\begin{table}%T6
\par
\caption{\label{tab:shock_H2_fluxes_3C326}MHD shock model parameters and predicted H$_2$ line fluxes\tablefootmark{a} for 3C~326.}
\small%\centering
\par
\begin{tabular}{c c c c c c c c c c c c}
\hline\hline\noalign{\smallskip}
$n_{\rm H}$\tablefootmark{b}  &  $V_{\rm s}$\tablefootmark{c}  &  
\multicolumn{8}{c}{{H$_2$ line fluxes} [$10^{-18}$ W~m$^{-2}$]} & 
 \multirow{2}*{$\cal{F}_{\rm H_2}$\tablefootmark{d}} &
  \multirow{2}*{$\cal{F}_{\rm bol}$\tablefootmark{e}} \\
\cline{3-10}
$[$cm$^{-3}$]  & $\rm [km~s^{-1}]$   & S(0) & S(1) & S(2) & S(3) & S(4) & S(5) & S(6) & S(7) & & \\
\hline
\multirow{4}*{$10^4$} & 4   &  0.74 & 4.51 & 0.18 & $6.1  \times  10^{-3}$ & $3  \times  10^{-4}$ & $8.6  \times  10^{-4}$ &$2.9  \times  10^{-4}$ &$7.5  \times  10^{-4}$ & 5.43 & 13.02    \\
& 15 & 0.09 &  3.22 &  3.19 &  10.36 &   1.35 &   0.68 &  0.02 & $2.2  \times  10^{-3}$ & 18.92& 20.55 \\
& 34 &  $4.2  \times  10^{-3}$ &  0.19 &  0.29 &   2.32 &   1.38 &   5.33 &   1.58 &  2.99 & 14.09 & 16.35  \\
%\cline{2-12}
& Sum &  0.84 &  7.92 &   3.66 &  12.69 &  2.73 &  6.01 &  1.60 &   2.99 &  38.44 & 49.92   \\
\hline
\multirow{4}*{$10^3$} & 4 & 1.61 & 3.74 &  0.018 &  $1.3  \times  10^{-3}$ & $4.3  \times  10^{-4}$ & $1.2  \times  10^{-3}$ & $4  \times  10^{-4}$ & $10^{-3}$ & 5.37 & 10.6 \\
& 24 &  0.08 &  3.01 & 2.44 & 5.09 & 0.46 & 0.17 & $7  \times  10^{-3}$ & $6.6   \times  10^{-3}$ & 11.3 & 11.6 \\
& 40 & 0.02 & 1.01 & 1.32 & 7.57 & 2.73 & 5.24 & 0.68 &  0.56 & 19.13 & 20.07 \\
%\cline{2-12}
& Sum & 1.71 & 7.75 &  3.78 & 12.66 &   3.2 &  5.42 &  0.68 &  0.56 &  35.77 & 42.27\\
%\hline
\multicolumn{2}{c}{\textit{Spitzer} Obs.} & $2.0 \pm  0.3$ & $7.5  \pm   0.5$ & $4.1  \pm   0.4$ & $12.6  \pm   0.4$ & $3.1  \pm   0.6$ & $5.0  \pm 2.5$ & $2.5 \pm 1.0$ & $2.9  \pm   1.0$ & $39.7  \pm   2.3$  &  \\
\hline
\end{tabular}
\tablefoot{\tablefoottext{a}{This table lists the shock model velocities, the predicted H$_2$ rotational line fluxes, and bolometric luminosities associated with each shock velocity components. Measured H$_2$ fluxes are taken from \citet{ogle07,ogle09}.} \tablefoottext{b}{Preshock hydrogen density.} \tablefoottext{c}{MHD shock velocity.} \tablefoottext{d}{Sum of the $\rm H_2$ S(0) to S(7) rotational lines in $10^{-18}$~W~m$^{-2}$.} \tablefoottext{e}{Sum over all the lines (bolometric luminosity of the shock).}} \vspace*{3mm}
\end{table}