\begin{table}%t3
\caption{\label{tab3}Percentage of polarised flux density and position angle of the 
electric vector at the five frequencies.}
\small%\centerline
 {
{
\begin{tabular}{llrrrrrrrrrrr}
\hline\hline
Name  &        & $LS$ &$m_{1.4}$ & $m_{2.64}$ & $m_{4.85}$ & $m_{8.35}$ & $m_{10.45}$ & $\chi_{1.4}$ & $\chi_{2.64}$ & $\chi_{4.85}$ & $\chi_{8.35}$ & $\chi_{10.45}$  \\
      &        & [kpc]       &    [$\%$]    &    [$\%$]    &      [$\%$]  &   [$\%$]    &        [$\%$]   & [deg]              & [deg]              & [deg]             & [deg]             & [deg]      \\
\hline
3C 43  &0127+23 & 12.85 &      &     &     & 2.1 $\pm$ 0.6 & 2.1 $\pm$ 0.4 &     &          &           & 2 $\pm$ 2   & 13 $\pm$ 3   \\
3C 48  &0134+32 & 4.00 & 0.44 $\pm$ 0.12 &     & 3.4 $\pm$ 0.8 & 4.9 $\pm$ 0.6 & 5.6 $\pm$ 0.4 & --70.8 $\pm$ 0.1&          & --78 $\pm$ 2 & --68 $\pm$ 2 & --61 $\pm$ 2  \\
3C 49  &0138+13 & 3.85 &      &     &     &     &     &               &          &           &           &            \\
3C 67  &0221+27 & 6.45 & 0.56 $\pm$ 0.12 &     &     & 3.9 $\pm$ 0.6 & 3.7 $\pm$ 0.5 & 59.3 $\pm$ 0.5 &          &           & 62 $\pm$ 2  & 62 $\pm$ 3   \\
4C 34.07&0223+34& 4.04* &      &     &     &     &     &             &          &           &           &            \\
4C 16.09&0316+16& 1.3$^+$ &      &     &     &     &     &          &          &           &           &            \\
       &0319+12& 0.2$^+$ &3.80 $\pm$ 0.18 & 5.6 $\pm$ 0.7 & 6.3 $\pm$ 0.8 & 5.8 $\pm$ 0.6 & 5.0 $\pm$ 0.4 & 41.0 $\pm$ 0.1 & 59 $\pm$ 3 & 73 $\pm$ 2  & 74 $\pm$ 2  & 71 $\pm$ 2   \\
3C 93.1&0345+33 & 0.7 &    &     &     &     & 2.4 $\pm$ 0.4 &           &          &           &           & 59 $\pm$ 3   \\ 
4C 76.03&0404+76& 0.6$^+$&       &     &     &     &     &             &          &           &           &            \\ 
OF247  &0428+20& 0.49 &      &     &     &     &     &           &          &           &           &            \\
3C 119& 0429+41 & 0.9 &      &     &     & 5.9 $\pm$ 0.6 & 8.8 $\pm$ 0.4 &       &          &           & 49 $\pm$ 2  & 179 $\pm$ 2  \\
3C 138& 0518+16 & 3.25 & 7.2 $\pm$ 0.25 &10.3 $\pm$ 0.7 & 9.9 $\pm$ 0.8 &11.7 $\pm$ 0.7 & 9.9 $\pm$ 0.4 & --11.1 $\pm$ 0.0& --11 $\pm$ 2& --13 $\pm$ 2 & --11 $\pm$ 2 & --7 $\pm$ 2   \\
3C 147& 0538+49 & 2.58 &      &     &     &     & 1.2 $\pm$ 0.4 &          &          &           &           & 189 $\pm$ 2  \\ 
3C 186& 0740+38 & 5.14 &      &     &     &     &     &          &          &           &           &            \\ 
3C 190& 0758+14 & 11.19 &     &     &     &     &     &          &          &           &           &            \\ 
3C 216& 0906+43 & 33.44 &     &     &     &     &     &          &          &           &           &            \\ 
3C 237& 1005+07 & 7.11 &      &     &     &     & 1.2 $\pm$ 0.4 &             &          &           &           & 18 $\pm$ 4   \\ 
3C 241& 1019+22 & 3.82 &     &     &     &     &     &           &          &           &           &            \\ 
4C 31.38&1153+31& 3.96 &     &     &     &     & 1.9 $\pm$ 0.4 &             &          &           &           & 16 $\pm$ 4   \\ 
3C 268.3&1203+64& 5.28 &     &     &     & 2.8 $\pm$ 0.6 & 3.0 $\pm$ 0.4 &      &          &           & --97 $\pm$ 2 & --98  $\pm$  6  \\ 
ON343 &1225+36& 0.23$^+$&     &     &     &     &     &           &          &           &           &            \\ 
3C 277.1&1250+56& 4.57 &     &     &        & 3.0  $\pm$  0.6 & 2.6  $\pm$  0.5 &  &          &          & 11 $\pm$ 2  & 7 $\pm$ 6    \\ 
4C 32.44&1323+32& 0.18$^+$ &      &     &     &     &     &         &          &           &           &            \\ 
3C 286& 1328+30 & 15.81 & 6.70 $\pm$ 0.23 &10.9 $\pm$ 0.7 &10.8 $\pm$ 0.8 &11.7 $\pm$ 0.7 &11.7 $\pm$ 0.5 & 35.0 $\pm$ 0.0 & 31 $\pm$ 2 & 33 $\pm$ 2  & 33 $\pm$ 2  & 33 $\pm$ 2   \\ 
