Eclipsing binary model fits with PHOEBE 2 to independently filtered KASOC light curve for KIC 10001167. Top panels illustrate the binned light curve (black points) and model (red) with time on the x-axis. Middle panels show the same, but with orbital phase on the x-axis. The bottom panels show zoomed-in views of just the two eclipses (phase-folded). The data have been binned in time, in three different ways depending on phase. See the text for details. The gaps between different binnings is a consequence of time-averaging within the bins, and a hard cut to avoid data overlap between them.