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Fig. 3

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Panel a) optimal BLS spectrum of Kepler’s KOI 1574 (blue) and its BLSternd (red) after removing planet candidate KOI 1574.01 using all available data through Quarter 13. Panel b) same, after removing BLSternd. Panels c), d) two zoomed-in regions with significant local peaks. Optimal frequency sampling is evident by the fact that each peak is sampled with similar number of samples despite the large difference in width.

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