Fig. 2
Rise of the flare observed during the XMM-Newton observation of IGR J18410-0535 with the Epic-pn camera. The start time of the lightcurve is the same as that in Fig. 1, and the binning time is 150 s. The upper panel shows the source lightcurve in the soft energy band (0.3–4 keV), the middle panel in the hard energy band (4–12 keV), and the bottom panel the hardness ratio (HR, defined as the ratio of the source count-rate in the soft to hard energy band versus time).
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