ID                   = CDS/C/CALIFA/V500/DR2
creator_did          = ivo://CDS/C/CALIFA/V500/DR2
obs_collection       = The Calar Alto Legacy Integral Field Area survey - V500 resolution mode (CALIFA V500) DR2
obs_title            = CALIFA DR2 V500 (R~850, 3750-7500 A)
obs_description      = The Calar Alto Legacy Integral Field Area survey is one of the largest IFS surveys performed to date. At its completion it will comprise 600 galaxies, observed with the PMAS spectrograph in the PPAK mode, covering the full spatial extent of these galaxies up to two effective radii. The wavelength range between 3700 and 7500 is sampled with two spectroscopic configurations, a high resolution mode (V1200, R~1700, 3700-4200), and a low resolution mode (V500, R~850, 3750-7500). A detailed explanation of the survey is given in the CALIFA Presentation Article (Sanchez et al. 2012). The second CALIFA Data Release (DR2) provides to the public the fully reduced and quality control tested datacubes of 200 objects in both setups (V500 and V1200). Each datacube contains ~1000 independent spectra, thus in total this DR comprises ~400,000 total independent spectra (~1.5 millon after cube reconstruction). The details of the data included in this DR are described in the CALIFA DR2 Article (Garcia Benito et al. 2014). The differences in the data reduction pipeline adopted for this dataset are described in this article too, in comparison with the current solution adopted for DR1 (Husemann et al. 2013)
obs_ack              = This study makes uses of the data provided by the Calar Alto Legacy Integral Field Area (CALIFA) survey
obs_copyright        = Based on observations collected at the Centro Astronomico Hispano Aleman (CAHA) at Calar Alto, operated jointly by the Max-Planck-Institut fur Astronomie and the Instituto de Astrofisica de Andalucia (CSIC)
obs_copyright_url    = http://www.caha.es/CALIFA/public_html/?q=content/califa-2nd-data-release
hips_release_date    = 2019-05-20T09:23Z
hips_builder         = Aladin/HipsGen v10.125
hips_version         = 1.4
hips_creation_date   = 2014-12-04T22:24Z
hips_creator         = Fernique P. (CDS)
hips_frame           = equatorial
hips_initial_ra      = 169.58868
hips_initial_dec     = +45.74914
hips_tile_width      = 512
hips_order           = 9
hips_pixel_cut       = 0 0.4641
hips_data_range      = -0.244 0.7321
hips_tile_format     = png
dataproduct_type     = cube
hips_initial_fov     = 0.02139
hips_cube_depth      = 1877
hips_cube_firstframe  = 938
moc_sky_fraction     = 2.937E-4
hips_estsize         = 26249845
client_category      = Cube
data_cube_crpix3     = 22
data_cube_crval3     = 2408000
data_cube_cdelt3     = -10305.46094
hips_status          = public master clonableOnce
hips_copyright       = CNRS/Unistra
prov_progenitor      = CAHA
bib_reference        = 2015A&A...576A.135G
bib_reference_url    = http://adsabs.harvard.edu/abs/2014arXiv1409.8302G
t_min                = 55348
t_max                = 56627
obs_regime           = Optical
em_min               = 3.75E-7
em_max               = 7.5E-7
hips_hierarchy       = mean
hips_pixel_scale     = 2.236E-4
order                = 9
hips_order_min       = 0
hipsgen_date         = 2019-05-20T09:23Z
hipsgen_params       = out=/asd-volumes/sc1-asd-volume6/CALIFA/V500DR2 UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/CALIFA/V500DR2
hips_progenitor_url  = https://alasky.cds.unistra.fr/CALIFA/V500DR2/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/CALIFA/V500DR2
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 8
obs_initial_ra       = 169.58868
obs_initial_dec      = +45.74914
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TIMESTAMP            = 1696351589138

ID                   = CDS/C/CGPS-HI
hips_doi             = 10.26093/cds/aladin/jkaj-0n
creator_did          = ivo://CDS/C/CGPS-HI
obs_collection       = Canadian Galactic Plane Survey data cubes HI (21cm)
obs_title            = CGPS data cubes HI (21cm)
obs_description      = The Dominion Radio Astrophysical Observatory, in collaboration with an international Consortium of astronomers, has carried out a high-resolution survey of the atomic hydrogen and radio continuum emission from our Milky Way galaxy. The observations of 373 fields with the DRAO Synthesis Telescope are presented in sixty-eight 5 deg x 5 deg mosaics, covering Galactic longitudes from L = 63 to 175 degrees and latitudes from B = -3.5 to +5.5 degrees and a latitude extension to B = +17.5 degrees between L = 100 to 116.5 degrees, with a resolution as small as 1 arcminute. For each mosaic (1024 x 1024 pixels), atomic hydrogen observations are presented as a data "cube" with 272 spectral channels having a velocity resolution of 1.3 km/s. Stokes I continuum images at 1420 MHz and 408 MHz are produced, as well as selected Stokes Q, U and V images at 1420 MHz. Complementary images in the four IRAS infrared bands and data cubes of CO (J=1-0) emission have also been created as part of the Survey.
bib_reference        = 2003AJ....125.3145T
bib_reference_url    = http://adsabs.harvard.edu/cgi-bin/bib_query?2003AJ....125.3145T&db_key=AST
obs_copyright_url    = http://www.ras.ucalgary.ca/CGPS/
obs_progenitor       = CADC
obs_ack              = This HiPS has used data from the Canadian Galactic Plane Survey, a Canadian project with international partners, supported by the Natural Sciences and Engineering Research Council
hips_release_date    = 2019-05-05T05:51Z
hips_builder         = Aladin/HipsGen v10.123
hips_order           = 5
hips_pixel_cut       = 6.599 124.1
hips_tile_format     = png fits
hips_cube_depth      = 272
hips_cube_firstframe  = 136
hips_frame           = equatorial
dataproduct_type     = cube
t_min                = 49808
t_max                = 51635
em_min               = 2.111E-1
em_max               = 7.347E-1
hips_version         = 1.4
hips_creation_date   = 2014-04-07T15:24Z
hips_creator         = Fernique P. (CDS)
hips_tile_width      = 512
moc_access_url       = http://alasky.u-strasbg.fr/CGPS/Moc.fits
hips_status          = public master clonableOnce
hips_pixel_bitpix    = 16
hips_hierarchy       = mean
hips_pixel_scale     = 0.003579
moc_sky_fraction     = 0.03684
hips_estsize         = 114948832
client_category      = Cube
data_cube_crpix3     = 145
data_cube_crval3     = -6.000000000000E+04
data_cube_cdelt3     = -8.2446002E+02
data_cube_bunit3     = m/s
order                = 5
hips_copyright       = CNRS/Unistra
prov_progenitor      = CGPS/RCPG
obs_copyright        = The following materials are copyrighted by the Canadian Galactic Plane Survey/Releve Canadien du Plan Galactique (CGPS/RCPG). They are intended as a news release material and for use for educational, academic, and research purposes and are not intended for commercial sale. Please contact Jayanne English (email: jayanne_english@umanitoba.ca) to inquire about permission for other non-commercial and/or commercial uses
obs_regime           = Radio
hips_initial_fov     = 30
hips_initial_ra      = 343
hips_initial_dec     = 62
hips_order_min       = 0
hipsgen_date         = 2019-05-05T05:51Z
hipsgen_params       = out=/asd-volumes/sc1-asd-volume10/CGPS UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/CGPS
hips_progenitor_url  = https://alasky.cds.unistra.fr/CGPS/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/CGPS
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 8
obs_initial_ra       = 343
obs_initial_dec      = 62
obs_initial_fov      = 0.2290324274544937
TIMESTAMP            = 1702419493712

