Fig. 6.
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Upper panel: comparison between the metallicity distribution derived in this work (black line) with those derived by Hayes et al. (2020, H20 samples) for Sgr main body (blue line; 710 stars) and Sgr stream stars (light blue line; 166 stars). Lower panel: Same comparison, but with the Sgr APOGEE DR17 H21 sample (red line; 1034 stars). The distributions are normalised to have a unit area.
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