Extended Data Fig. 1: Planetary mass and eccentricity constraints of TOI-2076 b,c,d from different observational sources.
From: An adolescent and near-resonant planetary system near the end of photoevaporation
Top: marginalized planet mass constraints from TTV (blue), RV (gray), and joint photodynamical and RV model (red). First three panels in bottom show the planet mass and eccentricity 1 and 2σ contours plot, color indexed as in top panels. Bottom rightmost panel shows the marginalized distribution of eccentricity from the joint photodynamical and RV model.
