_:n3b24db0787b64712830965ddc7cb867fxb128
<http://schema.org/caption>
"Figure 10. Comparison of spectroscopic log g versus transitderived log g for transiting planet host stars. There is a tendency (red solid line) for the spectroscopic log g to be overestimated at high Teff and underestimated at low Teff , by ∼0.1 dex. The sense of this trend is in the same sense as the systematics observed in the masses derived from spectroscopic log g for the radial-velocity planet hosts (Fig. 9, right). The correction previously suggested by Mortier et al. (2014) (solid black line) is somewhat larger than what we find here."
<https://www.semanticscholar.org/paper/Accurate-Empirical-Radii-and-Masses-of-Planets-and-Stassun-Collins/b0f0293ad3acb7e228f9be990695d8deefb10217>