Fig. A.1.
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Comparison of the ULLYSES (blue: LMC; green: SMC) and XSL libraries. XSL stars (filled circles) are separated by metallicity: [Fe/H] > − 0.5 (black) and [Fe/H] < − 0.5 (dark red). Temperatures, gravities, and metallicities of the ULLYSES stars in this figure were obtained from the literature. Solid lines are Geneva isochrones for Z⊙ and various ages (Ekström et al. 2012).
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