Fig. A.2
Flare distribution seen by Chandra and the detection probability of the Bayesian-blocks algorithm during an observation with XMM-Newton. The crosses are the X-ray flares detected during the Chandra XVP campaign of 2012. Left panel: the flare amplitude above the non-flaring level seen by EPIC/pn during the 2011 campaign. Right panel: the flare amplitude above the non-flaring level seen by EPIC/pn during the 2014 Feb. 28 observation.
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