\begin{table}%t2
\caption{\label{tab1}Multiwavelength properties of the core galaxies.}
\par
%\centerline
{
\begin{tabular}{c| c c c c }
\hline\hline
Name& $L_{\rm o}$& $P_{\rm core}$& $L_{1.4~{\rm GHz}}$ & $L_{\rm [O~III]}$ \\
\hline	                              
UGC~5902  &$<$39.10& 35.83&    35.81   &    37.96  \\
UGC~7203  & 39.85  & 37.45&    36.98   &    38.08  \\
UGC~7629  & 38.79  & 36.74&    37.93   &    37.40  \\
UGC~7760  & 38.73  & 37.44&    36.78   &    37.28  \\
UGC~7898  &$<$39.13& 37.27&    37.10   & $<$37.34  \\
UGC~8745  &  $-$   & 37.66&    38.00   &    38.41  \\
UGC~9655  &  $-$   & 36.72&    37.27   & $<$38.04  \\
\hline	 	   		            
UGC~0968  &$<$39.77& 36.96&    36.74   & $<$37.75  \\
UGC~6297  &$<$39.06& 36.46&    36.34   &    38.21  \\
UGC~7386  & 38.76  & 38.01&    37.86   &    38.95  \\
UGC~7797  &$<$40.19& 38.04&    37.76   &    38.79  \\
UGC~7878  & 39.07  & 36.75&    37.38   &    37.89  \\   
UGC~9706  & 39.25  & 37.59&    37.33   &    38.18  \\ 
UGC~9723  & $-$    & 37.07&    36.77   &    37.33  \\            
\hline
\end{tabular}}
\par
\medskip 
Column description: (1) name; (2) optical nuclear luminosity [erg
  s$^{-1}$] from \citet{balmaverde06b}; (3) radio core power [erg s$^{-1}$] at
  5~GHz and (4) total radio luminosity at 1.4 GHz [erg s$^{-1}$] estimated from
the fluxes given in Tab.~\ref{tab1}; (5) [O~III] emission line luminosity
[erg~s$^{-1}$]. \vspace*{-2.5mm}
\end{table}