Data and best-fit model for KOI-686. Top row: phase-folded Kepler LC (left) and SC (right) light curves. Bottom row: SOPHIE RV curve (left), and spectral energy distribution (right). The Kepler data are corrected for contamination and normalized to the out-of-transit flux listed in Table 7. The model of the Kepler LC data is shown binned down to the data sampling rate. For the SED, the best-fit spectrum is plotted as a solid black curve, and the integrated fluxes in the photometric bands are plotted as open circles.