Relativistic reflection within an extended hot plasma geometry

Open Access

Fig. 6.

(a) Time-averaged XMM-Newton and NuSTAR spectrum of ESO 033-G002 extracted and binned according to Sect. 4.1 and the full Model 2a in black. (b) Components of the best-fit of Model 2a for ESO 033-G002. The parameters of the fit are listed in Table 2 and the residuals are shown in Fig. 7c.

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