A smoothed 2D probability distribution function of planets consecutively transiting eclipsing binaries, having a mutual inclination following a 1° Rayleigh function. The darker the colour, the more probable planets are. Blue dots indicate Kepler-16, -34, -35, and -64. Squares are for the other circumbinary systems which fall outside the bounds of our simulation. Only the innermost circumbinary planets are shown. The black line delineates an approximation of the stability limit P_p = 4.5 P_bin. Side histograms give the marginalised probabilities.