\begin{table}%t9
\caption{Flux of the broad emission lines, from the simultaneous LETGS, MEG and HEG~fit. The wavelength was frozen to the rest wavelength of the line, while the {\it FWHM} was frozen to 8000~km~s$^{-1}$. The lines for which upper limits are detected were not used in the further analysis of the data.}\label{tab:bel}
%\centerline
{
\begin{tabular}{llll}
\hline  \hline
Ion                           & $\lambda$  & Flux                  & {\it EW}   \\
                              & (\AA)      & (ph~m$^{-2}$~s$^{-1}$) & (m\AA) \\
	          \hline
\ion{C}{v} f$^{a}$ & 41.421  & 1.0 $\pm$ 0.6   & 300 $\pm$ 180 \\
\ion{C}{v} 1s$^2$--1s2p $^1$P$_1$          & 40.268  & $<$0.6         & $<$230      \\
\ion{C}{vi} 1s--2p (Ly$\alpha$)            & 33.736  & 0.5 $\pm$ 0.2   & 150 $\pm$ 80  \\
\ion{N}{vii} 1s--2p (Ly$\alpha$)           & 24.781  & $<$0.05        & $<$70       \\
\ion{O}{vii} triplet$^{b}$                & 21.602  & 0.56 $\pm$ 0.13  & 130 $\pm$ 40  \\
\ion{O}{viii} 1s--2p (Ly$\alpha$)          & 18.969  & 0.4 $\pm$ 0.2   & 60 $\pm$ 30   \\
\ion{O}{vii} 1s$^2$--1s3p $^1$P$_1$        & 18.627  & 0.19 $\pm$ 0.07  & 70 $\pm$ 30   \\
\hline
\end{tabular}}
\medskip
$^{a}$ This coincides with the instrumental C-edge, therefore its detection is less certain due to possible calibration uncertainties.\\
$^{b}$ The resonance intercombination and forbidden lines significantly overlap, so separate measurements are difficult. \\
\end{table}