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Fig. 4.

image

Temporal distribution of the flare fluxes and fluences. The mean arrival times of the flares without observing gaps are represented by vertical lines. The dotted lines are the time of the beginning of the first observation of the year. The blue, green, and red lines are the Chandra, XMM-Newton, and Swift flares, respectively. The dashed lines tag the flares that begin or end outside the GTIs. Top panel: mean unabsorbed flux distribution. Bottom panel: mean unabsorbed fluence (flux time duration) distribution.

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