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Fig. 5.
Cumulative flare frequency distribution as a function flare energy, log E where E is given in ergs, of the TRAPPIST-1 K2 data (left, cf. Vida et al. 2017) and for long-cadence Kepler data of KIC 1722506 (right). In the right plot, the dashed line marks the upper energy limit used for the fit.
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