Notes. The values in this table are based on the residuals of the full dataset (Spitzer and Kepler) and the Toy model without redistribution fit. The photon noise-limited root-mean-square (rms) was calculated like the following: , where rms_obs is the rms of the residuals. β describes the ratio between the achieved standard deviation (rms_obs) of the binned residuals and the standard deviation in absence of red noise. It was calculated using the “time-averaging” method (Pont et al. 2006; Winn et al. 2007, 2008) by calculating median values of this ratio for binnings around the transit duration. The Allan deviation plots for each AOR can be found in Section C.4.