Image Details
Caption: Figure 15.
Eccentricity posteriors for TOI 560 b and c from our ExoFASTv2 results. The eccentricity values are on the horizontal axis, and the normalized probabilities are on the vertical axis. The colored histograms show individual MCMC walker chains, with the black histogram showing the medians of all walkers. The posterior for TOI 560 b slightly favors a mild eccentricity, whereas for TOI 560 c, a circular orbit is preferred.
© 2022. The Author(s). Published by the American Astronomical Society.