Fig. 3.
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XMM-Newton, Chandra, and NuSTAR spectra with a warm absorbed relativistic reflection model. Upper panel: unfolded spectra with the best fitted warm absorbed relativistic reflection disk model. Middle panel: ratio of the data and model with a simple power law plus a Guassion line for the 2–10 keV band spectra and extrapolated to 0.2–10 keV of XMM-Newton and Chandra spectra and the 3–70 keV of the NuSTAR spectrum. Bottom panel: ratio of the data and model with the best fitted warm absorbed relativistic reflection disk model.
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