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ExoMOD. I. A Forward Model for the Orbital Architecture of Kepler Multiplanet Systems

  • Authors: David Nesvorný, Daniel A. Yahalomi, David Kipping, Cristian Beaugé

David Nesvorný et al 2026 The Astrophysical Journal 1008 .

  • Provider: AAS Journals

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).

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