Fig. 1.
Left panel: light curve showing the flare on KIC 8414845 with start time at the flare peak (MJD 56285.43). A third-order polynomial function was fitted to the background to account for the modulation of the light curve due to the binary nature of the star (see inset). Right panel: flare model by Gryciuk et al. (2017) superposed on the detrended light curve of the flare.
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