Figure 2
The 0.5–70.0 keV spectrum and residuals after modelling of the continuum with a powerlaw, neutral reflection from the pexrav model, comptt to model the soft excess and wabs to account for Galactic absorption; the entire Fe K region is left unmodelled. XIS data are in black, HXD in red and BAT data are represented by blue circles.

The 0.5–70.0 keV spectrum and residuals after modelling of the continuum with a powerlaw, neutral reflection from the pexrav model, comptt to model the soft excess and wabs to account for Galactic absorption; the entire Fe K region is left unmodelled. XIS data are in black, HXD in red and BAT data are represented by blue circles.

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