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To compare the chemistries of stars in the Milky Way dwarf spheroidal satellite galaxies (dSph) with stars in the Galaxy, we have compiled a large sample of Galactic stellar abundances from the literature. When kinematic information is available, we have assigned the stars to standard Galactic components through Bayesian classification based on Gaussian velocity ellipsoids. As found in previous studies, the [α/Fe] ratios 1 This work was completed while visiting the Institute

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We describe the Sloan

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