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Fig. 13

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[Y/Eu], [Ba/Eu], [Ba/Y] vs. [Fe/H] at all metallicities, and [Ba/Fe] vs. [α/Fe] of stars more metal-rich than [Fe/H] =−1.5 in our sample compared to literature samples of MW halo stars and of stars in MW dwarf galaxies (for the symbols see legend in Figs. 8 and 9).

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