Data and best-fit models for KOI-200 (left) and KOI-889 (right). The parameters of the fits are reported in Table 4. Upper panels: Kepler phase-folded light-curve (black dots with 1-σ error bars) over-plotted with the best model (red line), and residuals. Middle panels: SOPHIE (red circles) and HARPS-N (blue squares) radial velocities and 1-σ error bars phase-folded to the orbital period of the planet (left) or as function of time (right) over-plotted with the best model (black line), and residuals. Lower panels: fitted spectral energy distribution (black line) over-plotted with measured magnitudes (red circles, Table 1) and corresponding integrated flux in each of the photometric bands according to the fit (open circles).