Top: synthetic Kepler light curve of secondary-only EB (as described in the text) with their best planetary model and residuals. From left to right, light curve are generated assuming the 1–0.5 M_⊙  secondary-only EB diluted by a gravitationally bound 1 M_⊙ star, the undiluted 1–0.2 M_⊙ secondary-only EB and the undiluted 1 M_⊙ –0.5 M_⊙ secondary-only EB. Bottom: posterior distribution from the MCMC analysis of the aforementioned secondary-only EBs, displaying the correlation between the orbital inclination and the planetary radius (assuming a 1-R_⊙ host). Colors and ranking from left to right are the same as for the upper plot. Vertical lines indicate the radius of Neptune (dotted line), the radius of Jupiter (dashed line), and twice the radius of Jupiter (solid line).