Comparison between the CIGALE derived properties (this work), M_star (top-left panel), M_dust (top-right panel), the SFR (bottom-left panel), and T_dust (bottom-right panel) and the corresponding properties presented in U et al. (2012). Pink octagons indicate sources with strong AGN (frac_AGN >  0.2). Wherever available, values come with their uncertainties. The grey solid line corresponds to the one-to-one relation. Extreme outliers are indicated with their IRAS names. In the bottom-right panel, green diamonds correspond to the comparison with the dust temperatures derived in Casey (2012), while blue boxes correspond to the comparison with the ones derived in Herrero-Illana et al. (2019). In this panel, sources with strong AGN are indicated by a pink edge-colour.