Fig. F.1.
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M*/L ratio derived from XSL PARSEC/COLIBRI (P/C) Salpeter models (orange), XSL Padova00 (P00) Salpeter models (green), and E-MILES BaSTI Salpeter models (black). The shaded areas represent the spread in M*/L arising from the metallicity spread from [Fe/H] = −0.4 dex (lower log M*/L) to [Fe/H] = +0.2 dex (higher log M*/L), centred on the solar-metallicity values.
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