Duration of the various post-MS phases (colors) for each grid of models using the MS mass-loss prescriptions by Vin01 (top row) and Bes20 (bottom row), at solar metallicity (left column) and LMC metallicity (right column). The dashed white vertical lines represent the approximate location of the break between the low and high MS mass-loss regimes. The durations are shown cumulatively, so there is no information about the order in which the different phases are traversed. Furthermore, the x-axis is a power scale (where $x\sim M_{\mathrm{ini}}^{-1.35}$), designed in such a way that the area of a region corresponding to one phase is proportional to the number of stars currently in that phase, assuming a population of constant star formation rate using the standard initial mass function by Salpeter (1955).