hips_initial_fov     = 2.67822
hips_initial_ra      = 23.46262
hips_initial_dec     = +30.65946
creator_did          = ivo://CDS/P/Quest-for-the-Missing-Dust/PACS100
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            = Quest-for-the-Missing-Dust PACS100
obs_collection       = Quest-for-the-Missing-Dust PACS100
obs_description      = Because the galaxies of the Local Group have such large angular sizes, much of their diffuse, large-angular-scale emission is filtered out by the Herschel data reduction process. In this work, we restore this previously missed dust in Herschel observations of the Large Magellanic Cloud, Small Magellanic Cloud, M31, and M33. We do this by combining Herschel data (including new reductions for the Magellanic Clouds), in Fourier space, with lower-resolution data from all-sky surveys (Planck, IRAS, and COBE) that did not miss the extended emission. For each galaxy, we provide this new Herschel data for 5 Hershcel bands: the PACS 100 and 160 micrometer bands, and the SPIRE 250, 350, and 500 micrometer bands. This data is provided in FITS format, with one FITS file for each band for each galaxy. Each of these files contains 4 extensions. Extension 1 (IMAGE) provides the standard feathered map. Extension 2 (UNC) provides the uncertainty map. Extension 3 (MASK) provides a binary mask map indicating the portion of the data where reliable, fully-feathered high-resolution coverage is available. Extension 4 provides the foreground-subtracted version of the feathered map (FGND_SUB), the header of which also describes the uncertainty on that subtraction.
obs_ack              = C.J.R.C. and J.R.-D. acknowledge financial support from the National Aeronautics and Space Administration (NASA) Astrophysics Data Analysis Program (ADAP) grant 80NSSC18K0944.
prov_progenitor      = The data can be found as an on line material provided by the authors
bib_reference        = 2021ApJ...921...35C
bib_reference_url    = https://iopscience.iop.org/article/10.3847/1538-4357/ac16d4
#obs_copyright       = Copyright mention of the original data
#obs_copyright_url   = URL to copyright page of the original data
t_min                = 54965.5878819 
t_max                = 56411.5878819 
obs_regime           = Infrared
em_min               = 1e-4
em_max               = 1e-4
client_category      = Image/Infrared/Quest-for-the-Missing-Dust
hips_builder         = Aladin/HipsGen v11.902
hips_version         = 1.4
hips_release_date    = 2022-07-06T10:07Z
hips_frame           = equatorial
hips_order           = 8
hips_order_min       = 0
hips_tile_width      = 512
#hips_service_url    = ex: http://yourHipsServer/Quest_for_the_Missing_Dust PACS100
hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_cut       = -7 280
hips_data_range      = -1295 3806
hips_pixel_scale     = 4.473E-4
s_pixel_scale        = 8.888E-4
dataproduct_type     = image
moc_sky_fraction     = 0.01018
hips_estsize         = 11786756
hipsgen_date         = 2022-07-06T10:07Z
hipsgen_params       = in=PACS_100/ out=HiPS_PACS_100/ creator_did=CDS/C/Quest_for_the_Missing_Dust/PACS100 "hips_pixel_cut=-7 280 sqrt"
hips_creation_date   = 2022-07-06T10:07Z