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Fig. 14.

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Median [O/Fe] and [Fe/H] for the stellar halo and each of its stellar populations: in-situ, endo-debris, and ex-situ, color-coded by the stellar halo mass (see color and symbols code in Fig. 10). The linear fit for the relation for the whole stellar halo abundances is included (black line; the shadow region is delimited by standard deviation).

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