Free Access

Fig. 4.


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.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.