Distributions of SFR for the MAGMA sample are shown as red-shaded regions in bins of M_star; the SDSS10 sample in yellow-shaded regions and the fit to the SFMS (shown as a solid gray curve) reported by Hunt et al. (2019) are also shown. The close agreement of MAGMA with SDSS and the SFMS, except possibly for the lowest M_star bin, suggests that starbursts do not dominate the galaxy population represented.