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Fig. 6

image

Temporal distribution of the flare fluxes and fluences. The mean arrival times of the flares without observing gaps and with the correction of the average flare detection efficiency 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 are only lower or upper limits on the flare flux and fluence due to the truncated flare duration when it begins before the start of the observation or ends after the stop of the observation. Top panel: the mean unabsorbed flux distribution is shown. Bottom panel: the mean unabsorbed fluence distribution is shown.

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