Using a new deblended Herschel catalog, the authors show that UV-to-mid-infrared SED fits recover the star-forming main sequence but under-predict far-infrared luminosity in low-mass galaxies when fixed dust templates are used.
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3D-Herschel: Constraining Dust Emission with Panchromatic Modeling of 3D-HST Galaxies
Using a new deblended Herschel catalog, the authors show that UV-to-mid-infrared SED fits recover the star-forming main sequence but under-predict far-infrared luminosity in low-mass galaxies when fixed dust templates are used.