New analysis of the RV dataset and its results on planet e. Top: priors and posteriors of the new analysis from Suárez Mascareño et al. (2022) where we include the constraints from TESS on its orbital period (Feinstein et al. 2022). Bottom: derived distributions of the planetary and orbital parameters. We note that we used the updated planetary radius from TESS (Feinstein et al. 2022) in our analysis in place of the one appearing in this figure, which is still based on the Kepler and K2 data, as in Suárez Mascareño et al. (2022).