Figure 3 from Accurate Empirical Radii and Masses of Planets and Their Host Stars with Gaia Parallaxes

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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 3.

Fractional uncertainty (left) and absolute uncertainty (right) on Θ for transiting-planet host stars (blue) and for all stars (black). One star with a fractional uncertainty larger than 0.1 is not shown in the left panel, and 15 stars with uncertainties larger than 20 μas are not shown in the right panel.

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