Examples of Kepler light curves where the polyfit and the two-Gaussian model give discrepant results. The plots show the observed Kepler light curve (gray dots) in normalized Kepler (K) magnitude, polyfit model (solid red line), and two-Gaussian model (dashed black line). Top left: light curve where both models agree; top right: no primary eclipse detected by the two-Gaussian model; bottom left: no secondary eclipse detected by the two-Gaussian model; bottom right: no secondary eclipse detected by polyfit.