Top panels: dust luminosity (L_d, top left), dust mass (M_d, top right), SFR (bottom left), and stellar mass (M_*, bottom right) obtained with CIGALE (Noll et al. 2009; Boquien et al. 2019) from the sample defined in Sect. 2 using the full photometric coverage (ordinate) or removing PACS data (abscissa). The blue dashed line shows a linear relation between the two quantities and the black cross in the bottom right corner shows the average errors in the fits. Bottom panels: histograms of the same quantities.