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1 Introduction
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2 Sample selection, observations and reductions
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3 Determination of stellar parameters
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4 Abundance determination
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5 Abundance distributions and comparison to galactic samples
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6 Comparison to the dwarf spheroidal galaxies
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7 Discussion
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8 Summary
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Appendix A: Comparison between equivalent width from DAOSPEC and from Splot-Iraf
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References
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Online Material
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