a. based on isochrone fits using ρ∗, from MCMC model and Teff and [Fe/H] from spectroscopy.
b. from MOOG analysis
c. from MCMC model
d. from TTV model e derived from other parameters

Kepler lightcurves for K00137. The upper panel shows the normalized raw Photometric Analysis (PA) lightcurves for quarters 0 through 6. The various discontinuities are due to effects such as spacecraft safe-mode events or loss of fine pointing. Each quarter put the star on a different detector, which accounts for the change in overall sensitivity. The long-term drifts in each quarter are temperature related. The lower panel shows the normalized corrected Pre-search Data Conditioned (PDC) lightcurve. Most of the spacecraft-related variability of the PA lightcurve has been removed.