Open Access

Fig. A.1.


Abundance differences between our GIRAFFE analysis and S+03, Δ[X/Fe] = [X/Fe]GIR − [X/Fe]S + 03. In the case of Fe, Δ[Fe/H] is plotted instead. For Ti and Fe, the ionised species are plotted to the right. Dotted lines are the average abundance offsets for each star, while solid cyan lines show the expected GIRAFFE precision.

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