\begin{table}%T3
\caption{\label{tab:HST-int2}Observed HST UV line fluxes, relative to He II 1640.}  
\small 
%%\centering

\par
\begin{tabular}{lccc}       
\hline\hline \noalign{\smallskip}
 Ion lambda  &  Bright lobe  &  Faint lobe  &  Combined  \\
\hline \noalign{\smallskip}
   He~{\sc{ii}}~$\lambda$1640~\AA   &   1.56$^a$  &   1.15$^a$    &  (2.7 +/$-$ 0.3)\tablefootmark{a,b} \\
   N~{\sc{v}}~$\lambda$1240~\AA     &   0.31  &       0.51      &       0.47 +/$-$ 0.04 \\
   O~{\sc{iv}}~$\lambda$1402~\AA       &  $<$0.06 &        --     &     $< 0.06$   \\
   N~{\sc{iv}}]~$\lambda$1488~\AA      & 0.17       &  noisy       &    0.12 +/$-$ 0.05 \\
   C~{\sc{iv}}~$\lambda$1550~\AA      &  1.10       &  1.33      &       1.28 +/$-$ 0.10 \\
%\hline 
   N~{\sc{iii}}]~$\lambda$1750~\AA &   $<$0.1       &           &           $<$0.1 \\
   C~{\sc{iii}}]~$\lambda$1909~\AA   &  $<$0.1       &           &            $<$0.1 \\
\par
\hline                            
\end{tabular}
\tablefoot{\tablefoottext{a}{The flux of  He~{\sc{ii}}~$\lambda$1640 is in units of 10$^{-14}$ \ergcmsq;} 
\tablefoottext{b}{all the flux in  He~{\sc{ii}}~$\lambda$1640, including both lobes.}  }
\end{table}