Image Details
Caption: Figure 3.
The marginalized best-fit ﹩{{ \mathcal M }}_{{\rm{obs}}}﹩ from the ﹩{{ \mathcal M }}_{219}﹩ model (red lines) is compared to the marginalized ﹩{{ \mathcal D }}_{{\rm{kep}}}﹩ (blue histograms and blue lines). The two columns of plots show the differential (left) and cumulative distribution functions (right). From top to bottom, the rows of plots show: the (1) planet radius (Rpl), (2) radius ratio of neighbor planets (Rj/Rj−1 for 2 ≤ j ≤ mobs), (3) transit depth (δ), (4) transit duration (Tdur), and (5) period-normalized transit duration ratio (ξ).
© 2026. The Author(s). Published by the American Astronomical Society.