ID                   = CDS/C/DM/simbad-biblio/pub-dates/1970-now
client_category      = Cube
hips_copyright       = © Université de Strasbourg - CNRS. All rights reserved
obs_copyright        = © Université de Strasbourg - CNRS. All rights reserved
client_sort_key      = B
hips_initial_fov     = 58.63230142835039
hips_initial_ra      = 0
hips_initial_dec     = +0
creator_did          = ivo://CDS/C/DM/simbad-biblio/pub-dates/1970-now
obs_title            = Simbad heatmap - 1990-now
obs_title_0          = DM simbad-biblio pub-dates 1991
obs_title_1          = DM simbad-biblio pub-dates 1992
obs_title_2          = DM simbad-biblio pub-dates 1993
obs_title_3          = DM simbad-biblio pub-dates 1994
obs_title_4          = DM simbad-biblio pub-dates 1995
obs_title_5          = DM simbad-biblio pub-dates 1996
obs_title_6          = DM simbad-biblio pub-dates 1997
obs_title_7          = DM simbad-biblio pub-dates 1998
obs_title_8          = DM simbad-biblio pub-dates 1999
obs_title_9          = DM simbad-biblio pub-dates 2000
obs_title_10         = DM simbad-biblio pub-dates 2001
obs_title_11         = DM simbad-biblio pub-dates 2002
obs_title_12         = DM simbad-biblio pub-dates 2003
obs_title_13         = DM simbad-biblio pub-dates 2004
obs_title_14         = DM simbad-biblio pub-dates 2005
obs_title_15         = DM simbad-biblio pub-dates 2006
obs_title_16         = DM simbad-biblio pub-dates 2007
obs_title_17         = DM simbad-biblio pub-dates 2008
obs_title_18         = DM simbad-biblio pub-dates 2009
obs_title_19         = DM simbad-biblio pub-dates 2010
obs_title_20         = DM simbad-biblio pub-dates 2011
obs_title_21         = DM simbad-biblio pub-dates 2012
obs_title_22         = DM simbad-biblio pub-dates 2013
obs_title_23         = DM simbad-biblio pub-dates 2014
obs_title_24         = DM simbad-biblio pub-dates 2015
obs_title_25         = DM simbad-biblio pub-dates 2016
obs_title_26         = DM simbad-biblio pub-dates 2017
obs_title_27         = DM simbad-biblio pub-dates 2018
obs_title_28         = DM simbad-biblio pub-dates 2019
hips_creator         = CDS Simbad
hips_builder         = Aladin/HipsGen v11.025
hips_version         = 1.4
hips_release_date    = 2021-03-03T10:07Z
hips_frame           = equatorial
hips_order           = 3
hips_tile_width      = 64
hips_status          = public mirror unclonable
hips_tile_format     = fits png
hips_pixel_bitpix    = -32
hips_pixel_cut       = -8.714E-4 4.421
hips_data_range      = -16.25 48.73
hips_pixel_scale     = 0.1145
hips_pixel_scale     = 0.01431
moc_sky_fraction     = 1
hips_estsize         = 19790
hips_estsize         = 890460
dataproduct_type     = cube
hips_cube_depth      = 30
hips_cube_firstframe  = 15
hipsgen_date         = 2019-11-05T12:56Z
hipsgen_params       = in=/data/hips-simbad/data/simbad-biblio//1991;/data/hips-simbad/data/simbad-biblio//1992;/data/hips-simbad/data/simbad-biblio//1993;/data/hips-simbad/data/simbad-biblio//1994;/data/hips-simbad/data/simbad-biblio//1995;/data/hips-simbad/data/simbad-biblio//1996;/data/hips-simbad/data/simbad-biblio//1997;/data/hips-simbad/data/simbad-biblio//1998;/data/hips-simbad/data/simbad-biblio//1999;/data/hips-simbad/data/simbad-biblio//2000;/data/hips-simbad/data/simbad-biblio//2001;/data/hips-simbad/data/simbad-biblio//2002;/data/hips-simbad/data/simbad-biblio//2003;/data/hips-simbad/data/simbad-biblio//2004;/data/hips-simbad/data/simbad-biblio//2005;/data/hips-simbad/data/simbad-biblio//2006;/data/hips-simbad/data/simbad-biblio//2007;/data/hips-simbad/data/simbad-biblio//2008;/data/hips-simbad/data/simbad-biblio//2009;/data/hips-simbad/data/simbad-biblio//2010;/data/hips-simbad/data/simbad-biblio//2011;/data/hips-simbad/data/simbad-biblio//2012;/data/hips-simbad/data/simbad-biblio//2013;/data/hips-simbad/data/simbad-biblio//2014;/data/hips-simbad/data/simbad-biblio//2015;/data/hips-simbad/data/simbad-biblio//2016;/data/hips-simbad/data/simbad-biblio//2017;/data/hips-simbad/data/simbad-biblio//2018;/data/hips-simbad/data/simbad-biblio//2019; out=/data/hips-simbad/data/simbad-biblio/cubes/1990-now creator_did=CDS/C/SIM cube
obs_title_29         = DM simbad-biblio pub-dates 2020
hips_creation_date   = 2019-11-05T12:56Z
hipsgen_date_1       = 2021-03-04T13:53Z
hipsgen_params_1     = in=/data/hips-simbad/data/simbad-biblio//1991;/data/hips-simbad/data/simbad-biblio//1992;/data/hips-simbad/data/simbad-biblio//1993;/data/hips-simbad/data/simbad-biblio//1994;/data/hips-simbad/data/simbad-biblio//1995;/data/hips-simbad/data/simbad-biblio//1996;/data/hips-simbad/data/simbad-biblio//1997;/data/hips-simbad/data/simbad-biblio//1998;/data/hips-simbad/data/simbad-biblio//1999;/data/hips-simbad/data/simbad-biblio//2000;/data/hips-simbad/data/simbad-biblio//2001;/data/hips-simbad/data/simbad-biblio//2002;/data/hips-simbad/data/simbad-biblio//2003;/data/hips-simbad/data/simbad-biblio//2004;/data/hips-simbad/data/simbad-biblio//2005;/data/hips-simbad/data/simbad-biblio//2006;/data/hips-simbad/data/simbad-biblio//2007;/data/hips-simbad/data/simbad-biblio//2008;/data/hips-simbad/data/simbad-biblio//2009;/data/hips-simbad/data/simbad-biblio//2010;/data/hips-simbad/data/simbad-biblio//2011;/data/hips-simbad/data/simbad-biblio//2012;/data/hips-simbad/data/simbad-biblio//2013;/data/hips-simbad/data/simbad-biblio//2014;/data/hips-simbad/data/simbad-biblio//2015;/data/hips-simbad/data/simbad-biblio//2016;/data/hips-simbad/data/simbad-biblio//2017;/data/hips-simbad/data/simbad-biblio//2018;/data/hips-simbad/data/simbad-biblio//2019;/data/hips-simbad/data/simbad-biblio/2020 out=/data/hips-simbad/data/simbad-biblio/cubes/1990-now creator_did=CDS/C/SIM cube
hips_service_url     = https://alaskybis.cds.unistra.fr/ancillary/simbad-biblio/cubes/1990-now
MOCSERVER_REMOVE     = true
moc_type             = smoc
moc_order            = 7
obs_initial_ra       = 0
obs_initial_dec      = +0
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TIMESTAMP            = 1676415318000

