HIGHLIGHTS
SUMMARY
As gas and dust are well mixed (e_g, Bohlin et_al 1978; Boulanger et_al 1996), an efficient method to infer Mgas indi? Similarly, single band measurements of the dust emission flux on the RayleighJeans side of the SED have also been calibrated against CO observations and under a series of assumptions (e_g, dust temperature, αCO conversion factor) can be used to infer gas mass estimates (e_g, Groves et_al 2015; Scoville et_al 2016, 2017a; Schinnerer et_al 2016; Liu et_al 2019b). If instead the dust opacity of a galaxy extends to λ > 100 µm, its Mdust based on . . .
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