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Fig. 1

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Diagnostic plots for NGC 6811. Panel a: apparent Gaia CMD colored according to the rotation period (Van-Lane et al. 2025). Panel b: distribution of Protation and Gaia G magnitude colored according to the temperature. If the temperature was unavailable, the stars are shown as gray dots. Panel c: distribution of Protation and temperature colored according to the G magnitude. The BL candidates (black squares) and the automatically detected outliers (red crosses) are highlighted.

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