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Fig. 10

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Comparisons between our observations (red dashed histograms) and the Besançon model predictions (black solid histograms) for the metallicities, rotational (V in Cartesian and Vφ in cylindrical coordinates system) and radial velocities. The left-side plots include the stars that are lower than 1 kpc, whereas the right-side plots include the stars farther than 1 kpc from the plane. Dotted black histogram corresponds to the raw Besançon model (as downloaded from the web, but biased to match our magnitude distribution), whereas the black continuous line corresponds to a model with a richer by 0.3 and 0.2 dex thick disc and halo, respectively.

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