Distributions of the specific star formation rate (SSFR) for early and late-type galaxies, with panels as in Fig. 2. All distributions have been normalised to have the same area. Below each panel we show the residuals between the CG’s and the other distributions. The binsize is 0.37. KS tests confirm that there is no pair of them drawn from the same underlying distribution. Colours and line types as in Fig. 1.