ID                   = CDS/C/GALFAHI/Narrow
creator_did          = ivo://CDS/C/GALFAHI/Narrow
obs_collection       = GALFA-HI Narrow
obs_title            = GALFA-HI Narrow
obs_description      = Data Release 1 (DR1) of the GALFA HI data set, obtained with the Arecibo L-band Feed Array (ALFA) on the Arecibo 305m telescope. This neutral hydrogen survey has a resolution of ~4', a spectral resolution of 0.18km/s for velocities -190 km/s<V<190 km/s. Details on the observations and this release are in Peek et al. 2011.
obs_ack              = Galactic ALFA HI (GALFA HI) survey data set obtained with the Arecibo L-band Feed Array (ALFA) on the Arecibo 305m telescope. Arecibo Observatory is part of the National Astronomy and Ionosphere Center, which is operated by Cornell University under Cooperative Agreement with the U.S. National Science Foundation. The GALFA HI surveys are funded by the NSF through grants to Columbia University, the University of Wisconsin, and the University of California. Peek, J.E.G et al. 2011, ApJS, 194, 20P
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
t_min                = 54587
t_max                = 55075
em_min               = 0.244728537142857
em_max               = 0.196585218360656
hips_builder         = Aladin/HipsGen v10.125
hips_version         = 1.4
hips_release_date    = 2019-05-20T11:13Z
hips_creator         = Bot C. (CDS)
hips_frame           = equatorial
hips_order           = 3
hips_tile_width      = 512
hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_bitpix    = 16
data_pixel_bitpix    = 16
hips_hierarchy       = mean
hips_pixel_cut       = 0 35
hips_data_range      = -15.02 53.09
hips_initial_ra      = 57.97088
hips_initial_dec     = +06.21575
hips_initial_fov     = 180
hips_pixel_scale     = 0.01431
s_pixel_scale        = 0.01667
dataproduct_type     = cube
hips_cube_depth      = 2048
hips_cube_firstframe  = 1024
moc_sky_fraction     = 0.3164
hips_estsize         = 422383616
hips_creation_date   = 2015-05-30T08:34Z
client_category      = Cube
data_cube_crpix3     = 1024.50
data_cube_crval3     = 0
data_cube_cdelt3     = 184.0307099
data_cube_bunit3     = m/s
order                = 3
hips_copyright       = CNRS/Unistra
obs_regime           = Radio
hips_order_min       = 0
hipsgen_date         = 2019-05-20T11:13Z
hipsgen_params       = out=/asd-volumes/sc1-asd-volume6/GALFAHI/GALFAHI-Narrow UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/GALFAHI/GALFAHI-Narrow
hips_progenitor_url  = https://alasky.cds.unistra.fr/GALFAHI/GALFAHI-Narrow/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/GALFAHI/GALFAHI-Narrow
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 8
obs_initial_ra       = 57.97088
obs_initial_dec      = +06.21575
obs_initial_fov      = 0.2290324274544937
TIMESTAMP            = 1696351589330

ID                   = CDS/C/GALFAHI/Narrow/DR2
creator_did          = ivo://CDS/C/GALFAHI/Narrow/DR2
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/
t_min                = 54784
t_max                = 56942
obs_regime           = Radio
em_min               = 0.244728537142857
em_max               = 0.196585218360656
hips_initial_fov     = 8.53335
hips_initial_ra      = 52.00878
hips_initial_dec     = +18.34167
hips_pixel_bitpix    = 16
data_pixel_bitpix    = 16
hips_sampling        = bilinear
hips_overlay         = mean
hips_hierarchy       = median
hips_builder         = Aladin/HipsGen v10.125
hips_version         = 1.4
hips_release_date    = 2019-05-22T07:24Z
hips_frame           = equatorial
hips_order           = 3
hips_order_min       = 0
hips_tile_width      = 512
hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_cut       = 1.5 30
hips_data_range      = -8.004 87.15
hips_pixel_scale     = 0.01431
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     = 184.0307099
data_cube_bunit3     = null
moc_sky_fraction     = 0.3217
hips_estsize         = 495097856
hipsgen_date         = 2018-04-10T20:25Z
hipsgen_params       = in=GALFA_HI2_N out=/data1/buga/HIPS_GALFA_HI2_N creator_did=ivo://CDS/C/GALFAHI/Narrow/DR2 verbose=4 maxthread=10 INDEX TILES PNG DETAILS
hips_creation_date   = 2018-04-10T20:25Z
hipsgen_date_1       = 2018-04-11T00:19Z
hipsgen_params_1     = in=GALFA_HI2_N out=/data1/buga/HIPS_GALFA_HI2_N creator_did=ivo://CDS/C/GALFAHI/Narrow/DR2 verbose=4 maxthread=10 INDEX TILES PNG DETAILS
hipsgen_date_2       = 2018-04-12T18:36Z
hipsgen_params_2     = in=GALFA_HI2_N out=/data1/buga/HIPS_GALFA_HI2_N creator_did=ivo://CDS/C/GALFAHI/Narrow/DR2 verbose=4 "hips_pixel_cut=1.5 30" -f INDEX TILES PNG DETAILS
hipsgen_date_3       = 2018-04-12T18:37Z
hipsgen_params_3     = in=GALFA_HI2_N out=/data1/buga/HIPS_GALFA_HI2_N creator_did=ivo://CDS/C/GALFAHI/Narrow/DR2 verbose=4 "hips_pixel_cut=1.5 30" -f INDEX TILES PNG DETAILS
hipsgen_date_4       = 2018-04-12T21:38Z
hipsgen_params_4     = in=GALFA_HI2_N out=/data1/buga/HIPS_GALFA_HI2_N creator_did=ivo://CDS/C/GALFAHI/Narrow/DR2 verbose=4 "hips_pixel_cut=1.5 30" -f INDEX TILES PNG DETAILS
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
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 8
obs_initial_ra       = 52.00878
obs_initial_dec      = +18.34167
obs_initial_fov      = 0.2290324274544937
TIMESTAMP            = 1696351637166

ID                   = CDS/C/GALFAHI/Wide/DR2
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/
t_min                = 54784
t_max                = 56942
obs_regime           = Radio
em_min               = 0.244728537142857
em_max               = 0.196585218360656
hips_initial_fov     = 8.53335
hips_initial_ra      = 108.00847
hips_initial_dec     = +10.34167
hips_pixel_bitpix    = 16
data_pixel_bitpix    = 16
hips_sampling        = bilinear
hips_overlay         = mean
hips_hierarchy       = median
hips_builder         = Aladin/HipsGen v10.125
hips_version         = 1.4
hips_release_date    = 2019-05-21T22:30Z
hips_frame           = equatorial
hips_order           = 3
hips_order_min       = 0
hips_tile_width      = 512
hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_cut       = 1.5 30
hips_data_range      = -12.61 61.06
hips_pixel_scale     = 0.01431
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
hipsgen_date_1       = 2018-04-16T18:04Z
hipsgen_params_1     = 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
hipsgen_date_2       = 2019-05-21T22:30Z
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
obs_initial_ra       = 108.00847
obs_initial_dec      = +10.34167
obs_initial_fov      = 0.2290324274544937
TIMESTAMP            = 1696351637078

