Figure 6.
Upper panel: the pn and NuSTAR spectra above 3 keV fitted with a model including a simple power law and three Gaussian lines. Lower panel: the ratio of the spectra to the model, showing an excess around 30 keV. The data were binned for plotting purposes.

Upper panel: the pn and NuSTAR spectra above 3 keV fitted with a model including a simple power law and three Gaussian lines. Lower panel: the ratio of the spectra to the model, showing an excess around 30 keV. The data were binned for plotting purposes.

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