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