ID                   = CDS/P/Fermi/4
hips_doi             = 10.26093/cds/aladin/1r4n-6sg
creator_did          = ivo://CDS/P/Fermi/4
obs_collection       = Fermi4 1-3GeV
obs_title            = Fermi 1-3GeV HEALPix survey.
obs_description      = Launched on June 11, 2008, the Fermi Gamma-ray Space Telescope observes the cosmos using the highest-energy form of light. This survey sums all data observed by the Fermi mission up to week 396. This version of the Fermi survey are intensity maps where the summed counts maps are divided by the exposure for each pixel. We anticipate using the HEASARC's Hera capabilities to update this survey on a roughly quarterly basis. Data is broken into 5 energy bands : 30-100 MeV Band 1, 100-300 MeV Band 2, 300-1000 MeV Band 3, 1-3 GeV Band 4 , 3-300 GeV Band 5. The SkyView data are based upon a Cartesian projection of the counts divided by the exposure maps. In the Cartesian projection pixels near the pole have a much smaller area than pixels on the equator, so these pixels have smaller integrated flux. When creating large scale images in other projections users may wish to make sure to compensate for this effect the flux conserving clip-resampling option.
obs_copyright        = Distributed by SkyView/HEASARC - HEALPixed by CDS
client_category      = Image/Gamma-ray
client_sort_key      = 00-01-03
hips_creation_date   = 2013-06-28T08:28Z
hips_release_date    = 2019-05-05T06:05Z
hips_builder         = Aladin/HipsGen v10.123
hips_creator         = Boch T. (CDS)
hips_version         = 1.4
hips_order           = 3
hips_frame           = equatorial
hips_tile_format     = jpeg fits
dataproduct_type     = image
moc_access_url       = http://alasky.u-strasbg.fr/Fermi/1-3GeV/Moc.fits
hips_status          = public master clonableOnce
hips_copyright       = CNRS/Unistra
obs_ack              = This research has made use of data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory's High Energy Astrophysics Division
prov_progenitor      = NASA/HEASARC
bib_reference        = 2009ApJ...697.1071A
bib_reference_url    = https://ui.adsabs.harvard.edu/?#abs/2009ApJ...697.1071A
obs_copyright_url    = http://skyview.gsfc.nasa.gov/current/cgi/survey.pl
t_min                = 54628
t_max                = 56291
obs_regime           = Gamma-ray
em_min               = 4.1328e-16
em_max               = 1.2398e-15
hips_tile_width      = 512
hips_pixel_scale     = 0.01431
hips_initial_fov     = 150.0
hips_initial_ra      = 266.4168166
hips_initial_dec     = -29.0078249
hips_order_min       = 0
hips_pixel_bitpix    = -32
moc_sky_fraction     = 1
hips_estsize         = 1112337
hipsgen_date         = 2019-05-05T06:05Z
hipsgen_params       = out=/asd-volumes/sc1-asd-volume10/Fermi/1-3GeV UPDATE
hips_service_url     = https://alasky.cds.unistra.fr/Fermi/1-3GeV
hips_service_url_1   = https://alaskybis.cds.unistra.fr/Fermi/1-3GeV
hips_status_1        = public mirror clonableOnce
moc_type             = stmoc
moc_time_order       = 25
moc_time_range       = 1
moc_order            = 3
obs_initial_ra       = 266.4168166
obs_initial_dec      = -29.0078249
obs_initial_fov      = 7.3290376785437985
TIMESTAMP            = 1721288415310