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/s<vlsr<+600km/s for declination >0deg; -470km/s<vlsr<+470km/s for declination <0deg) as observed with the 100-m radio telescope at Effelsberg and the 64-m radio telescope at Parkes. HI4PI covers the full 4-pi sky.
hips_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    = 2019-05-22T07:48Z
hips_frame           = equatorial
hips_order           = 3
hips_tile_width      = 512
hips_status          = public master clonableOnce
hips_tile_format     = jpeg fits
hips_pixel_cut       = -0.05778 37.03
hips_data_range      = -107.1 229
hips_pixel_scale     = 0.01431
s_pixel_scale        = 0.08333
dataproduct_type     = cube
hips_cube_depth      = 945
hips_cube_firstframe  = 472
data_cube_crpix3     = 471.921630003202
data_cube_crval3     = 0.0
data_cube_cdelt3     = 1288.21496912415
data_cube_bunit3     = null
moc_sky_fraction     = 1
hips_estsize         = 1059828840
hipsgen_date         = 2017-06-23T16:54Z
hips_initial_fov     = 360.25
hips_initial_ra      = 266.47043
hips_initial_dec     = -28.9223
hips_pixel_bitpix    = -32
data_pixel_bitpix    = -32
hips_sampling        = bilinear
hips_overlay         = mean
hips_hierarchy       = median
hipsgen_params       = in=in out=/data2/buga/HI4PI -f ivorn=ivo://CDS/P/HI4PI/ALLSKY partitioning=false
hips_creation_date   = 2017-06-23T16:54Z
hipsgen_date_1       = 2017-06-23T19:52Z
hipsgen_params_1     = in=in out=/data2/buga/HI4PI -f ivorn=ivo://CDS/P/HI4PI/ALLSKY partitioning=false
hipsgen_date_2       = 2017-06-27T13:42Z
hipsgen_params_2     = in=in out=/data2/buga/ALLSKY -f ivorn=ivo://CDS/P/HI4PI/ALLSKY partitioning=false "pixelcut=-0.05778 37.03" CLEANPNG JPEG
hipsgen_date_3       = 2017-06-27T13:42Z
hipsgen_params_3     = in=in out=/data2/buga/ALLSKY -f ivorn=ivo://CDS/P/HI4PI/ALLSKY partitioning=false "pixelcut=-0.05778 37.03" CLEANPNG JPEG
hipsgen_date_4       = 2017-06-27T16:37Z
hipsgen_params_4     = in=in out=/data2/buga/ALLSKY -f ivorn=ivo://CDS/P/HI4PI/ALLSKY partitioning=false "pixelcut=-0.05778 37.03" CLEANPNG JPEG
hips_order_min       = 0
hipsgen_date_5       = 2019-05-22T07:49Z
hipsgen_params_5     = out=/asd-volumes/sc1-asd-volume6/HI4PI/C_HI4PI_HI UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/HI4PI/C_HI4PI_HI
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
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 8
obs_initial_ra       = 266.47043
obs_initial_dec      = -28.9223
obs_initial_fov      = 0.2290324274544937
TIMESTAMP            = 1696351629478

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.
hips_initial_fov     = 11.33333
hips_initial_ra      = 293.06869
hips_initial_dec     = +13.93332
hips_pixel_bitpix    = 16
data_pixel_bitpix    = 16
hips_sampling        = bilinear
hips_overlay         = mean
hips_hierarchy       = median
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
t_min                = 50491
t_max                = 52437
obs_regime           = Radio
em_min               = 0.21
em_max               = 0.21
hips_builder         = Aladin/HipsGen v10.125
hips_version         = 1.4
hips_release_date    = 2019-05-22T15:01Z
hips_frame           = equatorial
hips_order           = 3
hips_order_min       = 0
hips_tile_width      = 512
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
obs_initial_ra       = 293.06869
obs_initial_dec      = +13.93332
obs_initial_fov      = 7.3290376785437985
TIMESTAMP            = 1696351642990

ID                   = CDS/C/MUSE-M42
creator_did          = ivo://CDS/C/MUSE-M42
obs_collection       = MUSE-M42
obs_title            = MUSE map of the central Orion Nebula (M 42)
obs_description      = Integral-field spectroscopic dataset of the central part of the Orion Nebula (M 42), observed with the MUSE instrument at the ESO VLT (reduced the data with the public MUSE pipeline) representing a FITS cube with a spatial size of ~5.9'x4.9' (corresponding to ~0.76 pc x 0.63 pc) and a contiguous wavelength coverage of 4595...9366 Angstrom, spatially sampled at 0.2", with a sampling of 1.25 Angstrom in dispersion direction.
obs_ack              = Based on data obtained from the ESO/VLT
prov_progenitor      = MUSE Consortium
bib_reference        = 2015A&A...582A.114W
bib_reference_url    = http://simbad.u-strasbg.fr/simbad/sim-ref?bibcode=2015A%26A...582A.114W
obs_copyright        = Copyright mention of the original data
obs_copyright_url    = http://muse-vlt.eu/science/m42/
hips_release_date    = 2019-05-21T21:18Z
hips_builder         = Aladin/HipsGen v10.125
hips_order           = 12
hips_pixel_cut       = 0 7760
hips_tile_format     = png fits
hips_cube_depth      = 3818
hips_cube_firstframe  = 1909
hips_frame           = equatorial
dataproduct_type     = cube
t_min                = 56693
t_max                = 56704
em_min               = 4.595e-7
em_max               = 9.366e-7
hips_version         = 1.4
hips_creation_date   = 2015-07-03T12:00Z
hips_creator         = Fernique P. (CDS)
hips_tile_width      = 512
hips_status          = public master clonableOnce
hips_pixel_bitpix    = -32
data_pixel_bitpix    = -32
hips_hierarchy       = mean
hips_initial_ra      = 83.82094
hips_initial_dec     = -5.39542
hips_initial_fov     = 0.09811
hips_pixel_scale     = 2.795E-5
s_pixel_scale        = 5.555E-5
moc_sky_fraction     = 2.980E-7
hips_estsize         = 1131658833636416
data_bunit           = 10**(-20)*erg/s/cm**2/Angstrom
data_cube_crpix3     = 1
data_cube_crval3     = 4595
data_cube_cdelt3     = 1.25
data_cube_bunit3     = Angstrom
client_application   = AladinDesktop
hips_copyright       = CNRS/Unistra
obs_regime           = Optical
hips_order_min       = 0
hipsgen_date         = 2019-05-21T21:18Z
hipsgen_params       = out=/asd-volumes/sc1-asd-volume6/MUSE/MUSE-M42 UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/MUSE/MUSE-M42
hips_service_url_1   = https://alaskybis.cds.unistra.fr/MUSE/MUSE-M42
hips_status_1        = public mirror clonableOnce
client_category      = Cube
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 12
obs_initial_ra       = 83.82094
obs_initial_dec      = -5.39542
obs_initial_fov      = 0.014314526715905856
TIMESTAMP            = 1696351618218

