Analogues of Figs. 3 (top panel) and 4 (bottom panel) considering only galaxies in systems having a halo mass in the range 13.5 < log₁₀[M_halo/M_⊙] < 14.2, typically corresponding to the cluster s regime. The size of bins increased in comparison with the original Figs due to a low number of statistics. The dependencies were calculated for 46 clusters with 2721 satellites in total.