Flux difference between the observed measurement and the transit model for data points inside the transit region. Outliers mostly due to the misidentification of cosmic rays by the Kepler pipeline are marked in the same color code as in the right panel of Fig. 5. The Kepler quarters of the mission with few or no data for this KOIdue to the failure of CCD Module 3 are highlighted as gray shaded regions(see Sect. 2.1).