Similar to Fig. 12. Here we compare to the study by Whitaker et al. (2014) (solid lines), who also report a steepening towards low stellar masses. Their SFRs are seen to be lower, but adding 0.45 to their fits, we obtain a better fit to our data (dash-dotted curves). We do not see any evidence for shallower redshift evolution at low masses as they report. The dashed vertical line marks the division between their individual object (above 10¹⁰) and stacked object (below 10¹⁰) fits. Dotted curves are extrapolations of their fits where they had no data.