\begin{table}%t1
\caption{The source sample.}\label{tab:b3-list}
%\centering
\par
\begin{tabular}{lcclclrcc}
\hline \hline
Name & Id & $m_{\rm V}$ & $z$ & $S_{0.4}$ & {\it LAS} & {\it LLS} & Log~$P_{0.4}$ & Morph. \\
    &  &           &  & Jy & \arcsec & $h^{-1}$ kpc & $h^{-2}$ W~Hz$^{-1}$ & \\                    
 (1) & (2) & (3) & (4) & (5) & (6) & (7) & (8) & (9) \\
\hline 
\object{0003+387}  & G & 23.7  & 1.47  & 1.36  & 1.3   & 5.5   &    27.65  & D    \\
\object{0034+444}  & G & 22.8  & 2.79  & 2.25  & 3.2   & 11.9  &    28.53  & U    \\
\object{0039+391}  & G &       & 1.01  & 1.02  & 0.38  & 1.6   &    27.19  & Dc   \\
\object{0039+398}  & E &       &       & 1.98  & 3.7   & 16    & $>$26.8   & Dc   \\
\object{0039+412}  & E &       &       & 0.91  & 2.0   & 8.5   & $>$26.4   & Dc   \\
\object{0041+425}  & E &       &       & 1.26  & 1.0   & 4.1   & $>$26.6   & D    \\
\object{0049+379}  & G &       & 1.7K  & 2.55  & 1.45  & 6.1   &    28.10  & Dc   \\
\object{0110+401}  & Q & 20.0  & 1.479 & 1.08  & 3.9   & 16.7  &    27.44  & cJ   \\
\object{0120+405}  & G &       & 0.84  & 1.68  & 2.4   & 10.1  &    27.20  & Dc   \\
\object{0123+402}  & G & 23.8  &       & 0.81  & 1.22  & 5.2   & $>$26.4   & Ta   \\
\object{0128+394}  & G & 22.9  & 1.6K  & 0.92  & 2.7   & 11.5  &    27.53  & D    \\
\object{0137+401}  & Q & 18.5  & 1.62  & 0.82  & 4.2   & 17.6  &    27.48  & Dc   \\
\object{0140+387}  & G &       & 2.9K  & 1.81  & 1.1   & 4.1   &    28.55  & D    \\
\object{0144+432}  & Q & 21.0  & 1.26  & 0.82  & 4.0   & 17.2  &    27.21  & D    \\
\object{0213+412}  & G & 21.4  & 0.515 & 1.26  & 2.0   & 7.3   &    26.58  & Dc   \\
\object{0222+422}A & G &       & 3.5K  & 0.81  & 3.4   & 11.9  &    28.24  & D    \\
\object{0228+409}A & E &       &       & 0.90  & 3.8   & 16.2  & $>$26.4   & D    \\  
\object{0254+406}  & G & 24.0  & 1.224 & 1.43  & 4.5   & 18.9  &    27.49  & D    \\
\object{0255+460}  & Q & 20.5  & 1.21  & 1.74  & 0.75  & 3.2   &    27.51  & D    \\
\object{0701+392}  & Q & 18.7  & 1.238 & 1.17  & 1.8   & 7.8   &    27.35  & Dc   \\
\object{0722+393}A & E &       &       & 2.91  & 0.25  & 1.0   & $>$26.9   & U    \\ 
\object{0729+437}  & E &       &       & 0.90  & 1.3   & 5.6   & $>$26.4   & Dc   \\
\object{0744+464}  & G &       & 2.926 & 1.66  & 1.4   & 5.1   &    28.46  & Dc   \\
\object{0805+406}  & E &       &       & 1.33  & 2.5   & 10.7  & $>$26.6   & cJ  \\
\object{0809+404}  & G &       & 0.551 & 2.31  & 1.2   & 4.5   &    26.9   & Da   \\
\object{0810+460}B & G & 20.3  & 0.33R & 4.08  & 1.03  & 3.0   &    26.74  & D    \\
\object{0814+441}  & E &       &       & 0.84  & 4.0   & 17.0  & $>$26.4   & Dc   \\ 
\object{0856+406}  & G & 24.3  & 2.28  & 1.07  & 0.8   & 3.2   &    28.10  & D    \\
\object{0902+416}  & E &       &       & 0.93  & 0.34  & 1.4   & $>$26.4   & D    \\ 
\object{0930+389}  & G &       & 2.395 & 0.92  & 3.7   & 14.4  &    27.97  & D    \\
