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Fig. 6

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Phase distribution of the TESS flares on the primary component in the reference frame of the binary orbit. The relative radii and separation of the circles are for scale. The colors are realistic digital colors for the given spectral types from Harre & Heller (2021). The gray area shows a Gaussian kernel density estimation with the bandwidth of 2°. Black ticks denote the orbital phase values of the flare observations.

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