 150 over the northern sky, (DEC < +25o). The one-dimensional spectral data for a given position is available for downloading in a variety of different formats.
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hips_overlay         = mean
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hips_creator         = Lutz K. (CDS) , Buga M. (CDS)
hips_copyright       = CNRS/Unistra
obs_ack              = The Parkes telescope is part of the Australia Telescope which is funded by the Commonwealth of Australia for operation as a National Facility managed by CSIRO.
prov_progenitor      = https://doi.org/10.25919/5c36de6d37141
bib_reference        = 2001MNRAS.322..486B
bib_reference_url    = https://ui.adsabs.harvard.edu/?#abs/2001MNRAS.322..486B
obs_copyright        = Creative Commons Attribution 4.0 International Licence: Koribalski, Baerbel; Staveley-Smith, Lister (2004): The HI Parkes All Sky Survey (HIPASS) image cubes. v1. CSIRO. Data Collection. 102.100.100/70188 https://doi.org/10.25919/5c36de6d37141
obs_copyright_url    = https://data.csiro.au/dap/landingpage?pid=csiro:32333
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hips_version         = 1.4
hips_release_date    = 2019-05-22T15:01Z
hips_frame           = equatorial
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hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_cut       = -0.0135 0.19
hips_data_range      = -0.606 0.688
hips_pixel_scale     = 0.01431
s_pixel_scale        = 0.06667
dataproduct_type     = cube
hips_cube_depth      = 1024
hips_cube_firstframe  = 512
moc_sky_fraction     = 0.7708
hips_estsize         = 457960448
hipsgen_date         = 2019-01-18T04:29Z
hipsgen_params       = maxthread=6 in=ALL_HIPASS/ out=HIPASS_HiPS creator_did=CDS/P/HIPASS "hips_pixel_cut=-0.0135 0.19"
hips_creation_date   = 2019-01-18T04:29Z
hipsgen_date_1       = 2019-01-18T22:14Z
hipsgen_params_1     = maxthread=6 in=ALL_HIPASS/ out=HIPASS_HiPS creator_did=CDS/P/HIPASS "hips_pixel_cut=-0.0135 0.19"
hipsgen_date_2       = 2019-05-22T15:01Z
hipsgen_params_2     = out=/asd-volumes/sc1-asd-volume2/HIPASS UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/HIPASS
hips_progenitor_url  = https://alasky.cds.unistra.fr/HIPASS/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/HIPASS
hips_status_1        = public mirror clonableOnce
client_category      = Cube
moc_type             = stmoc
moc_time_order       = 41
moc_time_range       = 538
moc_order            = 3
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obs_initial_fov      = 7.3290376785437985
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ID                   = CDS/I/100A/w10
publisher_id         = ivo://CDS
obs_id               = I/100A/w10
obs_title            = Results of obs with the 6-inch transit circle (Hammond+ 1927-1982) (w10)
obs_description      = W210
nb_rows              = 2428
obs_regime           = Optical
obs_astronomy_kw     = Proper_Motions
obs_astronomy_kw     = Stars
obs_astronomy_kw     = Positional_Data
vizier_popularity    = 1
data_ucd             = time.epoch
data_ucd             = phot.mag;em.opt.V
data_ucd             = pos.eq.ra
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ID                   = CDS/I/243/out
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ID                   = CDS/I/246/act
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ID                   = CDS/I/247/ac2000
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ID                   = CDS/I/248/catalog
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ID                   = CDS/I/250/catalog
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obs_astronomy_kw     = Positional_Data
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,
ID                   = CDS/III/223/mk12
publisher_id         = ivo://CDS
obs_id               = III/223/mk12
obs_title            = 12th General Catalogue of MK Spectral Classification (Buscombe+ 1995) (mk12)
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,
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publishe