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Fig. 9

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Comparison of metallicity determinations for a set of common stars in between p1m4 sample and that studied in Hill et al. (2011) in Baade’s Window. Left panel: scatter plot of individual metallicity determinations. Right panel: the MDF from Hill et al. (2011) has been displaced by 0.21 dex and is overploted with the MDF of the common stars from the field p1m4.

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