\begin{table}%t5
\caption{Rest wavelengths and intrinsic luminosity (in units of $10^{41}$~erg~s$^{-1}$) of the lines in the LETGS (as reported in Table~\ref{t:gaussian}) compared with the X-ray line luminosities 
as predicted by the LOC~model (last column) are listed. Note that the observed X-ray line luminosities were not used in the LOC~fitting, which was based on UV~data only. Here the triplets location has been identified with the wavelength of the forbidden line.}\label{t:x_cloudy} 
\small%\centerline
{
\begin{tabular}{lllll}
\hline\hline
&  Ion  & Wavelength  & Lum$_{\rm obs}$ & Lum$_{\rm LOC}$		\\
&    & (\AA)  & (10$^{41}$ erg s$^{-1})$ & (10$^{41}$ erg s$^{-1})$		\\
\hline
&\cv$^1$ 	& 41.47		& $<$$3$	    	    & 0.3		\\
&\cvi\					&33.73		&$1.1\pm0.5$	    & 0.6		\\
&\nvi$^1$					&28.78		&$<$$1.1$	    	    & 0.2		\\
&\nvii\					&24.78		&$<$$1.7$	    	    & 0.3		\\
&\ovii$^1$	&$22.09$	&$5.0\pm0.8$	    & 4.8		\\
&\oviii$^2$   	&$18.96$	&$2.4\pm1.0$	    & 1.0		\\
&\neix$^1$	& 13.44		&$<$$2.5$	    	    & 0.8		\\
&\nex\ 					& $12.13$	&$\dots$    	    & 0.1		\\
\hline
\end{tabular}}
\medskip
$^1$ Triplets; $^2$ blended with the \ovii\ He$\beta$.
\end{table}