ID                   = CDS/C/MaNGA
creator_did          = ivo://CDS/C/MaNGA
obs_title            = MaNGA
obs_collection       = MaNGA
obs_description      = Unlike previous SDSS surveys which obtained spectra only at the centers of target galaxies, MaNGA (Mapping Nearby Galaxies at APO) enables spectral measurements across the face of each of ~10,000 nearby galaxies thanks to 17 simultaneous "integral field units" (IFUs), each composed of tightly-packed arrays of optical fibers. MaNGA's goal is to understand the "life history" of present day galaxies from imprinted clues of their birth and assembly, through their ongoing growth via star formation and merging, to their death from quenching at late times
hips_initial_fov     = 0.00583
hips_initial_ra      = 183.04456
hips_initial_dec     = +32.79612
hips_pixel_bitpix    = 16
data_pixel_bitpix    = -32
hips_sampling        = bilinear
hips_overlay         = mean
hips_hierarchy       = median
hips_creator         = Buga M. (CDS)
hips_copyright       = CNRS/Unistra
obs_ack              = Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS web site is www.sdss.org. SDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the
prov_progenitor      = SDSS Sloan Digital Sky Survey
bib_reference        = 2015AJ....149...77D
bib_reference_url    = http://adsabs.harvard.edu/abs/2015AJ....149...77D
obs_copyright        = SDSS
obs_copyright_url    = https://www.sdss.org/collaboration/citing-sdss/
t_min                = 56901
t_max                = 57233
obs_regime           = Optical
em_min               = 3.6e-7
em_max               = 1.034e-6
client_category      = Cube
hips_builder         = Aladin/HipsGen v10.125
hips_version         = 1.4
hips_release_date    = 2019-06-03T17:09Z
hips_frame           = equatorial
hips_order           = 12
hips_tile_width      = 64
hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_cut       = 0 3
hips_data_range      = -10 10
hips_pixel_scale     = 2.236E-4
s_pixel_scale        = 1.388E-4
dataproduct_type     = cube
hips_cube_depth      = 4563
hips_cube_firstframe  = 2281
moc_sky_fraction     = 2.104E-5
hips_estsize         = 436770360
hipsgen_date         = 2019-05-28T20:03Z
hipsgen_params       = in=images_MaNGA/ out=MaNGA_DR13/ creator_did=CDS/C/MaNGA hips_order=12 hips_tile_width=64 maxthread=40 fading=false partitioning=false "pixelrange=-10 10" "pixelcut=0 3 log" hips_pixel_bitpix=16 blank=0 "fitskeys=PLATEIFU MANGAID METFILE NEXP EXPTIME MJDMIN MJDMED MJDMAX DATE-OBS" INDEX TILES PNG DETAILS
hips_creation_date   = 2019-05-28T20:03Z
hipsgen_date_1       = 2019-05-29T15:29Z
hipsgen_params_1     = in=images_MaNGA/ out=MaNGA_DR13/ creator_did=CDS/C/MaNGA hips_order=12 hips_tile_width=64 maxthread=40 fading=false partitioning=false "pixelrange=-10 10" "pixelcut=0 3 log" hips_pixel_bitpix=16 blank=0 "fitskeys=PLATEIFU MANGAID METFILE NEXP EXPTIME MJDMIN MJDMED MJDMAX DATE-OBS" INDEX TILES PNG DETAILS
hips_order_min       = 0
hipsgen_date_2       = 2019-06-03T10:21Z
hipsgen_params_2     = out=MaNGA_DR13 UPDATE
hipsgen_date_3       = 2019-06-03T17:09Z
hipsgen_params_3     = out=MaNGA_DR13 UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/MaNGA
hips_progenitor_url  = https://alasky.cds.unistra.fr/MaNGA/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/MaNGA
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 12
obs_initial_ra       = 183.04456
obs_initial_dec      = +32.79612
obs_initial_fov      = 0.014314526715905856
TIMESTAMP            = 1696351629270

ID                   = CDS/C/Mopra/12CO
hips_initial_fov     = 1.09167
hips_initial_ra      = 214.15922
hips_initial_dec     = -61.19972
creator_did          = ivo://CDS/C/Mopra/12CO
hips_pixel_bitpix    = -32
data_pixel_bitpix    = -32
hips_sampling        = bilinear
hips_overlay         = mean
hips_hierarchy       = median
hips_creator         = Buga M. (CDS)
hips_copyright       = CNRS/Unistra
obs_title            = Mopra 12CO
obs_collection       = Mopra 12CO
obs_description      = The Mopra CO survey of the Southern Galactic Plane is being conducted with the Mopra millimetre-wave telescope in Coonabarabran, New South Wales, Australia. The survey is designed to map the distribution and dynamics of the carbon monoxide molecule (CO) along a 120 degree sector of the Galactic Plane, from l=250-370deg. The principal scientific motivations are to study how molecular clouds are formed in space, and to examine the nature of TeV gamma-ray sources observed with H.E.S.S and the forthcoming Cherenkov Telescope Array. Data Release 3 contains observations of fifty square degrees of the Mopra carbon monoxide (CO) survey of the Southern Galactic Plane, covering Galactic longitudes l = 300-350deg and latitudes |b| <= 0.5deg. These data have been taken at 0.6arcminute spatial resolution and 0.1kms-1 spectral resolution, providing an unprecedented view of the molecular clouds and gas of the Southern Galactic Plane in the 109-115 GHz J = 1-0 transitions of 12CO, 13CO, C18O and C17O.
obs_ack              = The Mopra CO data were obtained using the Mopra radio telescope, a part of the Australia Telescope National Facility. The University of New South Wales (UNSW) digital filter bank (the UNSW-MOPS) used for the observations with Mopra was provided with support from the Australian Research Council (ARC), UNSW, Sydney and Monash Universities, as well as the CSIRO.
prov_progenitor      = MOPRA
bib_reference        = 2018PASA...35...29B
bib_reference_url    = https://ui.adsabs.harvard.edu/?#abs/2018PASA...35...29B/abstract
t_min                = 55562
t_max                = 57752
obs_regime           = Infrared
em_min               = 3.455744e+19
em_max               = 3.455744e+19
client_category      = Cube
hips_builder         = Aladin/HipsGen v10.125
hips_version         = 1.4
hips_release_date    = 2019-05-22T07:54Z
hips_frame           = equatorial
hips_order           = 4
hips_order_min       = 0
hips_tile_width      = 512
hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_cut       = -3.161 7.984
hips_data_range      = -15.65 17.53
hips_pixel_scale     = 0.007157
s_pixel_scale        = 0.008333
dataproduct_type     = cube
hips_cube_depth      = 2286
hips_cube_firstframe  = 1143
moc_sky_fraction     = 6.148E-4
hips_estsize         = 37037772
hipsgen_date         = 2019-03-04T17:19Z
hipsgen_params       = in=/data3/buga/Mopra_CO/images_Mopra_CO/12CO/cubes/Vcrop_partages/Vcrop_que_celles_homogenes/ out=hips2 creator_did=CDS/P/Mopra/12CO_2 maxThread=50 "BORDER=0 4 0 4" INDEX TILES PNG DETAILS
hips_creation_date   = 2019-03-04T17:19Z
hipsgen_date_1       = 2019-03-04T17:37Z
hipsgen_params_1     = in=/data3/buga/Mopra_CO/images_Mopra_CO/12CO/cubes/Vcrop_partages/Vcrop_que_celles_homogenes/ out=hips2 creator_did=CDS/P/Mopra/12CO_2 maxThread=50 "BORDER=0 4 0 4" INDEX TILES PNG DETAILS
hipsgen_date_2       = 2019-05-22T07:54Z
hipsgen_params_2     = out=/asd-volumes/sc1-asd-volume6/Mopra/12CO/hips_12CO UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/Mopra/12CO/hips_12CO
hips_progenitor_url  = https://alasky.cds.unistra.fr/Mopra/12CO/hips_12CO/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/Mopra/12CO/hips_12CO
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 9
obs_initial_ra       = 214.15922
obs_initial_dec      = -61.19972
obs_initial_fov      = 0.11451621372724685
TIMESTAMP            = 1696351643690

