The distribution of satellite galaxies in the sSFR–Σ_*,1kpc plane in four panels representing different environments in two mass bins (C and D). This is the same as Fig. 8 but using the raw unweighted and unsmoothed points. ‘Near’ and ‘Far’ refer to log D less than or greater than −0.6 (or R_proj ∼ 0.25R_vir). ‘Low M_h’ and ‘High M_h’ refer to haloes less massive than or more massive than 10^13.5 M_⊙. Satellites in the GV as defined in Fig. 2 lie roughly between the two horizontal lines. For reference, the vertical line marks the median Σ_*,1kpc of the field GV. The sample size of each panel is indicated in the bottom corner.