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Table 3:

Best fit parameters for the broand band ${\it Suzaku}$ (photoionization scenario) and XMM-Newton spectra.
  $\Gamma_{\rm s}$ $\Gamma_{\rm h}$ $N_{\rm H}$ R $E_{\rm line}$ EW $\chi^2_r$/d.o.f.
      (1023 cm-2)   (keV) (eV)  
${\it Suzaku}$ $1.71\pm0.12$ (= $\Gamma_{\rm s}$) $\rm 3.33^{+0.17}_{-0.15}$ $\rm 1.28^{+0.81}_{-0.56}$ $6.397\pm0.009$ $218\pm 24$ 1.16/219
XMM-Newton $2.49\pm0.23$ $\rm 1.62^{+0.11}_{-0.23}$ $\rm 1.76^{+0.13}_{-0.21}$ <2.1 $6.44\pm0.05$ $133\pm 63$ 1.21/70
Note: from left to right: the indices of the soft ( $\Gamma_{\rm s}$) and hard ( $\Gamma_{\rm h}$) power laws; the column density of the intrinsic absorber; the relative normalization of the Compton reflection component, R; the centroid energy, $E_{\rm line}$ and equivalent width (EW) of the iron line; the reduced $\chi^2$ and the d.o.f.

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