Fig. 16
Comparison between theoretical isochrones and our photometry (PARSEC isochrone of solar metallicity, 316 Myr, shifted by E(B − V) = 0.40 and (V − MV) = 11.45 and Dartmouth isochrone of solar metallicity, 250 Myr, E(B − V) = 0.37, (V − MV) = 11.6). The grey points are all the stars in our photometry, while the red points are the radial velocity members.
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