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Fig. 2


Flare detection efficiency of the Bayesian blocks algorithm (top panel) and the Degenaar et al. (2013) detection method (bottom panel) in the Swift observations. The points are the simulation grid for the Gaussian flare light curve above a non-flaring level of 0.027 counts s-1 in the 2–10 keV energy range. The contour levels are the detection probabilities in percent.

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