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Fig. B.1


XMM-Newton flares detected using the Bayesian blocks algorithm with a false positive rate for the flare detection of 0.1% from 2000 September to 2015 April. The black crosses are the pn light curves and their error bars. The bin size of the light curves are reported on the top of each figure. The red lines are the Bayesian blocks with their errors in horizontal gray rectangles. The vertical gray stripe is the bad time interval. Each flare is labeled with the index corresponding to the flare number in Table A.1. The horizontal line is the flare duration. See caption of Fig. B.2 for details.

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