Final stellar sample. Top to bottom: a) the distribution of stars in the Z vs. R plane; b) and c) radial gradients in the MW disk for [Fe/H] and [Mg/Fe]; d) the [Fe/H] − [Mg/Fe] relation. Colour represents age of a star. The three young open clusters, which are available in UVES iDR1, are shown with large crosses.
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