\begin{table}%t1
\caption{\label{tab1}The sources and their core luminosities in the radio,
$L_{\nu {\rm r}}$ ($\times 10^{23}$~W~Hz$^{-1}$), and 
IR/optical/UV bands, $L_{\nu {\rm IR}}$, $L_{\nu {\rm o}}$ and $L_{\nu 
{\rm UV}}$
($\times 10^{19}$  W Hz$^{-1}$).}
%\centerline
{
\begin{tabular}{cccccccc}
\hline\hline\noalign{\smallskip}
Source   & Alt. name & $z$ & Envir. & $L^{a}_{\nu {\rm r}}$ &  $L_{\nu {\rm IR}}$ &
 $L^{e}_{\nu {\rm o}}$ & $L_{\nu {\rm UV}}$  \\
\noalign{\smallskip}\hline  \noalign{\smallskip}
3C~~29     &          & 0.0438 &  A 119  &  3.5  &                & 4.1             &    $^*$                     \\
3C~~31     &  NGC 383 & 0.0169 & Arp 331 &  0.51 &                & 1.6             &                             \\
3C~66B     &          & 0.0215 &         &  1.6  &                & 8.8             & 3.5$^{h}$,  2.5$^{i}$, 1.35$^{m}$  \\
3C~~78     & NGC 1218 & 0.0288 &         &  15   &                & 96, 85$^{f}$&  27.5$^{m}$           \\
3C~83.1    & NGC 1265 & 0.0251 & Perseus &  0.26 &                & 0.42            &                           \\
3C~~189    & NGC 2484 & 0.0413 &         &  6.5  &                & 25$^{g}$    &             \\     
3C~272.1   &   M 84   & 0.0037 & Virgo   & 0.047 & 1.0$^{b}$, 0.95$^{c}$, 1.1$^{d}$ & 0.37$^{g}$, 0.13$^{f}$ & \\
3C~277.3   &          & 0.0857 & Coma A  &  1.8  &                & 3.7,  5.4$^{f}$   &                   \\
3C~288     &          & 0.246  &         &  39   &                & 15.1            &                          \\
3C~296     & NGC 5532 & 0.0237 &         &  0.84 &                & 0.65           &                    \\
3C~310     &          & 0.0535 &         &  4.5  &                & 3.6            &                   \\
3C~317     &          & 0.0342 & A 2052  &  8.9  &  27$^{b}$  & 5.1$^{g}$, 3.8$^{f}$ & 0.22$^{m}$        \\
3C~338     & NGC 6166 & 0.0303 & A 2199  &  1.9  & 2.6$^{b}$  & 3.0            &  0.14$^{m}$      \\
3C~346     &          & 0.162  &         & 120   &                & 241            & 29$^{l}$   \\
3C~348     &          & 0.154  & Her A   &  4.9  &                & 8.1            &               \\
3C~442     & NGC 7237 & 0.0262 & Arp 169 & 0.027 &                & 0.23,  0.13$^{f}$  &           \\    
3C~449     &          & 0.0171 &         &  0.21 &                & 2.5            &    $^*$          \\
\hline
\end{tabular} }
\smallskip
$^{a}$ 5 GHz;
$^{b}$ 16~000~\AA;
$^{c}$ 11~000~\AA;
$^{d}$ 20~500~\AA;
$^{e}$ 7020~\AA;
$^{f}$ 5500~\AA;
$^{g}$ 8140~\AA;
$^{h}$ 4440~\AA;
$^{i}$ 3400~\AA;
$^{l}$ 1400~\AA; 
$^{m}$ 2500~\AA;
$^*$ we did not use the HST data in the UV band for 3C~29 and 3C~449 
since the nuclear emission of these sources is clearly affected by 
obscuration from extended (kpc--scale) dusty structures 
(Chiaberge et~al. \cite{Chiaberge2002}).
\end{table}