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Table 1

Fit parameters for the baseline models discussed in Sect. 5.

Model 1: pexrav (var. cold refl.)
Γ
Ecut (keV)
R
χ2/d.o.f. 327.1 / 367

Model 2: pexrav (const. refl.)
Γ
Ecut (keV)
R 3.8 ± 1.4/1.7 ± 0.8a
χ2/d.o.f. 327.7 / 367

Model 3: pexrav × zxipcf (ion. abs.)
Γ 2.33 ± 0.10
Ecut (keV)
NH (cm-2) 1.3 ± 0.3 × 1024
CF 0.62 ± 0.1
log ξ (erg cm s-1) 2.4 ± 0.4 b
χ2/d.o.f. 325.5 / 365

Model 4: relxill_lp (relativistic refl.)
Γ 2.26 ± 0.04
h (rG) < 3.5
a > 0.68
cos(i) > 0.83
log ξ (erg cm s-1) 1.8 ± 0.5 c
χ2/d.o.f. 333.8 / 365

Notes. Model 1 is a PEXRAV model with all the parameters linked between XMM-Newton and NuSTAR, except for the normalizations. Model 2 has the normalization of the reflection component linked between the XMM-Newton and NuSTAR data, while the primary power law is left free to vary independently, so that the two data sets have two different R parameters. The Γ and high-energy cutoff are linked between the power-law and the reflection component, and between the two data sets. Model 3 includes an ionized absorber with partial covering superimposed on a PEXRAV model with R = 0. Model 4 is a RELXILL_LP relativistic reflection model, where the Ecut is frozen to 300 keV. In Models 1, 2, and 3 the inclination angle is frozen to the default value cos(i) = 0.45.

(a)

R values for XMM-Newton and NuSTAR, respectively.

(b)

Ionization parameter of the obscuring material.

(c)

Ionization parameter of the accretion disk.

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