\begin{table}%t3
\caption{\label{tab:luminosities}IR~and X-ray luminosities.}
\small%\centering
\par
\begin{tabular}{lcccccccc}
\hline\hline\noalign{\smallskip}
Source & $\log L_{\rm IR}^{\rm tot}$\tablefootmark{a} & $\log L_{\rm IR}^{\rm AGN}$\tablefootmark{a} & $\log L_{\rm IR}^{\rm SB}$\tablefootmark{a} &  $\log L_{\rm IR,RTM}^{\rm tot}$\tablefootmark{b} & $\log L_{\rm IR,RTM}^{\rm AGN}$\tablefootmark{b} & $\log L_{\rm IR,RTM}^{\rm SB}$\tablefootmark{b} & $\log L_{\rm X}^{\rm AGN}$\tablefootmark{c} & $N_{\rm H}$\tablefootmark{d} \\\noalign{\smallskip}
       & (erg s$^{-1}$)           & (erg s$^{-1}$)           & (erg s$^{-1}$)          &  (erg s$^{-1}$)               & (erg s$^{-1}$)               & (erg s$^{-1}$)              & (erg s$^{-1}$)        & (cm$^{-2}$) \\
\hline\noalign{\smallskip} 
\multicolumn{9}{l}{Class A HLIRG} \\
\noalign{\smallskip} 
PG~1206+459      & 48.0 & 48.0 & 0    & 47.8 & 47.8 & $<$$46.7$ & $\rm 45.11^{+0.02}_{-0.04}$ & ... \\
PG~1247+267      & 48.8 & 48.8 & 0    & 47.9 & 47.9 & $<$$46.8$ & $\rm 45.93^{+0.02}_{-0.03}$ & ... \\ 
IRAS~F12509+3122 & 47.6 & 46.8 & 47.5 & 47.0 & 46.8 & 46.6    & $\rm 42.26^{+0.05}_{-0.05}$ & ... \\ 
IRAS~14026+4341\tablefootmark{e}  & 46.5 & 45.8 & 46.5 & 46.5 & 46.3 & 46.1    & $\rm 42.7^{+0.2}_{-0.5}$    & ... \\
IRAS~F14218+3845 & 47.1 & 46.5 & 46.9 & 46.9 & 46.1 & 46.8    & $\rm 44.60^{+0.03}_{-0.03}$ & ... \\ 
IRAS~16347+7037  & 48.5 & 48.5 & 0    & 47.7 & 47.7 & $<$$46.8$ & $\rm 46.00^{+0.07}_{-0.09}$ & ... \\ 
IRAS~18216+6418  & 47.1 & 46.9 & 46.6 & 46.8 & 46.6 & 46.4    & $\rm 45.6^{+0.04}_{-0.05}$  & ... \\ 
\noalign{\smallskip} 
\multicolumn{9}{l}{Class B HLIRG} \\
\noalign{\smallskip} 
IRAS~F00235+1024 & 46.7 & 46.4 & 46.4 & 46.7 & 46.4    & 46.4    & $<$$42.2$ & $>$$10^{25}$\\ 
IRAS~07380-2342  & 47.0 & 46.7 & 46.7 & 47.0 & 46.8    & 46.5    & $<$$41.7$ & ... \\ 
IRAS~00182-7112  & 46.6 & 46.3 & 46.3 & 46.7 & $<$$46.5$ & 46.7    & $44.82^{+0.16}_{-0.14}$ & $>$$10^{25}$ \\ 
IRAS~09104+4109  & 47.3 & 47.1 & 46.8 & 46.8 & 46.8    & $<46.2$ & $\rm 45.30^{+0.36}_{-0.09}$ & $>$$10^{25}$ \\ 
IRAS~12514+1027  & 46.7 & 46.5 & 46.2 & 46.5 & 46.2    & 46.2    & $\rm 43.3^{+1.4}_{-0.7}$    & $(4^{+20}_{-3})\times10^{23}$ \\ 
IRAS~F15307+3252 & 47.9 & 47.6 & 47.6 & 46.9 & 46.6    & 46.7    & $\rm 45.49^{+0.09}_{-0.11}$ & $>$$10^{25}$ \\ 
\noalign{\smallskip} 
\hline
\end{tabular}
\tablefoot{\tablefoottext{a}{IR~luminosities (1$-$1000~$\mu{\rm m}$) estimated using our SED fitting.} \\
\tablefoottext{b}{IR~luminosities (1$-$1000~$\mu{\rm m}$) estimated by the analysis of the IR~SED using RTM \citep{Rowan00,Farrah02submm}.} \\
\tablefoottext{c}{Absorption corrected 2$-$10 keV luminosities from \citet{Ruiz07}.} \\
\tablefoottext{d}{Intrinsic absorption estimated using X-ray spectra \citep{Ruiz07}.} \\
\tablefoottext{e}{The X-ray luminosity of this source has been calculated from 2XMMi fluxes \citep{2xmmi}, and it is not corrected for absorption.}}
\end{table}