sSFR (logarithm) plotted against NUV-W1 (AB) color. The gray region and contours correspond to the GSWLC (Salim et al. 2016), with the GSWLC medians over the same range as for MAGMA given by a black dashed line. MAGMA medians are shown by a thick gray line with black borders as in previous figures. As described in the text, the SFRs and stellar masses from the GSWLC are compatible with those for MAGMA.