\begin{table}%t2
 %\centering
\par
        \caption{Parameters from the Compton emission (CE) model fit to the spectra of \EPIC\ and \ISGRI\ combined. 
	Also listed are the values of the CE model (without
	a blackbody) fit to the pulse and plateau states of the phase-resolved \PN\ spectra
	constrained with the \ISGRI\ spectrum. The integrated fluxes are listed as observed ($F_{2-10}$) or unabsorbed
	($F^{{\rm UA}}_{2-10}$). Errors denote 90\% confidence.}
   \label{tab_spec}
        \begin{tabular}{lcccl}  \hline\hline
               	Parameter & CE & Pulse & Plateau & Unit \\
               	\hline
                       $C_{I}$ & 0.8~$\pm$~0.2 & 0.6~$\pm$~0.2 & 1.3~$\pm$~0.7 &  \\
	$\tau$ & 9~$\pm$~1 & $\rm 12^{+6}_{-2}$ & $\rm 8^{+4}_{-2}$ &  \\
        $kT_{{\rm e}}$ & 4.4~$\pm$~0.3 & 4.4~$\pm$~0.3 & 4.4~$\pm$~0.4 & keV  \\
        $N_{{\rm H}}$ & 25~$\pm$~2 & $\rm 23^{+2}_{-6}$ & $\rm 24^{+3}_{-7}$ & 10$^{22}$~cm$^{-2}$  \\
	${Z}_{{\rm Fe}}$ & $\rm 1.0^{+0.4}_{-0.2}$ & $\rm 0.9^{+0.6}_{-0.3}$ & $\rm 1.2^{+0.8}_{-0.6}$ & ${Z}_{\odot}$  \\
	$F_{2-10}$ & 4.4 & 5.2 & 3.0 & 10$^{-11}$~erg~cm$^{-2}$~s$^{-1}$  \\
	$F^{{\rm UA}}_{2-10}$ & 9.2 & 9.8 & 6.7 & 10$^{-11}$~erg~cm$^{-2}$~s$^{-1}$  \\
	$E_{\rm K\alpha}$ & 6.41~$\pm$~0.03 & 6.44~$\pm$~0.03 & 6.41~$\pm$~0.04 & keV  \\
	$F_{\rm K\alpha}$ & 1.1~$\pm$~0.2 & 1.1~$\pm$~0.4 & 0.8~$\pm$~0.4 & 10$^{-4}$~ph~cm$^{-2}$~s$^{-1}$  \\
	$E_{\rm K\beta}$ & 7.1~$\pm$~0.1 & 7.1~$\pm$~0.3 & 7.2~$\pm$~0.3 & keV  \\
	$F_{\rm K\beta}$ & $<$0.62 & $<$1.1 & $<$1.3 & 10$^{-4}$~ph~cm$^{-2}$~s$^{-1}$  \\
	$\chi_{\nu}^{2}/$d.o.f. & 0.95/676 & 0.92/140 & 0.92/94 &  \\
	                \hline
        \end{tabular}
\end{table}