Fig. 1
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Left panel: sample of 7347 field stars from Magrini et al. (2021), with our selected subsamples highlighted in red and blue. Right panel: mass distribution with metallicity ([Fe/H]) of stars in our selected samples. The blue error bar indicates the mean uncertainty value of our selected dwarf MS sample. The black vertical line marks [Fe/H] = -0.8 dex.
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