Fig. 9.
Pseudo-HR diagram of our results with the full sample, plotting both the derived log g and log g after corrections based on trigonometric log g from Delgado Mena et al. (2017) against Teff for all the stars in the sample. Worst outlier stars are excluded from this plot. PARSEC isochrones with [M/H] = 0.0 dex from Bressan et al. (2012) are overplotted.
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