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Fig. 3

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Predicted metallicity distribution functions (top row); age-metallicity relations (second row); [O/Fe]-[Fe/H] relations (third); and [O/Fe] distributions (bottom row), for “solar neighbourhood” regions of the MaGICC (left column: Stinson et al. 2013) and MUGS (right column: Stinson et al. 2010) realisations of simulation g1536.

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