As in Fig. 2, but using stellar mass and SFR values from CIGALE. We do not show bins with fewer than ten galaxies. The presence or absence of certain bins with respect to Fig. 2 is driven by the differences in stellar mass and SFR between LEPHARE and CIGALE. All lines are defined similar to Fig. 2. This confirms that our results are unaffected by the SED fitting tool or assumptions.