Fig. 20.
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Relation between the molecular gas mass derived using the total dust mass and assuming a gas-to-dust ratio of G/D = 80 and the molecular gas mass derived using CO observations for galaxies with ALMA (empty symbols) and CARMA (filled symbols) data. The different galaxies are indicated by different symbols. The dotted line shows the expected relation for a gas-to-dust ratio G/D = 80.
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