Evolutionary tracks reconstructed from the seismic observations for stellar masses in the [ 0.9−2.9 M_⊙] range. The 1.9 M_⊙ track is not shown because more information is needed to define the limit between the clump and secondary-clump stars. On the RGB, the dispersion due to the first luminosity bump is too high to allow an unambiguous definition of the evolutionary tracks for stellar masses above 1.9 M_⊙. Dotted lines indicates the boundaries between evolutionary stages.