The infrared emission of galaxies via machine learning techniques Ghent University
For a typical galaxy like the Milky Way, roughly one third of all starlight is re-processed through
cosmic dust. The only way to directly observe and measure the interstellar dust content of galaxies
uses observations at far-infrared and sub-millimeter (FIR/submm) wavelengths. Unfortunately,
there are now no FIR/submm missions operational or approved. In principle, however, it should be
possible to ...