Dependence of the dynamical mass M_dyn to stellar mass M_∗ ratio on central velocity dispersion σ₀ using the Sersic fit parameters. The alternative candidates are indicated by black stars. The galaxies belonging to the Ta10 sample are represented using filled green triangles and the Tr09 sample is marked by filled cyan diamonds. B19 is indicated by a filled grey square. The magenta dashed line marks the limiting scaling central velocity dispersion for our sample selection. The area below the black dashed line is considered to be unphysical, because M_∗ would exceed M_dyn.