Fig. 5.

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RsSFR/Rnorm as a function of stellar mass. The two shaded grey regions show limits on the measurements of RsSFR/Rnorm. We have excluded any galaxies where the sSFR profile spans fewer than three data points, so the dashed black line has RsSFR = 6.545″. In principle, any sSFR profile with more than three data points could still have a truncation at the first data point, so the dash-dotted line has RsSFR = 2.805″. In both cases, Rnorm is determined from the size mass relation in Fig. 4 at a distance of 16.5 Mpc.
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