Fig. 2
Upper panel: distribution of the Teff of the 119 stars in our sample with Teff taken from the literature (Huber et al. 2014; Frasca et al. 2016). Lower panel: comparison between the Teff drawn from the literature and the ones obtained with the SED fitting is reported for thesame sample of stars. The colors represent the original work in which the Teff was derived.Blue: Frasca et al. (2016); red: Huber et al. (2014).
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