Fits similar to those shown in Fig. 2 but allowing the inner slope of the stellar mass profile to vary (dashed green lines) and the inner and outer slopes to vary independently (orange lines). The density used for the fitting was assumed to be ρ_abc in Eq. (15) with different bonds between a, b, and c for the green and orange lines. See the main text and the caption of Fig. 2 for further details.