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Table 2

Results from spectral fits.

Model Parameter Cha2000 Cha2007 XMM

1 (APL) Γ
NH( × 1022 cm-2)  <1.20  <0.64
C-stat/d.o.f. 137.3/170 270.1 / 268 493.2/529

2 (APL+Gauss) Γ
NH( × 1022 cm-2)  <0.89  <0.41

Eline (keV)
σ (keV)  <0.95  <0.42
EW (keV)
C-stat/d.o.f. 117.0/167 247.0 262 478.9/525

3 (APL+Edge) Γ
NH( × 1022 cm-2)  <0.74  <0.35

Eedge (keV)
τ
C-stat/d.o.f. 120.2/168 246.00 264 482.8/528

4 (WARM(APL)) Γ
NH( × 1022 cm-2)  <1.03  <3.63  <0.95

z 1.50 ± 0.15 1.87 ± 0.14 0.94 ± 0.07 2.15 ± 0.10
NH( × 1022 cm-2)  >55.8  >28.7
log(ξ) (erg cm s-1)  >3.24  >3.25  >3.38
C-stat/d.o.f. 118.3/167 247.6 262 482.7/527

Notes. Model APL is a power law with Galactic absorption and intrinsic absorption (XSPEC model wabs*zwabs*pow); model APL+Gauss is an absorbed power law plus Gaussian absorption lines (XSPEC model wabs*zwabs(pow+zgauss)); APL+Edge is an absorbed power law plus absorption edges (XSPEC model wabs*zwabs*zedge*pow); model WARM(APL) is an absorbed power law modified by an intrinsic ionized absorbers (XSPEC model wabs*zwabs*warmabs*pow). All energies are given in the rest frame. Errors are given at 90% confidence level (ΔC = 2.706 for one parameter of interest, Avni 1976).

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