Fig. 5.
FIR SFR against M(H2) for our CLoGS dominant galaxies (black circles or arrows) and non-CLoGS galaxies observed in our deep observations (cyan squares or arrows). The dashed line indicates the molecular gas mass to SFR relation of Gao & Solomon (2004), equivalent to typical depletion timescales ∼1 Gyr, and the shaded region a range of a factor of 5 about the relation.
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