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Fig. 2
Left: residuals in the (rest-frame) iron line band, after a 3–10 keV fit on the three Suzaku XIS spectra, with a simple power law. Right: the same as above, but for model III, after the relativistic component of the iron line is removed (see Table 1). Data have been rebinned for clarity.
This figure is made of several images, please see below:
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