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Fig. 1

image

Long-cadence transit light curve of KOI-12.01, normalized and phase-folded over the Kepler observations. The best fit to the data is displayed as a red line, with residuals in the lower panel. One of the light curves was found to be abnormally deep, and there is also a small increase in the residual scatter during the transits. These variations should not affect the derived parameters, but may slightly increase their uncertainties.

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