Free Access

Fig. 6


Spectral evolution seen during the large flare. The 3–10 keV spectra taken from (i) 68–72 ks; (ii) 72–80 ks; and (iii) 80–88 ks in Fig. 4 are shown. The histogram indicates the best-fit photoionized absorption model (see text). The Fe K emission lines are modelled by a Gaussian. The dotted line indicates the observed energy of 6.5 keV where the mean Fe K line peaks.

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.