ID                   = CDS/C/Mopra/13CO
hips_initial_fov     = 1.09167
hips_initial_ra      = 191.92583
hips_initial_dec     = -62.87491
creator_did          = ivo://CDS/C/Mopra/13CO
hips_pixel_bitpix    = -32
data_pixel_bitpix    = -32
hips_sampling        = bilinear
hips_overlay         = mean
hips_hierarchy       = median
hips_creator         = Buga M. (CDS)
hips_copyright       = CNRS/Unistra
obs_title            = Mopra 13CO
obs_collection       = Mopra 13CO
obs_description      = The Mopra CO survey of the Southern Galactic Plane is being conducted with the Mopra millimetre-wave telescope in Coonabarabran, New South Wales, Australia. The survey is designed to map the distribution and dynamics of the carbon monoxide molecule (CO) along a 120 degree sector of the Galactic Plane, from l=250-370deg. The principal scientific motivations are to study how molecular clouds are formed in space, and to examine the nature of TeV gamma-ray sources observed with H.E.S.S and the forthcoming Cherenkov Telescope Array. Data Release 3 contains observations of fifty square degrees of the Mopra carbon monoxide (CO) survey of the Southern Galactic Plane, covering Galactic longitudes l = 300-350deg and latitudes |b| <= 0.5deg. These data have been taken at 0.6arcminute spatial resolution and 0.1kms-1 spectral resolution, providing an unprecedented view of the molecular clouds and gas of the Southern Galactic Plane in the 109-115 GHz J = 1-0 transitions of 12CO, 13CO, C18O and C17O.
obs_ack              = The Mopra CO data were obtained using the Mopra radio telescope, a part of the Australia Telescope National Facility. The University of New South Wales (UNSW) digital filter bank (the UNSW-MOPS) used for the observations with Mopra was provided with support from the Australian Research Council (ARC), UNSW, Sydney and Monash Universities, as well as the CSIRO.
prov_progenitor      = MOPRA
bib_reference        = 2018PASA...35...29B
bib_reference_url    = https://ui.adsabs.harvard.edu/?#abs/2018PASA...35...29B/abstract
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hipsgen_date         = 2019-03-05T14:26Z
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hipsgen_date_2       = 2019-05-22T08:41Z
hipsgen_params_2     = out=/asd-volumes/sc1-asd-volume6/Mopra/13CO/hips_13CO UPDATE
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TIMESTAMP            = 1696351643834

ID                   = CDS/C/Mopra/C17O
hips_initial_fov     = 1.09167
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hips_initial_dec     = -62.15144
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hips_creator         = Buga M. (CDS)
hips_copyright       = CNRS/Unistra
obs_title            = Mopra C17O
obs_collection       = Mopra C17O
obs_description      = The Mopra CO survey of the Southern Galactic Plane is being conducted with the Mopra millimetre-wave telescope in Coonabarabran, New South Wales, Australia. The survey is designed to map the distribution and dynamics of the carbon monoxide molecule (CO) along a 120 degree sector of the Galactic Plane, from l=250-370deg. The principal scientific motivations are to study how molecular clouds are formed in space, and to examine the nature of TeV gamma-ray sources observed with H.E.S.S and the forthcoming Cherenkov Telescope Array. Data Release 3 contains observations of fifty square degrees of the Mopra carbon monoxide (CO) survey of the Southern Galactic Plane, covering Galactic longitudes l = 300-350deg and latitudes |b| <= 0.5deg. These data have been taken at 0.6arcminute spatial resolution and 0.1kms-1 spectral resolution, providing an unprecedented view of the molecular clouds and gas of the Southern Galactic Plane in the 109-115 GHz J = 1-0 transitions of 12CO, 13CO, C18O and C17O.
obs_ack              = The Mopra CO data were obtained using the Mopra radio telescope, a part of the Australia Telescope National Facility. The University of New South Wales (UNSW) digital filter bank (the UNSW-MOPS) used for the observations with Mopra was provided with support from the Australian Research Council (ARC), UNSW, Sydney and Monash Universities, as well as the CSIRO.
prov_progenitor      = MOPRA
bib_reference        = 2018PASA...35...29B
bib_reference_url    = https://ui.adsabs.harvard.edu/?#abs/2018PASA...35...29B/abstract
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hips_cube_depth      = 2228
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hipsgen_date         = 2019-03-06T10:26Z
hipsgen_params       = in=Vcrop/ out=hips_C17O creator_did=CDS/P/Mopra/C17O maxThread=50 "BORDER=4 4 4 4" INDEX TILES PNG DETAILS
hips_creation_date   = 2019-03-06T10:26Z
hipsgen_date_1       = 2019-03-06T10:39Z
hipsgen_params_1     = in=Vcrop/ out=hips_C17O creator_did=CDS/P/Mopra/C17O maxThread=50 "BORDER=4 4 4 4" INDEX TILES PNG DETAILS
hipsgen_date_2       = 2019-05-22T08:44Z
hipsgen_params_2     = out=/asd-volumes/sc1-asd-volume6/Mopra/C17O/hips_C17O UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/Mopra/C17O/hips_C17O
hips_progenitor_url  = https://alasky.cds.unistra.fr/Mopra/C17O/hips_C17O/HpxFinder
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hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 25
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moc_order            = 9
obs_initial_ra       = 207.04685
obs_initial_dec      = -62.15144
obs_initial_fov      = 0.11451621372724685
TIMESTAMP            = 1696351643926

ID                   = CDS/C/Mopra/C18O
hips_initial_fov     = 1.09167
hips_initial_ra      = 204.94326
hips_initial_dec     = -62.35372
creator_did          = ivo://CDS/C/Mopra/C18O
hips_pixel_bitpix    = -32
data_pixel_bitpix    = -32
hips_sampling        = bilinear
hips_overlay         = mean
hips_hierarchy       = median
hips_creator         = Buga M. (CDS)
hips_copyright       = CNRS/Unistra
obs_title            = Mopra C18O
obs_collection       = Mopra C18O
obs_description      = The Mopra CO survey of the Southern Galactic Plane is being conducted with the Mopra millimetre-wave telescope in Coonabarabran, New South Wales, Australia. The survey is designed to map the distribution and dynamics of the carbon monoxide molecule (CO) along a 120 degree sector of the Galactic Plane, from l=250-370deg. The principal scientific motivations are to study how molecular clouds are formed in space, and to examine the nature of TeV gamma-ray sources observed with H.E.S.S and the forthcoming Cherenkov Telescope Array. Data Release 3 contains observations of fifty square degrees of the Mopra carbon monoxide (CO) survey of the Southern Galactic Plane, covering Galactic longitudes l = 300-350deg and latitudes |b| <= 0.5deg. These data have been taken at 0.6arcminute spatial resolution and 0.1kms-1 spectral resolution, providing an unprecedented view of the molecular clouds and gas of the Southern Galactic Plane in the 109-115 GHz J = 1-0 transitions of 12CO, 13CO, C18O and C17O.
obs_ack              = The Mopra CO data were obtained using the Mopra radio telescope, a part of the Australia Telescope National Facility. The University of New South Wales (UNSW) digital filter bank (the UNSW-MOPS) used for the observations with Mopra was provided with support from the Australian Research Council (ARC), UNSW, Sydney and Monash Universities, as well as the CSIRO.
prov_progenitor      = MOPRA
bib_reference        = 2018PASA...35...29B
bib_reference_url    = https://ui.adsabs.harvard.edu/?#abs/2018PASA...35...29B/abstract
t_min                = 55562
t_max                = 57752
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client_category      = Cube
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hips_version         = 1.4
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hips_frame           = equatorial
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hips_order_min       = 0
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hips_data_range      = -9.005 8.005
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dataproduct_type     = cube
hips_cube_depth      = 2177
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moc_sky_fraction     = 3.681E-4
hips_estsize         = 28860489
hipsgen_date         = 2019-03-06T09:27Z
hipsgen_params       = in=/data4/buga/images_Mopra_CO/C18O/Vcrop/images_2177frames/ out=hips_C18O creator_did=CDS/P/Mopra/C18O maxThread=50 "BORDER=4 4 4 4" INDEX TILES PNG DETAILS
hips_creation_date   = 2019-03-06T09:27Z
hipsgen_date_1       = 2019-03-06T09:42Z
hipsgen_params_1     = in=/data4/buga/images_Mopra_CO/C18O/Vcrop/images_2177frames/ out=hips_C18O creator_did=CDS/P/Mopra/C18O maxThread=50 "BORDER=4 4 4 4" INDEX TILES PNG DETAILS
hipsgen_date_2       = 2019-05-22T08:58Z
hipsgen_params_2     = out=/asd-volumes/sc1-asd-volume6/Mopra/C18O/hips_C18O UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/Mopra/C18O/hips_C18O
hips_progenitor_url  = https://alasky.cds.unistra.fr/Mopra/C18O/hips_C18O/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/Mopra/C18O/hips_C18O
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 9
obs_initial_ra       = 204.94326
obs_initial_dec      = -62.35372
obs_initial_fov      = 0.11451621372724685
TIMESTAMP            = 1696351644022

