\begin{table}%t3
\caption{\label{sandint3}Observational vs. modeled line strengths.}
%\centering
\par
\begin{tabular}{llr@{\hspace{5pt}}lrrc}
\hline\hline \noalign{\smallskip}
ID     & $\lambda_0$ [\AA] & \multicolumn{2}{c}{Observed}  & \multicolumn{2}{c}{Model} & Ratio\\[1.5pt]
       &                   &              & & dyn & \multicolumn{1}{c}{eq} & eq/dyn\\[1.5pt]
\hline
\noalign{\smallskip}
 \ion{N}{v}	 & 1238+1242  &     426\tablefootmark{a}  & (40)    & 330 &  697 & 2.11\\
 \ion{N}{iv}]	 & 1486       &      87\tablefootmark{a}  & (30)    & 124 &  276 & 2.23\\ 
 \ion{C}{iv}	 & 1548+1550  &     660\tablefootmark{a}  & (50)    & 668 & 1319 & 1.97\\
 \ion{C}{iii}]   & 1906+1909  &      55\tablefootmark{a}  & (30)    &  31 &   64 & 2.06\\ 
 \ion{O}{iv}]	 & 1402+1405  & ${<}37$\tablefootmark{a}  &	    &	6 &   13 & 2.17\\
{}[\ion{O}{iii}]   & 5007       &     3.5\tablefootmark{b}  & (0.4)   & 3.3 &  4.4 & 1.33\\
{}[\ion{O}{iv}]	 & 26~$\mu$m &      --  	     &         &  26 &   30 & 1.15\\ 
{}[\ion{Ne}{iv}]   & 2422+2425  &      25\tablefootmark{a}  & (12)    &  38 &   62 & 1.63\\
{}[\ion{Ne}{v}]	 & 3426       &      86\tablefootmark{a}  & (9)     &  78 &  119 & 1.52\\
{}[\ion{Ne}{iii}]  & 3869       &  ${<}1$\tablefootmark{b}  &	    & 0.4 &  0.5 & 1.25\\
{}[\ion{Ne}{v}]	 & 14~$\mu$m &      --  	     &         &  90 &  102 & 1.13\\ 
\ion{He}{ii}     & 4686       &      82\tablefootmark{b}  & (1)     &  82 &   80 & 0.98\\
\hline
\end{tabular}
\tablefoot {All values are specified in units of $\hb$~$=$ $100$. Columns~1 and~2 give the emission line names and the rest wavelength~$\lambda_0$. Measured values of~{\obj} are given in Col.~3, with errors in parentheses. Corresponding values of dynamic~(dyn) and equilibrium~(eq) models, and their ratio, are given in Cols.~4$-$6 (cf.~Sect.~\ref{sec:discabundances}). \\
\tablefoottext{a}{Jacoby (priv.~comm.);}
\tablefoottext{b}{this~paper.}}
\end{table}