Table 2: The main parameters of the spectral model for the average XMM-Newton spectra from 2005 and 2006. The numbers in brackets are the errors and have to be multiplied by the same power of ten as to that for the parameters. ``n.h.p.'' is the ``null hypothesis probability''.
    2005 2006

wabs
nH [1022 cm-2] 4.1E-02 (0.8) 4.7E-02 (0.6)
pcfabs nH [1022 cm-2] 7.9 (0.6) 9.5 (0.5)
  CvrFract 0.61 (0.02) 0.67 (0.01)
mekal kT [keV] 79.9 [35]1 79.9 [35]1
  norm 7.3E-03 (0.4) 6.5E-03 (0.3)
bbody kT [keV] 5.9E-02 (0.07) 5.4E-02 (0.05)
  norm 1.9E-04 (0.9) 2.2E-04 (0.9)
Gaussian LineE [keV] 6.4 (- 2) 6.4 (- 2)
  Sigma [keV] 0.1 (- 2) 0.07 (0.02)
  norm 3.1E-05 (0.7) 2.9E-05 (0.6)
Gaussian LineE [keV] 6.7 (- 2) 6.7 (- 2)
  Sigma [keV] 0.1 (- 2) 0.09 (0.03)
  norm 3.1E-05 (0.7) 2.5E-05 (0.7)
$\chi^{2}_{\nu}$ (d.o.f)   1.034659 (948) 1.046327 (1754)
n.h.p.   2.2E-01 8.7E-02
1 The temperature of the mekal component ran against its upper limit. The value in brackets is the plasma temperature which is compliant with both the XMM and INTEGRAL spectrum (see Fig. 5 and Chap. 3). 2 The parameters were fixed to these values.

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