Fig. 7.
Time-averaged XMM-Newton spectrum with best-fitting 2-BPL model (Sect. 3.1). Upper panel: OM (red) and pn (black) data with folded model. Middle panel: data-to-model ratio. Lower panel: best-fitting model E2f(E), without Galactic absorption and reddening, including the double-broken power law (dashed line) plus the blackbody, the Gaussian line, and the host galaxy (dotted lines). The data were binned for plotting purposes.
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