hips_initial_fov     = 80
hips_initial_ra      = 291.88185
hips_initial_dec     = 21.43516
creator_did          = ivo://CDS/P/PanSTARRS/DR1/y
hips_pixel_bitpix    = 16
data_pixel_bitpix    = 16
hips_sampling        = bilinear
hips_overlay         = mean
hips_hierarchy       = mean
hips_creator         = Boch T. (CDS)
hips_copyright       = CNRS/Universite de Strasbourg
hips_license         = ODbL-1.0
obs_title            = PanSTARRS DR1 y
obs_collection       = PanSTARRS DR1 y
obs_description      = Pan-STARRS is a system for wide-field astronomical imaging developed and operated by the Institute for Astronomy at the University of Hawaii. Pan-STARRS1 (PS1) is the first part of Pan-STARRS to be completed and is the basis for Data Release 1 (DR1).  The PS1 survey used a 1.8 meter telescope and its 1.4 Gigapixel camera to image the sky in five broadband  filters (g, r, i, z, y). The PS1 Science Consortium funded the operation of the Pan-STARRS1 telescope, situated at Haleakala Observatories near the summit of Haleakala in Hawaii, for the purposes of astronomical research. The PS1 consortium is made up of astronomers and engineers from 14 institutions from six countries.\nPan-STARRS1 has carried out a set of distinct synoptic imaging sky surveys including the 3pi Steradian Survey and the Medium Deep Survey in 5 bands (grizy). The mean 5sigma point source limiting sensitivities in the stacked 3pi Steradian Survey in grizy are (23.3, 23.2, 23.1, 22.3, 21.4) respectively. The upper bound on the systematic uncertainty in the photometric calibration across the sky is 7-12 millimag depending on the bandpass. The systematic uncertainty of the astrometric calibration using the Gaia frame comes from a comparison of the results with Gaia: the standard deviation of the mean and median residuals (Delta ra, Delta dec ) are (2.3, 1.7) milliarcsec, and (3.1, 4.8) milliarcsec respectively.
obs_ack              = Images data retrieved from the Mikulski Archive for Space Telescopes (MAST) at STScI. Thanks to Clara Brasseur for her help.
prov_progenitor      = MAST/STScI
bib_reference        = 2016arXiv161205560C
bib_reference_url    = https://ui.adsabs.harvard.edu/?#abs/2016arXiv161205560C
obs_copyright        = PS1 Science Consortium
obs_copyright_url    = http://panstarrs.stsci.edu/
t_min                = 55076.5476324608
t_max                = 56957.199631561
obs_regime           = Optical
# PanSTARRS y-filter is described at http://svo2.cab.inta-csic.es/svo/theory/fps/index.php?id=PAN-STARRS/PS1.y&mode=browse&gname=PAN-STARRS&gname2=PS1#filter
em_min               = 8.970e-7
em_max               = 11.100e-7
client_category      = Image/Optical/PanSTARRS
hips_builder         = Aladin/HipsGen v10.130
hips_version         = 1.4
hips_release_date    = 2019-07-04T15:14Z
hips_frame           = equatorial
hips_order           = 11
hips_tile_width      = 512
#hips_service_url    = ex: http://yourHipsServer/PanSTARRS DR1 y
hips_status          = public master clonableOnce
hips_tile_format     = fits jpeg png
hips_data_range      = -2.323 7.915
# JPEG/PNG tiles are generated on the fly
hips_pixel_cut       = -0.2 8
hips_pixel_scale     = 5.591E-5
s_pixel_scale        = 6.944E-5
dataproduct_type     = image
moc_sky_fraction     = 0.7599
hips_estsize         = 27523364430
hipsgen_date         = 2018-11-12T17:48Z
hipsgen_params       = tiles
hips_creation_date   = 2018-11-12T17:48Z
hips_order_min       = 0
hipsgen_date_1       = 2019-05-20T09:35Z
hipsgen_params_1     = out=/asd-volumes/sc1-asd-volume7/Pan-STARRS/DR1/y UPDATE
hipsgen_date_2       = 2019-07-04T15:14Z
hipsgen_params_2     = out=/volume7/CDS_P_PanSTARRS_DR1_y UPDATE
hipsgen_date_3       = 2019-07-04T15:14Z
hipsgen_params_3     = out=/volume7/CDS_P_PanSTARRS_DR1_y UPDATE