Parametrization of stellar evolution as function of the timescale-adapted evolutionary coordinate over phases beyond the ZAMS−TACHeB sequence. Stars across the initial mass range are evolved from the pre-MS up to post-CHeB evolution (post-asymptotic giant branch evolution for low-mass stars, and onset of core carbon burning for massive stars) as function of (unnormalized) timescale-adapted evolutionary coordinate . The color marking denotes the evolutionary phases pre-main sequence (PMS), main sequence (MS), red giant branch (RGB), core helium burning (CHeB), early asymptotic giant branch (EAGB), thermally pulsating asymptotic giant branch (TPAGB), post asymptotic giant branch (postAGB), and Wolf-Rayet (WR) phase.