\begin{table*}
\caption{The sample of FR~II radiogalaxies}
\tiny
\begin{tabular}{l c c c c c| l c c c c c} \hline
%\begin{tabular}{l r r} \hline

Source Name    &  redshift & Class. & $S_t$ (178)   &  $\log L_r$             &  $\log L_{[OIII]}$ & Source Name    &  redshift & Class. & $S_t$ (178)   &  $\log L_r$             &  $\log L_{[OIII]}$ \\      
               &   $z$     &        &     Jy       & erg s$^{-1}$ Hz$^{-1}$  &   erg s$^{-1}$     &                &   $z$     &        &      Jy       & erg s$^{-1}$ Hz$^{-1}$  &   erg s$^{-1}$     \\     
               &           &        &               &              &                    &                       &           &        &               &              &       \\
   3C~15       &   0.073   &   LEG  &      15.8     &   31.54      &       40.38        &           3C~227$^a$  &   0.086   &   WQ   &      30.0     &   30.48      &       41.78          \\  
   3C~17       &   0.220   &   WQ   &	   20.0     &   32.76	   &	   41.91    	&   	    3C~234      &   0.185   &   WQ   &      26.1     &   31.88      &       43.17          \\  
   3C~18       &   0.188   &   HEG  &	   19.8     &   31.84	   &	   41.88    	&  	    3C~236      &   0.099   &   LEG  &      20.5     &   31.51      &       40.47          \\  
   3C~33       &   0.059   &   HEG  &	   53.0     &   30.27	   &	   42.01    	&   	    3C~284      &   0.239   &   HEG  &       6.1     &   30.25      &       42.19          \\  
   3C~33.1     &   0.181   &   WQ   &	   11.4     &   31.03	   &	   41.66    	&  	    3C~285      &   0.079   &   HEG  &      6.0      &   29.93      &       40.73          \\  
   3C~35       &   0.067   &   LEG  &	    7.3     &   30.27	   &	   40.03    	&  	    3C~287.1    &   0.216   &   QSO  &      14.2     &   32.53      &        --            \\  
   3C~40       &   0.018   &   LEG  &	   28.6     &   30.60	   &	   38.85    	&  	    3C~300      &   0.270   &   HEG  &      17.97    &   31.07      &       42.16          \\  
   3C~61.1     &   0.184   &   LEG  &	   34.51    &   30.33	   &	   42.09    	&  	    3C~303      &   0.141   &   WQ   &      10.6     &   31.80      &        --            \\  
   3C~63       &   0.175   &   HEG  &	   19.1     &   30.97	   &	    --      	&  	    3C~318.1    &   0.046   &   LEG  &      12.0     &    --        &        --            \\  
   3C~79       &   0.256   &   HEG  &	   24.8     &   31.19	   &	   42.43    	&  	    3C~319      &   0.192   &   LEG  &      14.2     &   29.93      &        --            \\  
   3C~88       &   0.030   &   LEG  &	   17.5     &   30.50	   &	   39.78    	&  	    3C~321      &   0.096   &   HEG  &      11.2     &   30.78      &       42.15          \\  
   3C~98       &   0.030   &   HEG  &	   35.5     &   29.25	   &	   40.87    	&  	    3C~323.1    &   0.264   &   QSO  &      10.0     &   31.69      &       42.93          \\  
   3C~105      &   0.089   &   HEG  &	   18.0     &   30.36	   &	   40.78    	&  	    3C~326      &   0.089   &   LEG  &       7.8     &   30.34      &       40.64          \\  
   3C~111      &   0.049   &   WQ   &	   35.2     &   31.69	   &	    --      	&  	    3C~327      &   0.104   &   HEG  &      43.0     &   30.88      &       42.05          \\  
   3C~123      &   0.218   &   LEG  &	  189.0     &   31.82	   &	   41.58     	&  	    3C~332      &   0.152   &   QSO  &       9.5     &   30.65      &        --            \\  
   3C~132      &   0.214   &   LEG  &	   12.4     &   31.40	   &	    --      	&  	    3C~349      &   0.205   &   HEG  &      13.3     &   31.18      &       41.42          \\  
   3C~133      &   0.277   &   --   &	   21.0     &   32.32	   &	    --      	&  	    3C~353      &   0.030   &   LEG  &      220.0    &   30.54      &       39.34          \\  
   3C~135      &   0.127   &   HEG  &	   18.2     &   30.18	   &	    --      	&  	    3C~357      &   0.167   &   HEG  &       8.2     &   30.48      &        --            \\  
   3C~136.1    &   0.064   &   --   &	   14.0     &    --	   &	    --      	&  	    3C~379.1    &   0.256   &   HEG  &       --      &    --        &        --            \\  
   3C~153      &   0.277   &   HEG  &	   16.67    &   29.73	   &	    --      	&  	    3C~381      &   0.161   &   HEG  &      15.2     &   30.48      &       42.37          \\  
   3C~165      &   0.296   &   LEG  &	   13.5     &   31.08	   &	    --      	&  	    3C~382      &   0.058   &   WQ   &      15.2     &   31.13      &       41.52          \\  
   3C~166      &   0.245   &   --   &	   14.7     &   32.73	   &	    --      	&  	    3C~388$^b$  &   0.091   &   LEG  &      22.5     &   31.04      &       40.49          \\  
   3C~171      &   0.238   &   HEG  &	   21.8     &   30.36	   &	   42.50    	&  	    3C~390.3$^b$ &   0.056   &   WQ   &      52.4     &   31.38      &       42.05          \\  
   3C~173.1    &   0.292   &   LEG  &	   14.3     &   31.18	   &	   41.35    	&  	    3C~401      &   0.201   &   LEG  &      24.0     &   31.50      &       41.01          \\  
   3C~180      &   0.220   &   --   &	   14.2     &    --   	   &	    --    	&  	    3C~402      &   0.025   &   HEG  &      9.0      &   29.73      &        --            \\  
   3C~184.1    &   0.118   &   HEG  &	   14.3     &   30.25	   &	   42.19    	&  	    3C~403      &   0.059   &   HEG  &      28.0     &   29.87      &       41.55          \\  
   3C~192      &   0.060   &   HEG  &	   23.2     &   29.73	   &	   41.60    	&  	    3C~430      &   0.056   &   --   &       --      &    --        &        --            \\  
   3C~197.1    &   0.131   &   HEG  &	    8.1     &   30.30	   &	    --      	&  	    3C~436      &   0.215   &   HEG  &      15.7     &   31.21      &       41.52          \\  
   3C~198      &   0.082   &   HEG  &	   18.0     &    --	   &	   41.04    	&  	    3C~445$^{a,b}$  &   0.057   &   QSO  &      23.5     &   31.34      &       42.05          \\  
   3C~219      &   0.174   &   WQ   &	   34.3     &   31.54	   &	   41.62    	&  	    3C~452      &   0.081   &   HEG  &      58.3     &   31.24      &        --            \\  
   3C~223      &   0.137   &   HEG  &	   14.2     &   30.57	   &	   42.17    	&  	    3C~456      &   0.233   &   HEG  &      14.0     &   31.39      &       42.59          \\  
   3C~223.1    &   0.108   &   HEG  &	   8.7      &   30.24	   &	   41.65    	&  	    3C~458      &   0.289   &   --   &       --      &    --        &        --            \\  
		&          &        &               &              &                    &	    3C~460      &   0.268   &   HEG  &       8.1     &   31.39      &       41.67          \\  



