Comparison of the SED fitting results for the 53 FIR-detected galaxies using their full photometry from UV to FIR with respect to a fitting using only the optical ugrizy-bands. From top to bottom, the panels show the difference in SFR, L_IR, and A_V estimated from the two fits, as a function of the stellar mass of the galaxies. The red dashed line marks the mean and scatter along different stellar mass bins. The histograms beside each panel give the overall distribution of each quantity, with their mean and scatter indicated at the top of each histogram. When comparing the stellar mass estimates of the two fits, we found that there is only a minor difference, as expected, with a mean difference of −0.09 ± 0.13 dex.