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\label{fig:keplerfig} \emph{Kepler} light curve of the eclipsing binary KIC 9246715 \revise{with out-of-eclipse points flattened}. \emph{Top:} Detrended SAP flux over 17 quarters. quarters \revise{with out-of-eclipse variability removed}.  The detrending process is described in Section \ref{kepler}. \emph{Middle:} Folded version of the above over one orbit. The dotted lines indicate the portion of the light curve used in subsequent modeling. \emph{Bottom:} A zoomed view of secondary and primary eclipses corresponding to the dotted lines above. To avoid overlaps, each observed eclipse is offset in magnitude from the previous one. The colored disks illustrate the eclipse configuration, with the red disk representing Star 1 and the yellow disk representing Star 2.