Median SFR (first row), stellar mass (second row), and sSFR (third row) surface densities as a function of distance from the centre (in kiloparsecs) for galaxies in the redshift range [0.2:0.7]. The three columns indicate galaxies with different stellar masses: 9.5 < Log(M_⋆/M_⊙) < 10.0 in the first, 10.0 < Log(M_⋆/M_⊙) < 10.5 in the second, and 10.5 < Log(M_⋆/M_⊙) < 11.0 in the third column, respectively. The thickness of the profiles in a given bin of distance from the centre is given by ± the standard deviation of the values in that bin, dived by the square root of the number of points in that bin. Different colours mark different bins of distance from the MS, as defined in Fig. 4. The sSFR profiles of galaxies below the MS are characterised by a central suppression that becomes more significant with increasing distance from the MS.