\begin{table}%t2
\par
\caption{\label{tab:temp}SED templates used as models.}
\small%\centering
\par
\begin{tabular}{lll}
\hline\hline\noalign{\smallskip}
Label  & Source & Description \\
\hline\noalign{\smallskip}
AGN1   & ...                &   local quasar's mean SED$^1$\\
AGN1-L & ...                &   luminosity-dependent quasar's SED$^2$ \\
AGN3   & NGC~5506           & Sy2, $N_{\rm H}=3\times10^{22}~{\rm cm^{-2}}$ \\
AGN4   & NGC~4507           & Sy2, $N_{\rm H}=4\times10^{23}~{\rm cm^{-2}}$ \\
AGN5   & Mnk~3              & Sy2, $N_{\rm H}=1.4\times10^{24}~{\rm cm^{-2}}$ \\
AGN6   & NGC~3393           & Sy2, $N_{\rm H}>1\times10^{25}~{\rm cm^{-2}}$ \\
SB1    & NGC~5253           & Young and dusty SB\\
SB2    & NGC~7714           & Young and unobscured SB\\
SB3    & M82                & Old SB~\\
SB4    & IRAS~12112+0305    & ULIRG \\
CP1    & NGC1068            &  Composite template: AGN: $\sim$$50\%$ \\
CP2    & Mnk~231            &  Composite template: AGN: $\sim$$70\%$ \\
CP3    & IRAS~19254-7245    &  Composite template: AGN: $\sim$$45\%$ \\
CP4    & IRAS~22491-1808    &  Composite template: AGN: $\sim$$70\%$ \\
 \hline 
\end{tabular}
\tablebib{(1) \citealt{Richards06}; (2) \citealt{Hopkins07}.}
\end{table}