Fig. 3.
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Gaia DR3 Apsis age estimates as a function of the BP − RP colour for single stars in the Hyades (left) and Pleiades (right). The blue horizontal dashed-dotted lines mark the range of ages assigned to the open clusters by isochrone fitting. For both clusters, Apsis age estimates show a strong correlation with the colour of the star for BP − RP ≤ 0.8 mag.
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