hips_initial_fov     = 12.58167
hips_initial_ra      = 13.16112
hips_initial_dec     = -72.80113
creator_did          = ivo://CDS/P/Quest-for-the-Missing-Dust/SPIRE250
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 SPIRE250
obs_collection       = Quest-for-the-Missing-Dust SPIRE250
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               = 0.00025
em_max               = 0.00025
client_category      = Image/Infrared/Quest-for-the-Missing-Dust
hips_builder         = Aladin/HipsGen v11.902
hips_version         = 1.4
hips_release_date    = 2022-07-06T10:11Z
hips_frame           = equatorial
hips_order           = 7
hips_order_min       = 0
hips_tile_width      = 512
#hips_service_url    = ex: http://yourHipsServer/Quest_for_the_Missing_Dust SPIRE250
hips_status          = public master clonableOnce
hips_tile_format     = png fits
hips_pixel_cut       = 0 110
hips_data_range      = -200.2 606.1
hips_pixel_scale     = 8.946E-4
s_pixel_scale        = 0.001667
dataproduct_type     = image
moc_sky_fraction     = 0.01162
hips_estsize         = 3362602
hipsgen_date         = 2022-07-06T10:10Z
hipsgen_params       = in=SPIRE_250/ out=HiPS_SPIRE_250/ creator_did=CDS/C/Quest_for_the_Missing_Dust/SPIRE250 "hips_pixel_cut=0 110 sqrt"
hips_creation_date   = 2022-07-06T10:10Z