\begin{table}%t3
\caption{\label{TabISOflx}Far-infrared line fluxes from the ISO~LWS observations of Cas~A.}
%\centerline
 {\small \begin{tabular}{llllllll}
\hline\hline
Line           &   \#1 &   \#2 & \#3 &   \#4 &   \#5 &   \#6 & \#7 \\
\hline
\multicolumn{8}{c}{FIR line fluxes $F$, $10^{-11}$~erg/cm$^2$/s \large\strut}\\
{}[\ion{O}{iii}] 52~$\mu$m & 5.4 &   9.3 & 5.4 &$<$1.2 &   3.5 &   5.0 & 5.2 \\
{}[\ion{O}{i}] 63~$\mu$m   &$<$0.6&  2.6 & 1.2 &$<$1.2 &   1.0 &   1.0 & 0.9 \\
{}[\ion{O}{iii}] 88~$\mu$m & 7.5 &   4.2 & 2.7 &   0.5 &   1.9 &   3.2 & 3.4 \\
{}[\ion{O}{i}] 145~$\mu$m  &$<$0.1& $<$0.09&0.3 & 0.1   &$<$0.1 &$<$0.1 &$<$0.1 \\
\hline
\multicolumn{8}{c}{[\ion{O}{iii}] 4959 + 5007~\AA\ line flux $F$, $10^{-13}$~erg/cm$^2$/s   \large\strut}\\
&$<$0.1 & 25    & 2.0 &$<$0.1& 6.5   & 0.5   & 2.9\\
\hline
\end{tabular}}
\medskip
Fluxes from the matched regions in the HST~ACS $F475W$ filter are also given. The upper limits are at the 3$\sigma$ level.\\
Note: ISO region positions are shown in Fig.~\ref{FigISOobs}.
Regions~\#3, \#6 and \#7 have higher interstellar absorption column
\citep{BiegingOH}.
\end{table}