_:n3b24db0787b64712830965ddc7cb867fxb115
<http://schema.org/caption>
"Figure 1. (Left:) Fractional uncertainty on Fbol from the SED fitting procedure as a function of χ 2 ν and of Teff uncertainty. The vertical line represents the cutoff of χ2ν ≤ 5 for which the uncertainty on Fbol is at most 6% for most stars, thus permitting a determination of R? to ≈3%. Points with blue haloes represent stars with transiting planets. (Right:) Distribution of fractional Fbol uncertainties for stars with χ 2 ν ≤ 5. The median uncertainty on Fbol for transiting-planet host stars (blue) is 2%; it is 1.7% for all stars."
<https://www.semanticscholar.org/paper/Accurate-Empirical-Radii-and-Masses-of-Planets-and-Stassun-Collins/b0f0293ad3acb7e228f9be990695d8deefb10217>