Fig. D.1
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HR diagrams of the clusters with N>1 members which do not host Li-rich stars sorted by age. The OC parameters are taken from Table 5. The isochrones are taken from the PARSEC tracks. The left panels are the spectroscopic parameters and in the right the photometric Teff and trigonometric log ɡ. Non-members and stars with low signal to noise ratio are excluded.
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