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Fig. 13
Comparison of our integrated-light [Na/Fe] and [Mg/Fe] abundance ratios with measurements of individual stars from Carretta et al. (2009b, C2009) and Roediger et al. (2014, R2014). Slight offsets to the right and left have been applied to our integrated-light data points and those of Roediger et al. (2014) for clarity.
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