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Fig. 2

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Part of the TESS light curve from sector 6 corrected to the variability caused by stellar spots. The red curve and red interval mark the modulated flare model and the fit error, respectively. The green curve shows the recreated course of the stellar flare without the effects of foreshortening or stellar rotation. The gray points mark the data not used in the analysis. The translucent red area presents the uncertainty area.

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