Image Details
Caption: Figure 2.
The posterior probability density distribution of planetary eccentricities for LP 791-18 d and c with a fit to the TTV data of P23 using a tidally damped-state eccentricity prior and parameterizing e and ω as ﹩\sqrt{e}\cos (\omega )﹩ and ﹩\sqrt{e}\sin (\omega )﹩.
© 2025. The Author(s). Published by the American Astronomical Society.