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This article has an erratum: [https://doi.org/10.1051/0004-6361/202142441e]


Fig. 12.

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Age distribution of our programme stars derived by applying the period–age relations by De Somma et al. (2021) for two assumptions on the amount of core convective overshooting during the core H-burning stage: no extension above the canonical value predicted by the Schwarzschild criterion (canonical scenario, solid blue line), or a moderate core overshoot (non-canonical scenario, dashed red line).

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