Upper panel: location of galaxies from the IR-sample with varying B/T on the SFR−M_∗ plane, using the stellar mass and star formation rate (IR+UV) of the whole galaxy. On all plots, the vertical dotted line shows our adopted stellar mass cut, the horizontal dotted line is the 90% completeness in SFR, and the solid black line shows the locus of the z = 1 main sequence as observed through stacking in S15, while the solid gray line shows the extrapolation of the low-mass trend assuming a slope of unity, as observed at lower stellar masses (see Fig. 1). In each column, galaxies of different B/T are plotted. In the rightmost panel, we show all galaxies regardless of their B/T. The solid blue lines show the running median of the sample. Lower panel: same as upper panel, but on the SFR−M_disk plane.