Fig. 11

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Comparison between evolutionary and spectroscopic masses. The color bar represents the effective temperature of the targets with lighter colors reflecting lower Teff. The fuchsia hexagons correspond to the data of Trundle et al. (2004) and Trundle & Lennon (2005) and the dotted blue lines connect the same stars. The darker horizontal orange and gray bands represent, respectively, the intervals of 1σ obtained for G13 and B11. Likewise, the lighter colored bands are for 2σ.
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