Figure 4 from TTV-determined Masses for Warm Jupiters and Their Close Planetary Companions

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TTV-determined Masses for Warm Jupiters and Their Close Planetary Companions

Authors: Dong-Hong Wu, Songhu Wang, Ji-Lin Zhou, Jason H. Steffen, and Gregory Laughlin

2018 The Astronomical Journal 156 96.

Provider: AAS Journals

Caption: Figure 4.

Combined posterior mass and eccentricity distributions for the planets in Kepler-30. The dark and gray circles indicate the 68.3% and 95.5% confidence regions, respectively. Histograms show the marginalized mass and eccentricity posterior distributions from the DEMCMC.

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