\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}