\hline                                                                        				  
                                                                              				  
\end{tabular}                                                                 
\label{tab1}

\medskip

Redshifts and  $S_t$, the total radio  flux at 178 MHz,  are from NED;
optical   spectral  classification   is  from   Jackson   \&  Rawlings
\cite{jackson}       and      C.        Willott's       web      page,
http://www-astro.physics.ox.ac.uk/~cjw/3crr/3crr.html;  $L_r$  is  the
radio core  luminosity at 5  GHz (data are  taken from Zirbel  \& Baum
\cite{zirbel95}),    except   for    3C~123    (Hardcastle   et    al.
\cite{hardcastle98}, 8.44 GHz),  3C~133 (Nilsson \cite{nils98}, 5GHz),
3C~153  (Hardcastle  et al.   \cite{hardcastle98},  8.44 GHz),  3C~165
(Nilsson   \cite{nils98},  5   GHz),  3C~223.1   (Hardcastle   et  al.
\cite{hardcastle98},   8.35   GHz);    3C~349   (Hardcastle   et   al.
\cite{hardcastle98},  8.44  GHz).   Radio  core  data  at  frequencies
different  from  5   GHz  were  converted  to  5   GHz  using  a  flat
($\alpha_r=0$) spectral index.  $L_{[OIII]}$  is the luminosity of the
[OIII]  line  (again  from  Jackson  \&  Rawlings  \cite{jackson}  and
Willott's  web page,  except  for  3C~88, which  has  been taken  from
Tadhunter et al. \cite{tadhunter93}).  (a) line subtracted (see text);
(b) saturated core (see Paper~II for  an outline of the method used to
estimate the flux).


                                                                              
                                                                              
\end{table*}                                                                   

