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Accurate Empirical Radii and Masses of Planets and Their Host Stars with Gaia Parallaxes

  • Authors: Keivan G. Stassun, Karen A. Collins, and B. Scott Gaudi

2017 The Astronomical Journal 153 136.

  • Provider: AAS Journals

Caption: Figure 2.

SED fits for the stars HD 189733 (left) and HD 209458 (right), for which interferometric angular radii have been reported (Boyajian et al. 2015) as a check on the Θ and ﹩{F}_{\mathrm{bol}}﹩ values derived in this work. The two SED fits have ﹩{\chi }_{\nu }^{2}﹩ of 1.65 and 1.67, respectively. The Θ and ﹩{F}_{\mathrm{bol}}﹩ comparisons are presented in Table 1. Symbols and colors are as in Figure 14.

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