Distributions of the SSFR of late-type galaxies for log (M_∗/M_⊙) ≥ 10.5 (left panels) and for log (M_∗/M_⊙) < 10.5 (right panels). All distributions have been normalised to have the same area. Below each panel, we show the residuals between the CGs 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. However, the distributions between low and high mass LG samples in panels a) and c) are the same above 50%. Colours and line types as in Fig. 1.