Comparison of the Newtonian mass-follows-light models (thick solid lines, shifted for the sake of visibility) with the predictions of various SPS models (thin solid lines). For one galaxy for which the name was given with “W” in an exponent (NGC 2768), the comparison is made for its whole radial extent. For NGC 4365 and NGC 4486, the inner parts extend out to 1R_e and 0.35R_e, respectively; for the remaining seven objects, this plot shows the comparison for their inner parts, interior to ~ 3R_e. Open circles and asterisks denote M_dyn/L_B (Eq. (17)) and M_stars/L_B (dynamically measured by Cappellari et al. 2013b), respectively (see text for details). The names of the slow (fast) rotators are plotted using Roman characters (italic).