\object{0935+428}A & G & 24.0  & 1.291 & 1.35  & 1.3   & 5.5   &    27.54  & Dc   \\
\object{0951+422}  & Q & 20.5  & 1.783 & 1.08  & 2.0   & 8.3   &    27.64  & D    \\
\object{0955+390}  & E &       &       & 1.05  & 4.8   & 19.2  & $>$26.5   & Dc   \\
\object{1025+390}B & G & 18.7  & 0.361 & 1.54  & 3.2   & 9.7   &    26.36  & Dc   \\
\object{1027+392}  & E &       &       & 0.83  & 1.6   & 6.9   & $>$26.4   & Uc   \\
\object{1044+454}  & G & 24.8  & 4.1K  & 1.67  & 1.0   & 3.2   &    28.82  & Da   \\
\object{1055+404}A & E &       &       & 0.94  & 2.8   & 12.1  & $>$26.5   & cJ	  \\
\object{1128+455}  & G & 18.7  & 0.40  & 4.37  & 0.9   & 2.9   &    26.98  & U    \\
\object{1136+420}  & E & 21.7  & 0.829 & 0.84  & 1.0   & 4.3   & $>$26.5   & Da   \\
\object{1143+456}  & G & 24.0  & 0.762 & 2.26  & 0.8   & 3.3   &    27.26  & D    \\
\object{1157+460}  & G & 21.3  & 0.742 & 2.88  & 0.62  & 2.5   &    27.29  & Dc   \\
\object{1201+394}  & G & 19.0  & 0.445 & 1.11  & 2.1   & 7.2   &    26.40  & Dc   \\
\hline
\object{1204+401}  & G & 23.0  & 2.066 & 1.00  & 1.6   & 6.7   &    27.94  & D    \\
\object{1212+380}  & G & 24.0  & 1.5K  & 1.08  & 0.47  & 2.0   &    27.63  & D    \\
\object{1216+402}  & G & 22.1  & 0.756 & 1.00  & 3.8   & 15.5  &    26.88  & D    \\
\object{1217+427}  & E &       &       & 0.87  & 2.7   & 11.7  & $>$26.5   & D    \\ 
\object{1220+408}  & G & 23.2  &       & 1.50  & 4.1   & 17.6  & $>$26.7   & Dc   \\
\object{1233+418}  & G & 18.4  & 0.25R & 1.47  & 2.2   & 5.3   &    26.00  & D    \\
\object{1241+411}  & G & 17.7  & 0.259 & 0.80  & 1.0   & 2.6   &    25.72  & D    \\
\object{1350+432}  & G & 22.1  & 2.149 & 0.83  & 1.6   & 6.5   &    28.00  & U    \\
\object{1458+433}  & G & 22.3  & 0.927 & 1.08  & 1.6   & 6.9   &    27.08  & Dc   \\
\object{2301+443}  & G &       & 1.7K  & 4.04  & 0.5   & 2.1   &    28.34  & Dc   \\
\object{2302+402}  & E &       &       & 2.53  & 0.6   & 2.6   & $>$26.8   & Dc   \\
\object{2311+469}  & Q & 17.5  & 0.745 & 4.34  & 2.4   & 9.6   &    27.44  & Dc   \\
\object{2322+403}  & E &       &       & 0.85  & 3.2   & 14.0  & $>$26.4   & Dc   \\ 
\object{2349+410}  & Q & 19.2  & 2.046 & 1.38  & 0.82  & 3.3   &    27.99  & Dc   \\
\hline
\end{tabular}
\medskip
Notes. Column~1: source name; Col.~2: optical identification;
 Col.~3: optical magnitude;
 Col.~4: red-shift; K and~R indicate a~photometric red-shift from~$K$
 or $R$~magnitude (\citeauthor*[see][]{Fanti01});
 Col.~5: flux density at 0.4~GHz;
 Col.~6: largest angular size;
 Col.~7: largest linear size computed assuming $z=1.05$ for sources
 without~$z$ (\citeauthor*[see][]{Fanti01});
 Col.~8: Log of radio luminosity at 0.4~GHz; lower limits have been
 computed for $z=0.5$ \citeauthor*[see][]{Fanti01};
 Col.~9: morphological classification: D~= double; T~= triple;
 U~= uncertain; c~= core; cJ~= core-Jet; a~= asymmetric. 
Data are from \citeauthor*{Fanti01,Fanti04}. 
\end{table}