Fig. 4
Mean flux and difference S/N of the new transit candidate on the Kepler pixel map around Kepler-160 (center pixel) for Q5 (a, b), Q9 (c, d), and Q13 (e, f). The positions and Kepler magnitudes of Kepler-160 and two nearby sources are indicated with dots and labels. The difference S/N maps show that the transits are not caused by the nearby sources.
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