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) planet radius (R_pl), (2) radius ratio of neighbor planets (R_j/R_j−1 for 2 ≤ j ≤ m_int), and (3) transit depth (δ).