Fig. 3
Comparison of parameters estimated by SED fitting for the catalogue of artificial galaxies. The initial values of the parameters are on the x-axis and the values estimated after SED fitting on the y-axis. The galaxies without IR data are plotted as black dots, the galaxies with only a MIPS detection as green filled circles, and those also detected with PACS as large red filled circles. The regression lines for each subsample are also plotted as solid lines and the 1:1 relation as a dashed line. From the left top to the right bottom, the parameters considered are the SFR, Mstar, LIR, t1, log (t2), log (fySP), AFUV, Eb, and δ.
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