Binned residuals for the sample of large planets on long orbits. Contrary to Fig. 8, the x-axis is the distance from the stellar limb to the planet centre in units of planet radii. The blue line is the theoretical prediction for a Jovian planet on a 20-day orbit. It is equivalent to the blue line in Fig. 4 as observed through the 30-min long cadence of Kepler. Negative distances are when planets are inside of the stellar disc and positive distances are outside. The vertical black lines mark when the planet limb and centre cross the star limb.