\begin{table}%t3
%\centering
\par
\caption{XMM-{\em Newton} EPIC--PN spectral fitting results using the 
photoionized gas model described in the text. Fluxes are given in units of 
$10^{-13}$~erg~cm$^{-2}$ s$^{-1}$, luminosities in units of 
$10^{43}$~erg~s$^{-1}$; both are corrected for absorption. 
$^*$ denotes a fixed parameter.}
\label{refl}
\begin{tabular}{lll}
\par
\hline\hline 
\par
&  {1 APEC} &  {2 APEC} \\
\hline
\par
 {\bf Apec(1)} & & \\ 
$kT$ [keV] & $\rm 0.66^{+0.07}_{-0.04}$ & $\rm 0.76^{+0.08}_{-0.07}$ \\
$f~_{0.3 - 10\: {\rm keV}}$ & $0.62\pm0.07$ & $0.52\pm0.11$ \\   
\hline
\par
 {\bf Apec(2)} & & \\
$kT$ [keV] & -- & $\rm 0.26^{+0.08}_{-0.03}$ \\   
$f~_{0.3 - 10\: {\rm keV}}$ & -- & $\rm 0.23^{+0.11}_{-0.10}$ \\   
\hline
\par
\bf{Power-law(1)} & & \\
$N_{\rm H}$ [$10^{22}$~cm$^{-2}$] & $\rm 68^{+17}_{-15}$ & $\rm 65^{+15}_{-12}$ \\
$\Gamma$ & $1.9^*$ & $1.9^*$ \\  
$f~_{0.3 - 10 \:{\rm keV}}$ & $\rm 41_{-12}^{+21}$ & $\rm 39_{-11}^{+20}$ \\ 
\hline
\par
\bf{Power-law(2)} & & \\
$N{\rm H}$ [$10^{20}$~cm$^{-2}$] & $7^*$ & $7^*$ \\
$\Gamma$ & $1.9^*$ & $1.9^*$ \\  
$f~_{0.3 - 10 \:{\rm keV}}$ & $1.7\pm0.2$ & $1.5\pm0.2$ \\ 
\hline
\par
\bf{Fe K$\alpha$} & & \\
$E$ [keV] & $6.4^*$ & $6.4^*$ \\
$EW$ [eV] & $\rm 186_{-125}^{+165}$ & $\rm 185_{-122}^{+159}$ \\     
$f~_{0.3 - 10\: {\rm keV}}$ & $\rm 0.50^{+0.44}_{-0.34}$ & $\rm 0.47^{+0.40}_{-0.31}$ \\   
\hline
\par
\bf{Fe XXV} & & \\
$E$ [keV] & $6.7^*$ & $6.7^*$ \\
$EW$ [eV] & $\rm 121_{-102}^{+110}$ & $\rm 124_{-103}^{+110}$ \\     
$f~_{0.3 - 10\: {\rm keV}}$ & $\rm 0.34^{+0.31}_{-0.29}$ & $\rm 0.33^{+0.29}_{-0.27}$ \\   
\hline
\par
\bf{Total} & & \\
$f~_{0.3 - 10\: {\rm keV}}$ & 44.5 & 42.1 \\   
$L~_{0.3 - 10\: {\rm keV}}$ & 1.47 & 1.39 \\ 
\hline\noalign{\smallskip}
$\chi^2/$d.o.f. & 84.9/80 & 64.0/78 \\   
\hline
\end{tabular}
\end{table}