\begin{table}%T5
\caption{\label{tab:summary}Observed and bolometric luminosity of the line emission of molecular and ionized gas (H$\alpha$).}
\small
%\centering
\par
\begin{tabular}{lcccc}
\hline\hline\noalign{\smallskip}
                &  Molecular Gas & Ionized gas & Radio source\tablefootmark{a} & AGN X-ray\tablefootmark{b}\\
\hline
$\log{{\cal L}_{\rm obs}}$\tablefootmark{c}  & 41.9 & 41.3 & 44.6 & 40.6 \\
$\log{{\cal L}_{\rm bol}}$\tablefootmark{d}& 42.0 & 43   &      & \\ 
$\log{E_{\rm kinetic}}$\tablefootmark{e}   & 57.5 & 55.7 & 59.8 & \\
$\log{\rm Mass}$\tablefootmark{f}        & 9.5  & 7.3  &      & \\
$\log{\tau_{\rm diss}}$\tablefootmark{g}  & 8.2\tablefootmark{h}  & 7.2\tablefootmark{i}  &      & \\
\hline
\end{tabular}
\tablefoot{\tablefoottext{a}{Radio luminosity measured at 327 MHz.}  
\tablefoottext{b}{X-ray luminosity of the nuclear point source from \citet{ogle09}.} 
\tablefoottext{c}{erg s$^{-1}$.} 
\tablefoottext{d}{erg s$^{-1}$.} 
 \tablefoottext{e}{erg.} 
\tablefoottext{f}{$M_{\odot}$.} 
\tablefoottext{g}{yrs.} 
\tablefoottext{h}{For dissipation through the molecular gas.} 
\tablefoottext{i}{Assuming that all of the UV/optical line emission is due to dissipation of kinetic energy.}}
\end{table}