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Fig. B.1.


X-ray flares detected using the Bayesian blocks algorithm in 2016–2018. All these flares were observed during Chandra observations. The black crosses are the count rates and their error bars. The bin sizes of the light curves are reported at the top of each figure. The red lines are the Bayesian blocks and their errors are horizontal gray rectangles. Each flare is labeled with the index corresponding to the flare number in Table A.2. The horizontal line is the flare duration.

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