Figure 5
νFν plots of model D indicating the strength of any soft excess and relativistic line emission from the kerrdisk models. Consisting of powerlaw +comptt (where required) + unblurred reflionx+kerrdisk+ narrow ionized lines as required. XIS data are in black, HXD in red and BAT data are represented by blue circles.

νFν plots of model D indicating the strength of any soft excess and relativistic line emission from the kerrdisk models. Consisting of powerlaw +comptt (where required) + unblurred reflionx+kerrdisk+ narrow ionized lines as required. XIS data are in black, HXD in red and BAT data are represented by blue circles.

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