Fig. 11
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Residuals for metallicities between HRS (Spina et al. 2021) and LRS with respect to effective temperature and surface gravity. The blue dots are the difference between HRS and the original result from LRS, and the orange circles show the difference between HRS and LRS after correction. The gray shadow highlights stars with Teff < 5000 K and log g > 4.5 dex.
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