Top: phase-folded primary transit light curve of Kepler-5. The upper curve shows the circular fit, the bottom curve the eccentric fit. Solid (blue) lines indicate the best-fit resampled model (with bin number 4). The dashed (red) lines show the corresponding unbinned model, which one would get if the transit was observed with infinitely fine time resolution. Residuals from the best-fit resampled model for the circular and eccentric solutions are shown below in respective order.