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Fig. 5.


Left: [Ba/Fe], [Eu/Fe], [Gd/Fe], and [Dy/Fe] ratios in the thin disc (blue), thick disc (red), and in the mrαr population (green). Middle: average abundances binned in metallicity every 0.2 dex. The orange curves show the Galactic chemical evolution models of Prantzos et al. (2018). Right: corresponding normalized distributions.

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