I_e-R_e plane and 3DKS of SSP galaxy models with with the MRR of Eq. (15), i.e., the Cosmic Galaxy Shepherd. The specific intensity I_e in use is for the B-passband. Left panel: the I_e-R_e plane for the case with the constant ratio m = M_DM/M_S = 25, and the SFH described in the text. The black squares are the GLO-models while the dark olive green squares are the GAL-models. The small dots are the data of Burstein et al. (1997) and Illustris using the same color code of Fig. 1. In the same panel we also show GLO-models in which the ratio m = M_DM/M_S = 5. See the text for more details. Right panel: the corresponding 3DKS. Symbols and color codes are the same as in the left panel. The GLO-models for m = M_DM/M_S = 5 are not displayed because the difference with respect to those with m = M_DM/M_s = 25 is very small.