Fig. 5
Intensity vs. observation number of the 10 XMM-Newton pointings of the 2009 campaign. The black dashed line shows the rescaled (with the mean 3–10 keV flux equalling the mean line intensity) 3 − 10 keV source flux. The intensity of the resolved component of the Fe Kα line follows, with a 1-to-1 relation the 3–10 keV continuum variations without any measurable lag. 1σ errors are shown.
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