\begin{table}%t7
\caption{\label{t:refl} Alternative fit of the continuum, including reflection.}
%\centerline
{\begin{tabular}{lll}
\hline\hline
\noalign{\smallskip}
$T_{\rm mbb}$ & keV &  $0.21\pm0.3$\\
$\Gamma$ & &  $2.5\pm0.1$\\
blurred &&\\
$norm_{\rm pow}$ & $10^{51}$~ph~s$^{-1}$~keV$^{-1}$& $4.1\pm0.3$\\
$\Gamma$ &  & $1.73\pm0.08$\\
%$L_{pow}$ & $\dots$ & 
$\alpha$ & & $>$1.7\\
$i$ & deg &  $<$30\\
$s$&& $0.8\pm0.3$\\
%$q$&& $\dots$ &MANCA\\
unblurred&&\\
$norm_{\rm pow}$ & $10^{51}$~ph~s$^{-1}$~keV$^{-1}$&  $8.0\pm2.5$\\
$\Gamma$ &&  $1.73\pm0.08$\\
$i$ & deg &  60 fixed\\
$s$&&  $\rm 1.1^{+1.3}_{-0.2}$\\
$\chi^2/\nu$ & & 322/230\\
\hline
\end{tabular}}
\par
\tablefoot{The model includes a black body, a power law, blurred 
reflection from the accretion disk and reflection from unblurred cold and distant material.  
The value of $\chi^2_{\rm red}$ refers to full modeling, including absorption (Sect.~\ref{par:abs})
and emission lines (Sect.~\ref{par:broad}).}\vspace*{-2mm}
\end{table}