2 LocalGroup ivo://irsa.ipac/Herschel/Images/LocalGroup NASA/IPAC Infrared Science Archive Clark et al. IRSA Support Team

irsasupport@ipac.caltech.edu 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. This work restores this previously missed dust in Herschel observations of the Large Magellanic Cloud, Small Magellanic Cloud, M31, and M33 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. https://irsa.ipac.caltech.edu/data/Herschel/LocalGroup/overview.html Archive Research 2 https://irsa.ipac.caltech.edu/SIA?COLLECTION=herschel_localgroup& Pointed 2.0 2.0 26.9 26.9 15133 3664143360 20 10.684793 41.269065 Infrared Millimeter