Stellar-to-total dynamical mass relation for our CALIFA galaxies in terms of stellar population properties measured at different annuli. Each column corresponds to a different annulus with increasing galactocentric distance from left to right (see text). Galaxies are shown as circles color-coded by median ages (upper rows) and metallicities (bottom rows), measured within their corresponding annuli. Partial correlation-coefficient strengths are shown in the bottom right corner (solid black or green lines) between the stellar population parameters and M_★ (vertical) and M_tot (horizontal). Black (green) lines correspond to statistically (not) significant partial correlation coefficients. Solid gray lines have a length corresponding to a correlation coefficient of 0.6 for reference. The direction of maximal increase of the stellar population parameters (see main text) is indicated as a solid blue line when both partial correlation coefficients are significant, while it is red if at least one of the two is not significant.