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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 14.

The marginalized best-fit ﹩{{ \mathcal M }}_{{\rm{int}}}﹩ from the ﹩{{ \mathcal M }}_{228}﹩ (Poisson, red lines) and ﹩{{ \mathcal M }}_{235}﹩ (Zipfian, blue lines) models. 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) radius partitioning (QR), (2) radius monotonicity (MR), and (3) gap complexity (﹩{ \mathcal C }﹩) (G. J. Gilbert & D. C. Fabrycky 2020; M. Y. He et al. 2020).

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