\begin{table}%t6
\caption{\label{model.abs}PHASE and continuum parameter values for models $\mathcal{B}$ and
  $\mathcal{C}$ for the simultaneous fits to the EPIC and RGS spectra.}  
%\centerline
{\small
\par
\begin{tabular}{@{}l ll @{}l ll @{}l llr @{}l llr l@{}}
\hline\hline
  & \multicolumn{2}{c}{Powerlaw}     
&&  \multicolumn{2}{c}{Black body}             
&& \multicolumn{3}{c}{LIC}         
&& \multicolumn{3}{c}{HIC}   
& \multicolumn{1}{c}{$\chi^{2}_{\nu}$/d.o.f.}   \\
\cline{2-3} \cline{5-6} \cline{8-10} \cline{12-14}
& \multicolumn{1}{c}{$\Gamma$} & \multicolumn{1}{c}{$K_{\rm pwlw}$} 
&&  \multicolumn{1}{c}{$kT$} & \multicolumn{1}{c}{$K_{\rm bb}$} 
&& log~$U$ & log~$N_{\rm H}$ & \multicolumn{1}{c}{vel.}\ 
&& log~$U$ & log~$N_{\rm H}$ & \multicolumn{1}{c}{vel.} &\\
\noalign{\smallskip}
\hline	
model $\mathcal{B}$ & $\rm 1.67_{-0.02}^{+0.03}$ & $\rm 8.3_{-0.2}^{+0.3}$ 
&& $0.097_{\rm -0.003}^{+0.003}$     & $\rm 3.4_{-0.2}^{+0.2}$ 
&& $\rm 1.7_{-0.1}^{+0.4}$ & $\rm 21.0_{-0.2}^{+0.2}$    &  $\rm -300_{-300}^{+300}$ 
&&&&
&0.97/719 \\[3pt]			       
model $\mathcal{C}$ & $1.72_{\rm -0.01}^{+0.03}$ & $\rm 8.9_{-0.3}^{+0.3}$ 
&& $\rm 0.100_{-0.003}^{+0.003}$     & $\rm 3.4_{-0.3}^{+0.2}$ 
&&  $\rm 1.65_{-0.08}^{+0.07}$ & $\rm 21.2_{-0.2}^{+0.2}$    & $\rm 500_{-300}^{+300}$ 
&& $\rm 2.6_{-0.1}^{+0.1}$ & $\rm 21.51_{-0.01}^{+0.01}$ & $\rm 500_{-300}^{+300}$ 
& 0.90/706 \\
\hline 
\end{tabular}}
\smallskip
\par
Model $\mathcal{B}$ is similar to model $\mathcal{A}$ with one absorbing
  component and model $\mathcal{C}$ to model $\mathcal{B}$ with another
  absorbing component and a few Gaussian emission lines (see their parameters
  in Table~\ref{model.lines}). Both $\mathcal{B}$
  and $\mathcal{C}$ models include the Galactic absorption (with fixed 
  $N_{\rm H}=4.67\times 10^{20}$~cm$^{-2}$) and the Fe-K$\alpha$ line
  (with its parameters fixed to the model $\mathcal{A}$ values). 
  Normalizations $K_{\rm pwlw}$ and $K_{\rm bb}$ correspond to the \pn\
  spectrum. 
   $K_{\rm pwlw}$ in units of $10^{-4}$~ph~~keV$^{-1}$~cm$^{-2}$~s$^{-1}$; 
   $kT$ in keV; $K_{\rm bb}$ in
   $10^{-5}$~$L_{39}/D_{10}^{2}$ where $L_{39}$ is the source luminosity in
   units of $10^{39}$ erg~s$^{-1}$ and $D_{10}$ is the distance to the source
   in units of 10~kpc. $N_{\rm H}$ is given in cm$^{-2}$. Velocities, 
   given in \kms, are relative to the systemic velocity of \target.  
  Errors quoted are at 90{\%} confidence level.
\end{table}