ID                   = CDS/P/3D-Dust-Bayestar19
hips_initial_fov     = 60
hips_initial_ra      = 266.4168333
hips_initial_dec     = 29.0078055
creator_did          = ivo://CDS/P/3D-Dust-Bayestar19
hips_creator         = Boch T. (CDS)
hips_copyright       = CNRS/Universite de Strasbourg
obs_title            = Reddening (E(B-V)) Map (Green et al. 2019)
obs_description      = Bayestar 2019 is a new three-dimensional map of dust reddening, based on Gaia parallaxes and stellar photometry from Pan-STARRS 1 and 2MASS. This map covers the sky north of a declination of -30deg, out to a distance of several kiloparsecs. This new map contains three major improvements over our previous work. First, the inclusion of Gaia parallaxes dramatically improves distance estimates to nearby stars. Second, we incorporate a spatial prior that correlates the dust density across nearby sightlines.  This produces a smoother map, with more isotropic clouds and smaller distance uncertainties, particularly to clouds within the nearest kiloparsec. Third, we infer the dust density with a distance resolution that is four times finer than in our previous work, to accommodate the improvements in signal-to-noise enabled by the other improvements.
prov_progenitor      = Dataverse
prov_progenitor_url  = https://dataverse.harvard.edu/dataset.xhtml?persistentId=doi:10.7910/DVN/2EJ9TX
bib_reference        = 10.1051/0004-6361/201834695
bib_reference_url    = https://doi.org/10.1051/0004-6361/201834695
obs_copyright_url    = http://argonaut.skymaps.info/
hips_builder         = Aladin/HipsGen v10.130
hips_version         = 1.4
hips_release_date    = 2019-09-19T09:46Z
hips_frame           = galactic
hips_order           = 3
hips_order_min       = 0
hips_tile_width      = 128
hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_scale     = 0.05726
dataproduct_type     = cube
hips_cube_depth      = 120
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moc_sky_fraction     = 0.764
hips_estsize         = 8722800
hipsgen_date         = 2019-09-19T09:42Z
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hips_creation_date   = 2019-09-19T09:42Z
hips_pixel_bitpix    = -32
hipsgen_date_1       = 2019-09-19T09:46Z
hipsgen_params_1     = out=hips/cube UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/Bayestar19
hips_service_url_1   = https://alaskybis.cds.unistra.fr/Bayestar19
hips_status_1        = public mirror clonableOnce
client_category      = Cube
moc_type             = smoc
moc_order            = 7
obs_initial_ra       = 266.4168333
obs_initial_dec      = 29.0078055
obs_initial_fov      = 0.4580648549089874
TIMESTAMP            = 1696438160334

ID                   = CDS/P/ACT/DR4/f090
hips_initial_fov     = 360.0
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hips_initial_dec     = -20.00833
creator_did          = ivo://CDS/P/ACT/DR4/f090
hips_pixel_bitpix    = -64
data_pixel_bitpix    = -64
hips_sampling        = bilinear
hips_overlay         = mean
hips_hierarchy       = median
hips_creator         = Buga M. (CDS)
hips_copyright       = CNRS/Unistra
obs_title            = ACT DR4 f090
obs_collection       = ACT DR4 f090
obs_description      = The Atacama Cosmology Telescope (ACT) is a six-meter diameter telescope on Cerro Toco in the Atacama Desert of northern Chile (image above by Jon Ward). It is designed to make high-resolution measurements of the cosmic microwave background (CMB) temperature and polarization anisotropies and detect massive galaxy clusters via the thermal Sunyaev Zel'dovich (tSZ) effect. Reconstruction of the CMB lensing potential will play a key role in the cosmological detection of neutrino mass, and measuring the imprint of primordial gravitational waves in B-mode polarization could provide unique insights into the early universe and quantum nature of gravity. The majority of the DR4 products use data collected from 2013-16. DR4 also includes data collected from 2008-10. The second-generation, polarization-sensitive receiver ACTPol observed between 2013 and 2016. The four-year survey consists of 17,000 square degrees of the sky mapped at 98 and 150 GHz, with the deepest 600 square degrees at a noise < 10 uK-arcmin.
prov_progenitor      = https://lambda.gsfc.nasa.gov/product/act/actpol_prod_table.cfm
bib_reference        = 2020ApJ...903L..13M
bib_reference_url    = https://ui.adsabs.harvard.edu/abs/2020ApJ...903L..13M/abstract
obs_copyright        = LAMBDA HEASARC
obs_copyright_url    = https://lambda.gsfc.nasa.gov/
t_min                = 54466.6
t_max                = 57752.2
obs_regime           = Radio
client_category      = Cube
em_min               = 0.00305910
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hips_builder         = Aladin/HipsGen v11.037
hips_version         = 1.4
hips_release_date    = 2021-03-17T18:04Z
hips_frame           = equatorial
hips_order           = 4
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hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_cut       = -731.9 908.7
hips_data_range      = -2943 3001
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s_pixel_scale        = 0.008333
dataproduct_type     = cube
hips_cube_depth      = 3
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moc_sky_fraction     = 0.4578
hips_estsize         = 17992980
hipsgen_date         = 2021-03-17T17:58Z
hipsgen_params       = in=act_dr4.01_s08s16_AA_f090_night_map.fits out=HipS_ACT/ creator_did=CDS/P/ACT2/DR4/90 verbose=4 BLANK=0
hips_creation_date   = 2021-03-17T17:58Z
hips_service_url     = https://alasky.cds.unistra.fr/ACT/DR4/CDS_P_ACT_DR4_f90
hips_progenitor_url  = https://alasky.cds.unistra.fr/ACT/DR4/CDS_P_ACT_DR4_f90/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/ACT/DR4/CDS_P_ACT_DR4_f90
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 7
obs_initial_ra       = 0.00833
obs_initial_dec      = -20.00833
obs_initial_fov      = 0.4580648549089874
TIMESTAMP            = 1696351649142

