\begin{table}%t4 \caption{\label{tab:3c343-par}Polarimetric parameters for the components A and B of 3C~343. } \small%\centering \par \begin{tabular}{cccccccccccr} \hline \hline\noalign{\smallskip} Comp. A & & & & & & & &\\ IFs & & $S_{\rm tot}$ & $S_{\rm peak}$ &rms($1\sigma$)& $S_{\rm pol}$& rms($1\sigma$)& maj.ax & min.ax. & PA & $m$ & EVPA \\ & MHz & mJy & mJy/b & mJy/b & mJy & mJy/b & mas & mas & deg& \% & deg \\ \hline IF1 & 4619 & 102.1 & 30.3 & 0.4 & 3.7 & 0.2 & 16.8 & 8.4 & 108 & 3.6 & see Fig.~\ref{fig:3c343-Cband} \\ %75$\pm3$ \\ IF2 & 4657 & 80.0 & 33.3 & 0.6 & 2.6 & 0.2 & 12.5 & 6.5 & 112 & 3.2 &see Fig.~\ref{fig:3c343-Cband} \\ % 78$\pm4$ \\ IF3 & 4854 & 80.3 & 33.5 & 0.3 & 4.8 & 0.2 & 11.9 & 7.1 & 113 & 6.0 &see Fig.~\ref{fig:3c343-Cband} \\ % 83$\pm2$ \\ IF4 & 5094 & 54.7 & 36.0 & 0.4 & 2.6 & 0.2 & 6.5 & 5.0 & 131 & 4.7 &see Fig.~\ref{fig:3c343-Cband} \\ % 80$\pm2$ \\ & & & & & & & & & & & \\ IF1--4 & 8409 & 33.0 & 16.3 & 0.2 & 1.6 & 0.1 & 8.7 & 7.5 & 105 & 4.8 & $-5\pm3$ \\ & & & & & & & & & & & \\ \noalign{\smallskip} Comp.B & & & & & & & & & & & \\ IF1 & 4619 & 470.5 & 77.2 & 0.4 & 2.7 & 0.2 & 19.4 & 16.7 & 117 & 0.6 &see Fig.~\ref{fig:3c343-Cband} \\ % 46$\pm1$ \\ IF2 & 4657 & 305.2 & 69.3 & 0.6 & 3.6 & 0.2 & 16.6 & 13.1 & 128 & 1.2 &see Fig.~\ref{fig:3c343-Cband} \\ % 44$\pm1$ \\ IF3 & 4854 & 391.9 & 80.6 & 0.3 & 4.3 & 0.2 & 16.8 & 14.7 & 149 & 1.1 &see Fig.~\ref{fig:3c343-Cband} \\ % 45$\pm1$ \\ IF4 & 5094 & 208.8 & 68.5 & 0.4 & 3.2 & 0.2 & 12.5 & 10.4 & 131 & 1.5 &see Fig.~\ref{fig:3c343-Cband} \\ % $39\pm1$ \\ & & & & & & & & & & & \\ IF1--4 & 8409 & 198.7 & 51.4 & 0.2 & 5.9 & 0.1 & 15.8 & 11.8 & 5 & 3.0 & --$46\pm1$ \\ \hline \end{tabular} \tablefoot{The values for each components are organised as follows: Col.~1, IF number; 2,~observing frequency; 3,~total flux density; 4,~peak flux density; 5,~1$\sigma$ rms noise; 6,~polarised flux density; 7,~1$\sigma$ rms noise; 8,~major axis; 9,~minor axis; 10,~major axis PA; 11, percentage polarisation; 12,~electric vector position angle.} \end{table}