Bottom: first half of the 2.8 year long Kepler light curve from quarters Q06 through Q16, folded on the orbital period and binned into 50 bins, with a model fit as listed in Table 4. Middle: folded second half of the light curve, offset by 0.3 ppt for clarity. The structure in this curve relates to imperfect detrending around gaps in the light curve. Top: phased radial velocities from the spectra from the Nordic Optical (red dots) and William Herschel (blue dots) telescopes.