ID                   = CDS/P/ACT/DR4/f150
hips_initial_fov     = 360.0
hips_initial_ra      = 0.00833
hips_initial_dec     = -20.00833
creator_did          = ivo://CDS/P/ACT/DR4/f150
hips_pixel_bitpix    = -64
data_pixel_bitpix    = -64
hips_sampling        = bilinear
hips_overlay         = mean
hips_hierarchy       = median
hips_creator         = Buga M. (CDS)
hips_copyright       = CNRS/Unistra
obs_title            = ACT DR4 f150
obs_collection       = ACT DR4 f150
obs_description      = The Atacama Cosmology Telescope (ACT) is a six-meter diameter telescope on Cerro Toco in the Atacama Desert of northern Chile (image above by Jon Ward). It is designed to make high-resolution measurements of the cosmic microwave background (CMB) temperature and polarization anisotropies and detect massive galaxy clusters via the thermal Sunyaev Zel'dovich (tSZ) effect. Reconstruction of the CMB lensing potential will play a key role in the cosmological detection of neutrino mass, and measuring the imprint of primordial gravitational waves in B-mode polarization could provide unique insights into the early universe and quantum nature of gravity. The majority of the DR4 products use data collected from 2013-16. DR4 also includes data collected from 2008-10. The second-generation, polarization-sensitive receiver ACTPol observed between 2013 and 2016. The four-year survey consists of 17,000 square degrees of the sky mapped at 98 and 150 GHz, with the deepest 600 square degrees at a noise < 10 uK-arcmin.
prov_progenitor      = https://lambda.gsfc.nasa.gov/product/act/actpol_prod_table.cfm
bib_reference        = 2020ApJ...903L..13M
bib_reference_url    = https://ui.adsabs.harvard.edu/abs/2020ApJ...903L..13M/abstract
obs_copyright        = LAMBDA HEASARC
obs_copyright_url    = https://lambda.gsfc.nasa.gov/
t_min                = 54466.6
t_max                = 57752.2
obs_regime           = Radio
client_category      = Cube
em_min               = 0.00199861
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hips_builder         = Aladin/HipsGen v11.037
hips_version         = 1.4
hips_release_date    = 2021-03-17T18:10Z
hips_frame           = equatorial
hips_order           = 4
hips_order_min       = 0
hips_tile_width      = 512
hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_cut       = -569.8 701.2
hips_data_range      = -2487 2169
hips_pixel_scale     = 0.007157
s_pixel_scale        = 0.008333
dataproduct_type     = cube
hips_cube_depth      = 3
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data_cube_cdelt3     = 1.0
data_cube_bunit3     = null
moc_sky_fraction     = 0.476
hips_estsize         = 17992980
hipsgen_date         = 2021-03-17T18:07Z
hipsgen_params       = in=act_dr4.01_s08s16_AA_f150_night_map.fits out=HiPS_ACT_150/ creator_did=CDS/P/ACT2/DR4/150 verbose=4 BLANK=0
hips_creation_date   = 2021-03-17T18:07Z
hips_service_url     = https://alasky.cds.unistra.fr/ACT/DR4/CDS_P_ACT_DR4_f150
hips_progenitor_url  = https://alasky.cds.unistra.fr/ACT/DR4/CDS_P_ACT_DR4_f150/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/ACT/DR4/CDS_P_ACT_DR4_f150
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 7
obs_initial_ra       = 0.00833
obs_initial_dec      = -20.00833
obs_initial_fov      = 0.4580648549089874
TIMESTAMP            = 1696351649282

ID                   = CDS/P/ACT/DR5/f150
hips_initial_fov     = 360.0
hips_initial_ra      = 0.00833
hips_initial_dec     = -20.00833
creator_did          = ivo://CDS/P/ACT/DR5/f150
hips_pixel_bitpix    = -32
data_pixel_bitpix    = -32
hips_sampling        = bilinear
hips_overlay         = mean
hips_hierarchy       = median
hips_creator         = Buga M. (CDS)
hips_copyright       = CNRS/Unistra
obs_title            = ACT DR4 f150
obs_collection       = ACT DR4 f150
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hips_service_url_1   = https://alaskybis.cds.unistra.fr/ACT/DR5/CDS_P_ACT_Planck_DR5_f220
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 7
obs_initial_ra       = 0.00833
obs_initial_dec      = -20.00833
obs_initial_fov      = 0.4580648549089874
TIMESTAMP            = 1696351649558

ID                   = CDS/P/ACT_Planck/DR5/f90
hips_initial_fov     = 360.0
hips_initial_ra      = 0.00833
hips_initial_dec     = -20.00833
creator_did          = ivo://CDS/P/ACT_Planck/DR5/f90
hips_pixel_bitpix    = -32
data_pixel_bitpix    = -32
hips_sampling        = bilinear
hips_overlay         = mean
hips_hierarchy       = median
hips_creator         = Buga M. (CDS)
hips_copyright       = CNRS/Unistra
obs_title            = ACT_Planck DR5 f090
obs_collection       = ACT_Planck DR5 f090
obs_description      = The Atacama Cosmology Telescope (ACT) is a six-meter diameter telescope on Cerro Toco in the Atacama Desert of northern Chile (image above by Jon Ward). It is designed to make high-resolution measurements of the cosmic microwave background (CMB) temperature and polarization anisotropies and detect massive galaxy clusters via the thermal Sunyaev Zel'dovich (tSZ) effect. Reconstruction of the CMB lensing potential will play a key role in the cosmological detection of neutrino mass, and measuring the imprint of primordial gravitational waves in B-mode polarization could provide unique insights into the early universe and quantum nature of gravity. The  DR4  products  use  data  collected  from  2013-16 but also includes data collected from 2008-10. DR5 adds ACT data acquired in 2017-18 in frequency bands centered at 98, 150 and 220 GHz.
prov_progenitor      = https://lambda.gsfc.nasa.gov/product/act/actpol_prod_table.cfm
bib_reference        = 2020ApJ...903L..13M
bib_reference_url    = https://ui.adsabs.harvard.edu/abs/2020ApJ...903L..13M/abstract
obs_copyright        = LAMBDA HEASARC
obs_copyright_url    = https://lambda.gsfc.nasa.gov/
t_min                = 54466.6
t_max                = 58482.6
obs_regime           = Radio
client_category      = Cube
em_min               = 0.00305910
em_max               = 0.00305910
hips_builder         = Aladin/HipsGen v11.056
hips_version         = 1.4
hips_release_date    = 2021-05-21T10:03Z
hips_frame           = equatorial
hips_order           = 4
hips_order_min       = 0
hips_tile_width      = 512
hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_cut       = -278.8 340.1
hips_data_range      = -1043 1074
hips_pixel_scale     = 0.007157
s_pixel_scale        = 0.008333
dataproduct_type     = cube
hips_cube_depth      = 3
hips_cube_firstframe  = 1
data_cube_crpix3     = 1.0
data_cube_crval3     = 1.0
data_cube_cdelt3     = 1.0
data_cube_bunit3     = null
moc_sky_fraction     = 0.4749
hips_estsize         = 9116127
hipsgen_date         = 2021-05-21T10:03Z
hipsgen_params       = in=act_planck_dr5.01_s08s18_AA_f090_daynight_map.fits out=ACT_PLANCK_f090 creator_did=CDS/P/ACT_Planck/DR5/f90 verbose=4 BLANK=0
hips_creation_date   = 2021-05-21T10:03Z
hips_service_url     = https://alasky.cds.unistra.fr/ACT/DR5/CDS_P_ACT_Planck_DR5_f90
hips_progenitor_url  = https://alasky.cds.unistra.fr/ACT/DR5/CDS_P_ACT_Planck_DR5_f90/HpxFinder
hips_service_url_1   = https://alaskybis.cds.unistra.fr/ACT/DR5/CDS_P_ACT_Planck_DR5_f90
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 7
obs_initial_ra       = 0.00833
obs_initial_dec      = -20.00833
obs_initial_fov      = 0.4580648549089874
TIMESTAMP            = 1696351649782