Fig. 2

Phased and binned (to half-hour bins) light curves of the Kepler-87 system components relative to the time of mid transit, with over plotted best-fitting models. From top to bottom: transiting exoplanets Kepler-87 b and c and planetary candidates KOIs 1574.03 and 1574.04. Above each light curve we show the model residuals, shifted for clarity. We note the vertical scale in each panel may be different.
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