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
obs_regime = Infrared
em_min = 3.368437e+19
em_max = 3.368437e+19
client_category = Cube
hips_builder = Aladin/HipsGen v10.125
hips_version = 1.4
hips_release_date = 2019-05-22T08:58Z
hips_frame = equatorial
hips_order = 4
hips_order_min = 0
hips_tile_width = 512
hips_status = public master clonableOnce
hips_tile_format = png fits
hips_pixel_cut = -2.415 3.165
hips_data_range = -9.005 8.005
hips_pixel_scale = 0.007157
s_pixel_scale = 0.008333
dataproduct_type = cube
hips_cube_depth = 2177
hips_cube_firstframe = 1088
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