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Fig. 1.

image

Distribution of the background-subtracted J12270 count rate obtained from 20 s binned lightcurves from the 2009 January and 2011 January XMM-Newton EPIC data. We define the region between 0 cts s−1 and 2 cts s−1 as the low-soft mode, while the region between 4.6 cts s−1 and 9 cts s−1 is the high mode. Higher than 12 count s−1 we define flare mode. In the zoomed plot we can see that the double Gaussian fit does not interpolate data during the flares.

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