Median SFR (first row), stellar mass (second row), and sSFR (third row) surface densities as a function of distance from the centre (in R/R_e) 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. Different colours mark different bins of distance from the MS, as defined in Fig. 4. In the second row, the average Sérsic indices of galaxies in the six bins are written at the top of the panel, with colours corresponding to the bins. We observe that the trend of decreasing sSFR surface density in the central region of galaxies with increasing distance below the MS is also visible when considering the distance from the centre normalised by the mass-weighted effective radii.