\begin{table}%t5
\caption{\label{tab:rm-lit}Polarisation parameters of CSSs from mas-resolution observations. }
\small%\centering
\par
\begin{tabular}{lccccccll} 
\hline
\hline\noalign{\smallskip} 
Name     & Alt. Name  &  $z$    & Id. &  $m$                      &  DP                & $RM_{\rm rf}$      &  Notes                           & Ref. \\
         &            &       &     &  (\%)                   &                    & (rad~m$^{-2}$)&                                  &      \\
\hline
3C~43     & B0127+233   & 1.459 & Q   & ~0.4$_{\rm{1.6~GHz}}$  &                    & ~~~~14~236   &  E, $\sim$1600~pc from core         & 1   \\
3C~119\tablefootmark{a}& B0429+415   & 1.023 & Q?  & 14.4$_{\rm{8.4~GHz}}$  & 0.08$_{5.0/8.4}$   &  ~~~~10~200  &  C, $\sim$325~pc from core          & 2  \\
3C~138    & B0518+165   & 0.759 & Q   &  ~3.6$_{\rm{5.0~GHz}}$ &                    &  ~~$-$5287    &  B1, $\sim$40~pc from core          & 3   \\
3C~147    & B0538+498   & 0.545 & Q   &  ~6.6$_{\rm{8.4~GHz}}$ &                    & ~~$-$4872     &  BN, $\sim$37~pc from core A$_0$    & 4  \\
4C~16.14\tablefootmark{b} & B0548+165& 0.474 & Q   &~6.2$_{\rm{8.4~GHz}}$   & 0.26$_{4.6/8.4}$   & ~~$-$4275     &  5C, $\sim$540~pc from core         & 5  \\
3C~216    & B0906+430   & 0.670 & Q   &  30.0$_{\rm{8.4~GHz}}$ & 0.97$_{4.8/8.4}$   & ~~~~2200      &  Arc, $\sim$1050~pc from core       & 6 \\
3C~286\tablefootmark{c}& B1328+307   & 0.849 & Q   & 11.0$_{\rm{5.0~GHz}}$  &                    &                &  Core unclear                       & 7,12   \\
3C~287\tablefootmark{d}& B1328+254   & 1.055 & Q   & ~4.6$_{\rm{5.0~GHz}}$  &                    & ~~~~~~$\sim$0 &  Based on only 8.15 and 8.54~GHz    & 8   \\
OQ~172\tablefootmark{e}& B1442+101   & 3.529 & Q   & ~2.7$_{\rm{8.4~GHz}}$  &                    &   ~~40~000       &  Within $\sim$20~pc from core       & 9,11   \\
3C~309.1  & B1458+718   & 0.905 & Q   & ~1.5$_{\rm{~15~GHz}}$  &
0.10$_{8.4/15}$    & ~~$-$1633   & Core {\it RM} between 8.4 and 15~GHz & 10 \\
3C~318    & B1517+204   & 1.574 & NG  & ~3.5$_{\rm{4.8~GHz}}$  &                    &  ~~~~3030     &  K2, Core unclear                   & 2   \\
OR$-$140\tablefootmark{f}& B1524$-$136 & 1.687& Q & 30.2$_{\rm{8.4~GHz}}$  & $\sim$1$_{4.6-5.1/8.4}$   &$-$10~000 &  C, $\sim$810~pc from core F        & 5 \\
3C~343\tablefootmark{g}& B1634+628   & 0.988 & Q   & ~4.8$_{\rm{8.4~GHz}}$  & 0.91$_{4.6-5.1/8.4}$ & ~~~$>$6000     &  core unclear      & 2 \\
%3C380    &B1828+48 & 0.69~ & Q  &             &           &           &   2 ?? \\
3C~454    & B2249+185   & 1.757 & Q   & 10.9$_{\rm{1.6~GHz}}$  &                    &  ~~~~5334     & B, $\sim$300~pc from possible core  &   1   \\  
\hline 
\end{tabular}
\tablefoot{Table~\ref{tab:rm-lit} is organised as follows: 
Col.~1, source name; 2, alternative name; 3, redshift; 
4, optical identification; 
5, polarisation percentage of the emission; 
6, highest value of depolarisation;
7, highest measured rest frame {\it RM}; 
8, notes: letters refer to components designetion as in references
quoted in Col.~9; 9, references: 
1) Cotton et~al. (2003);
2)~present work; 3) \citet{Cotton03b}; 4) \citet{Rossetti09};
5) \citet{Mantovani02}; 6) \citet{Venturi99}; 7) \citet{Jiang96};
8) \citet{Dallacasa98}; 9) \citet{Udomprasert97}; 10) \citet{Aaron97};
11)~Mantovani, private communication; 12) Cotton et~al. (1997).\\
 \tablefootmark{a}{$m$ and DP values are for component~C, where the peak of polarised 
intensity is surrounded by
a region with {\it RM} in the range of $\sim$9000$-$10~200~rad~m$^{-2}$;}
\tablefootmark{b}{$m$ and DP values are for the entire component~5;}
\tablefootmark{c}{fractional polarisations are 8.9 and 11.0\% at 5~GHz for 
the western and eastern knots respectively (Cotton et~al. 1997);
polarisation is 11.3\% for the dominant component~with the VLA-A array 
at 4.885~GHz (Perley 1982); 
     {\it RM} expected to be low but not determined with mas resolution;}
\tablefootmark{d}{polarisation is 4.6\% with the VLA-A array at 4.885~GHz (Perley 1982);} 
\tablefootmark{e}{polarisation is 2.0\% with the VLA-A array at 4.885~GHz (Perley 1982);} 
\tablefootmark{f}{DP estimated using 8.4~GHz and the mean of four measurements between 
4.6 to 5.1~GHz; }
\tablefootmark{g}{DP estimated using 8.4~GHz and the mean of four measurements between 
4.6 to 5.1~GHz for component~A;
there appears to be different regions of high {\it RM}. 
}  
}
\end{table}