Image Details
Caption: Figure C2.
Posterior distributions of Kk (left), ek (center), and ωk (right) for the L 98-59 planets from an RV-only fit and the joint RV–TTV fit (fixed-inclination model). The eccentricity distributions are normalized so that their heights are equal to improve visibility. The small TTVs detected on L 98-59 c and d provide significant constraints on the orbital architecture of the system.
© 2025. The Author(s). Published by the American Astronomical Society.