Image Details
Caption: Figure 6.
Marginalized posterior distributions of the orbital eccentricities of the L 98-59 planets from the joint TTV–RV fit (fixed inclinations) using the full data set (black) and TTVs from TESS only (red). The 2D posteriors show 1σ, 2σ, and 3σ contours.
© 2025. The Author(s). Published by the American Astronomical Society.