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Fig. 5
Our XRT/JEM-X/ISGRI combined spectra during the INTEGRAL revolutions 1145 and 1146 (see text for details). The best-fit model is obtained by using a power law with a high-energy cut-off plus a cyclotron absorption-line at ~20 keV. The mid panel shows the residuals from the fit when the cyclotron feature is not included.
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