Fig. 1
Comparison of the radii derived from interferometrically calibrated photometric data by Bourgés et al. (2017) with the 0.8 Gyr PARSEC isochrones for [Fe/H] = 0.0, + 0.12, and + 0.19, plotted withred, black, and green lines, respectively. The outliers are indicated by the pale dots and constitute a subset of the CMDoutliers shown in the inset.
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