Best-fit double Schechter function parameters of the GSMFs shown in Fig. 7, using the same colour-coding by M_halo. Panel a is in the centre, while panels b and c are on the left and right, respectively. For clarity, the vertical error bars corresponding to the passive galaxies in the left-hand panel and the centrals in the right-hand panel have been slightly offset to the right. Corresponding corner plots illustrating the correlations among fitted parameters are provided in Figs. A.6–A.8.