Fig. 8
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Abundances for the high-confidence sample, plotted as [Mg/H] against [Si/Mg]. The sample is split according to the kinematic selection made in Paper I, and also into different dwarf galaxies according to Battaglia et al. (2022) and for the Magellanic Clouds, the selection made in Paper I. The median errors for the abundances are shown in the bottom left corner.
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