Fig. 13.
SED-derived SFR vs. Mstar in logarithmic space superimposed on the GSWLC sample shown in gray-scale from Salim et al. (2016, see text for details). As in previous figures, filled symbols correspond to high specific SFR (Log(sSFR/yr−1) > −10.6), and open ones to low specific SFR (Log(sSFR/yr−1) ≤ −10.6). The (gray) dashed line corresponds to the SFMS relation found by Hunt et al. (2016) for nearby galaxies.
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