Fig. B.1
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Gaia metallicity estimates for our sample compared to values determined from APOGEE and GALAH. Panel (a): APOGEE. Panel (b): GALAH. The Gaia estimates show a larger fraction of low- and high-metallicity stars, while the APOGEE and GALAH samples are more centralised around 0. The colour represents the density of points, while the grey dashed line shows the x=y diagonal.
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