Image Details
Caption: Figure 8.
Corner plot of posteriors for TTV model parameters for LP 791-18 d and c from the damped eccentricity (red) and nondamped (blue) versions of the TTV fit, made with the corner package (D. Foreman-Mackey 2016). Fit parameters included planet-to-star mass ratios but we have converted these distributions into units of Earth masses for ease of reference. Columns labels are displayed for the undamped fit results.
© 2025. The Author(s). Published by the American Astronomical Society.