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Fig. 3.

Radii determined using the spectroscopic Teff from Sect. 3.2, the bolometric luminosity from Sect. 3.1, and Stefan–Boltzmann’s law plotted against interferometric radii from Boyajian et al. (2012b). The two discussed outliers are Gl 411 and Gl 412A with Rinterf of 0.392 and 0.398 R⊙, respectively.
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