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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 5.

The marginalized best-fit observed multiplicity distributions (red lines) from ﹩{{ \mathcal M }}_{220}﹩ (top panel), ﹩{{ \mathcal M }}_{221}﹩ (middle), and ﹩{{ \mathcal M }}_{222}﹩ (bottom) are compared to the marginalized ﹩{{ \mathcal D }}_{{\rm{kep}}}﹩ (blue histogram and blue lines). The two columns of plots show the differential (left) and cumulative distribution functions (right).

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