Fig. D.1.

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HR diagrams of PARSEC versions 1.2s (solid green) and v2.0 (dashed pink) presented in this work for three metallicities. Cyan and orange stars indicate the final pre-SN location in the HR diagram of stellar tracks computed with PARSEC v1.2s and v2.0, respectively. The initial mass of each is indicated near the ZAMS in solar masses. Diagonal dashed gray lines indicate constant stellar radii as labeled. It is worth noting that for Z = 0.0001, the helium abundances are slightly different Y = 0.249 and Y = 0.2487 for v1.2 and v2.0, respectively.
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