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Fig. 5
[F/Fe] and [O/Fe] as functions of [Fe/H] for the B3-BW-B6 stars. The stars are color-coded as the corresponding fields in Fig. 1. The black dots are the microlensed bulge dwarfs of Bensby et al. (2013) that are also marked in Fig. 1. Conservative estimates of the uncertainties are marked in the upper corners.
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