HIGHLIGHTS
SUMMARY
To perform this analysis, the authors selected three types of dust emission available in CIGALE: (i) a mid-IR power law and a general modified blackbody (Casey 2012): PL+G_MBB, (ii) a mid-IR power law and an optically thin modified blackbody (Casey 2012): PL+OT_MBB, and_(iii) the models from Draine et_al: DL2014. The authors only show the results of this test assuming PL+OT_MBB, but the authors checked that the results were the same regardless of the assumed dust emission option. The authors only make use of DL2014 and PL+OT_MBB dust . . .
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