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Fig. 14.

image

Comparison of the relations of stellar age and mean metallicity [Fe/H] (left) as well as mean [α/Fe] (right) for the stars of this study (black) and the stars from Bensby et al. (2014; blue), showing that the two relations agree between the studies within their uncertainties. The data points are calculated in 1.5 Gyr steps from 1 to 14.5 Gyr) and the errors are the means of the age uncertainties as well as the standard deviations for the mean [Fe/H] and [α/Fe], respectively.

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