Fig. 3
a) Unfolded XMM-Newton and RXTE data and best-fit model components. Green line: reflection continuum in the frame of the disk (note the strong Compton broadening; the “jitter” above 50 keV is due to the numerical resolution of the reflection model). Purple line: relativistically smeared reflection component. b) Measured count rate spectra. c) Residuals of the best-fit setting the relativistic convolution to zero. d) Best-fit residuals including relativistic convolution.
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