Image Details
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).
© 2026. The Author(s). Published by the American Astronomical Society.