Image Details
Caption: Figure 2.
Left panel: number of stars in bins of iron abundance, [Fe/H], that pass the quality cuts described in Section 2. Right panel: distribution of stars in our sample in stellar parameters log(surface gravity), ﹩\mathrm{log}g﹩, and effective temperature, ﹩{T}_{\mathrm{eff}}﹩, with points colored by the iron abundance.
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