Fig. 12.

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SFR vs. M plane of COSMOS2015 galaxies (colored circles) as it results from the SED fitting performed by the Prospector code (Leja et al. 2021). Only the objects cross-correlated to COSMOS2020 (0.6″ searching radius) are shown, both those having a MIPS 24 μm counterpart (in the upper panel) and objects without FIR detection (lower panel). Each data point is color-coded according to the difference in SFR between Prospector and the SOM estimator. A dashed line at constant sSFR = 10−11 yr−1 is plotted in each panel to guide the eye.
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