Results from the analysis of the white light curve of HAT-P-32 b. Top panel: normalized raw light curve. Second panel: light curve divided by the best-fit model for the systematics. Third panel: fitting residuals. Bottom panel: autocorrelation function of the residuals. This planet belongs to this group, which is affected by additional systematics (group c in Section 2.4) and as we can see in the lower two panels the residuals are not following a Gaussian distribution.