\begin{table}%T3
\par
\caption{\label{tab:irsline}{Tentative} \textit{Spitzer} IRS line fluxes {derived from the SH and LH~spectra}.}
\small%\centering
\par
\begin{tabular}{lcrrr}
\hline\hline\noalign{\smallskip}
Line 		& $\lambda$ (\mic) & \multicolumn{3}{c}{Flux ($10^{-18}$~W~m$^{-2}$)}\\
{}						&					& Feb. 2005 & Mar. 2005 & Nov. 2008\\
\hline
 H$_2$ $0{-}0$ $S(2)$						&	12.2786	& 			& 	&	$7.8 \pm 0.8$ \\
{}[\ion{Ne}{ii}]	$^2P_{1/2}$--$^2P_{3/2}$ 		&	12.8136	& $41.1 \pm 0.7$	& $39.7 \pm 1.1$	&	$42.7 \pm 0.9$ \\
{}[\ion{S}{iii}] $^3P_2$ -- $^3P_1$			&	18.7130	& $46.5 \pm 1.4$	& $42.5 \pm 1.5$	&	$34.6 \pm 1.2$ \\
H$_2$ $0{-}0$ $S(0)$						&	28.2188	& $15.2 \pm 2.2$	& $18.9 \pm 3.4$	&	$9.5 \pm 1.6$ \\
{}[\ion{S}{iii}] $^3P_1$ -- $^3P_0$				&	33.4810	& $463.3 \pm 9.6$	& $374.4 \pm 7.9$	&	$183.4 \pm 4.7$\\
\hline
\end{tabular} 
\end{table}