\begin{table}%T4
\caption{\label{table5}Ratio ($I_{\lambda}$/\Hb)$_{\rm calc}$/($I_{\lambda}$/\Hb)$_{\rm obs}^1$
for the UV lines.}
%\centerline
{
\begin{tabular}{lc} \hline \hline 
\     line    &  M1\\
\hline 
 Ly$\alpha$ & 1.0\\  
 \ion{N}{v} 1214&0.33 \\
 \ion{O}{iv}\rbrack+\ion{Si}{iv} $\lambda$1400& 1.27\\
 \ion{N}{iv}\rbrack~$\lambda$1486& 0.50\\
 \ion{C}{iv} $\lambda$1550& 1.23\\
 \ion{He}{ii} $\lambda$1640&  4.7\\
 \ion{O}{iii}\rbrack~$\lambda$1663&0.66\\
 \ion{N}{iii}\rbrack~$\lambda$1750&0.22 \\
 \ion{Si}{iii}\rbrack~$\lambda$1890&1.60 \\
 \ion{C}{iii}\rbrack~$\lambda$1909&1.19\\
 \lbrack\ion{Ne}{iv}\rbrack~$\lambda$2423&1.36\\
 \ion{Mg}{ii} $\lambda$2800 & 0.20\\
\hline 
\end{tabular}}
\smallskip
$^1$ From Crenshaw et~al. (\cite{cren02}, Table 2, reddening corrected).
\end{table}