Fig. 5.
Total and far IR luminosities versus the CO luminosity. Solid lines show linear fits to our (U)LIRG sample, yielding 
and 
. Dashed lines are fits including the comparison samples, which also show linear slopes when using LTIR (0.97 ± 0.06) or LFIR (1.05 ± 0.06). To avoid AGN contamination, only those (U)LIRGs with an AGN bolometric fraction <0.20 (obtained from Díaz-Santos et al. 2017) were plotted and fitted.
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