Fig. 8.

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Cumulative distributions of flares per day with energies above a given threshold (log N(E > E0)). Dashed line indicates the full sample of flares (Nflares = 60); thin solid line is relative to the flares observed at planetary transits (Nflares = 47); thick solid line is relative to the flares observed at secondary transits (Nflares = 13). The lines refer to a linear fit of each sample in the form log N(EX > E0)∝βlog EX. The range with energies log EX < 31.2 not used for the fit to the slopes is shaded in gray color.
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