Fig. 5
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Inferred metallicity distribution of JP×Gr16.55kpc sample (solid histogram) for stars with absolute r magnitudes fainter than 4.2 mag, using Grid A from Table 3. The dash-dotted line shows the metallicity distribution of an APOGEE DR17 sample, selected as described in Appendix A.2. The dashed line indicates the normal function adopted as the prior on [M/H] for the PARSEC models.
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