Notes. We note that M_ini is the initial mass in M_⊙; α_ov the amount of CBM on the main sequence; D is short for log(D_env/cm²s⁻¹), the amount of envelope mixing; t_H, t_He, and t_tot the duration of hydrogen burning, helium burning, and the total evolution time in millions of years, respectively. We note that M_∗,H, M_∗,He, and M_∗,C are the masses of the stars at the end of their respective burning phases in M_⊙; M_c,He and M_c,C the masses of the hydrogen- and the helium-depleted core, respectively, at the end of the corresponding burning phases in M_⊙; (C/O)_c is the carbon-over-oxygen ratio of the core at the end of helium burning; ²²Ne_tot gives the total mass of ²²Ne at the end of helium burning in M_⊙, ΔM the total mass lost in M_⊙; T_c, f is the final core temperature in K and ρ_c, f is the final core density in g/cm³.