3C 287& 1328+25 & 0.43 & 0.65 $\pm$ 0.12 & 3.6 $\pm$ 0.7 & 3.7 $\pm$ 0.8 & 3.2 $\pm$ 0.6 & 3.3 $\pm$ 0.4 & 29.9 $\pm$ 0.2 & 105 $\pm$ 2&--32 $\pm$ 2  & --15 $\pm$ 2 & --6 $\pm$ 2   \\
4C 62.22&1358+62& 0.17$^+$ &     &     &     &     &     &         &          &           &           &            \\
       &1413+34& 0.26 &          & 3.1 $\pm$ 0.7 &     &     &     &      & 199 $\pm$ 3&           &           &            \\   
3C 298&1416+06  & 9.1 &    &     &     & 1.8 $\pm$ 0.6 & 2.1 $\pm$ 0.4 &         &          &           & --42 $\pm$ 3 & --30 $\pm$ 4  \\ 
3C 299&1419+41  & 36.31 &     &     &     &     &     &         &          &           &           &            \\   
OQ172  &1442+10  & 0.1$^+$ & 1.30 $\pm$ 0.13 & 4.5 $\pm$ 0.9 & 2.6 $\pm$ 0.8 & 2.2 $\pm$ 0.6 &     & --86.2 $\pm$ 0.3& 212 $\pm$ 4& 69 $\pm$ 2  & 76 $\pm$ 3  &            \\
3C 303.1&1443+77& 1.28 &     &     &     &     &     &         &          &           &           &            \\ 
3C 305.1&1447+77& 7.86 &     &     &     &     &     &         &          &           &           &            \\
3C 309.1&1458+71& 9.25 & 1.20 $\pm$ 0.13 & 3.7 $\pm$ 0.7 & 2.4 $\pm$ 0.7 & 2.7 $\pm$ 0.6 & 2.5 $\pm$ 0.4 & 39.9 $\pm$ 0.1 & 104 $\pm$ 2&252 $\pm$ 2  & 247 $\pm$ 2 & 243 $\pm$ 2  \\
3C 318& 1517+20 & 3.25 &     &     & 3.4 $\pm$ 0.8 & 6.6 $\pm$ 0.6 & 9.2 $\pm$ 0.6 &   &          & 60 $\pm$ 2  & --14 $\pm$ 2 & --24 $\pm$ 2  \\
     & 1600+33 & $<$0.4 &    &     &     &     &     &       &          &           &           &            \\
OS111& 1607+26 & 0.19$^+$&     &     &     &     &     &      &          &           &           &            \\   
3C 343&1634+62  & 11.48 &      &     &     &     & 1.4 $\pm$ 0.4 &        &          &           &           & --104 $\pm$ 3 \\   
3C 343.1&1637+62& 1.54 &      &     &     &     &     &       &          &           &           &            \\
3C 346&1641+17  & 27.01 & 2.20 $\pm$ 0.14 &     &     &     & 1.8 $\pm$ 0.4 & --82.7 $\pm$ 0.1&          &           &           & --4 $\pm$ 3   \\  
4C 39.56&1819+39& 3.20 &      &     &     &     &     &       &          &           &           &            \\
3C 380& 1828+48 & 55.62 & 0.45 $\pm$ 0.12 &     &     &     &     & 44.2 $\pm$ 0.1 &          &           &           &            \\  
4C 29.56 &1829+29& 12.40 &     &     &     &     &     &        &          &           &           &            \\
4C 11.69&2230+11& 9.7 & 1.6 $\pm$ 0.13 & 4.0 $\pm$ 0.7 & 3.6 $\pm$ 0.8 & 3.7 $\pm$ 0.6 & 3.6 $\pm$ 0.4 & --61.1 $\pm$ 0.1& 7 $\pm$ 2  & 48 $\pm$ 2  & 58 $\pm$ 2  & 60 $\pm$ 2   \\ 
3C 454 &2249+18 & 8.39 & 3.6 $\pm$ 0.16  & 5.8 $\pm$ 0.7 & 9.3 $\pm$ 0.8 &11.2 $\pm$ 0.7 &11.2 $\pm$ 0.4 & 53.4 $\pm$ 0.1 & 41 $\pm$ 2 & 87 $\pm$ 2  & 98 $\pm$ 2  & 101 $\pm$ 2  \\ 
3C 454.1&2248+71& 5.5 &      &     &     &     &     &         &          &           &           &            \\ 
3C 455&2252+12  & 11.75 & 2.10 $\pm$ 0.14 & 3.4 $\pm$ 0.7 &     &     & 1.5 $\pm$ 0.5 & --7.5 $\pm$ 0.2 & 149 $\pm$ 3&           &           & 151 $\pm$ 8  \\   
     &2342+82  & 0.72$^+$ &     &     &     &     &     &        &          &           &           &            \\  
\hline
\end{tabular}}}
\medskip
Table~\ref{tab3} is organized as follows: Col.~1, source name; Col.~2, other name; Col.~3, source linear size. Asterisks mark sources for which new redshifts have been obtained and new linear sizes were calculated;  $^+$~signs mark sources with improved measurements of their angular sizes (Rossetti et~al. \cite{Rossetti05}; 0319+12 Mantovani in~prep.; 1442+10 Udomprasert et~al. \cite{Udomprasert97}); Cols.~4 to~8, percentage of polarised emission~$m$; Cols.~9 to~13, position angle of the electric vector~$\chi$.
\end{table}