From top to bottom: stacked maps of SFR, stellar mass, sSFR, uncorrected L_UV, dust corrected L_UV, and E(B − V) of galaxies with axis ratio q >  0.5, 0.05″ <  re <  0.8″, 0.7 <  z <  1.0, and 10.0 < Log(M_⋆/M_⊙) < 10.5. The six columns are the six bins of distance from the MS. On the right side of the figure, the median radial profiles of galaxies in each bin are shown using the same colour code as Figs. 4 and 5. The trends shown in this figure hint towards inside-out quenching below the MS and enhanced SF activity above the MS.