\begin{table}%t3
\caption{\label{RM_3_tab}Observer's and source's frame three-frequency Rotation Measures and
$n_{1.4}\times 180^\circ$ ambiguities.} 
%\centerline
{
\begin{tabular}{rlrrcrl | llrrcrl}
\hline
\hline
&Name& $RM_{\rm{obs}}$ &$RM_{\rm sf}$& &~$n_{1.4}$&& &Name& $RM_{\rm{obs}}$&$RM_{\rm sf}$& &$n_{1.4}$&\\
\hline
$\dag$&\object{0034+444} &    59&    1850&  &   1&       & ~$\dag$&\object{0809+404} &$-$56&$-$156&no&$-$1&    \\  
      &\object{0039+412} &$-$98&[$-$118]&  &$-$1&       &	     &\object{0930+389} &    33&  3800&  &   4& 5  \\
$\dag$&\object{0110+401} &$-$61&      55& *&   0&      1&	     &\object{0951+422} &    78&   533&  &   1& 2  \\
      &\object{0120+405} &$-$378&$-$ 1043&  &$-$5&       &        &\object{0955+390} &    16&  [29]&no&   0&    \\
      &\object{0137+401} &$-$235&$-$ 1133&  &$-$3&$-4,-5$& ~$\dag$&\object{1039+424} &    13&  [17]&  &   0&    \\
      &\object{0144+432} &$-$56&      72&  &$-$1&~$-$2  & ~$\dag$&\object{1055+404A}&     9&   [0]&  &   0&    \\
      &\object{0213+412} &$-$67&       7&**&$-$1&~$-$2  &	     &\object{1201+394} &    33&    50&  &   0& 1  \\
      &\object{0222+422A}&   75&    2940&  &   1&  2,3  &	     &\object{1216+402} &$-$117&$-$347&  &$-$1&$-$2\\
      &\object{0228+409A}&$-$14&   [235]&  &   0&~$-$1  &	     &\object{1220+408} &    25&  [67]& *&   1&    \\
      &\object{0254+406} &$-$25&     221&  &   0&    1  &	     &\object{1233+418} &$-$ 10&$-$8&  &   0&    \\
      &\object{0701+392} &   254&    1230&  &   4&  5,6  & ~$\dag$&\object{1343+386} &    68&   476&no&   0& 1  \\
      &\object{0744+464} &$-$276&$-$ 4400&  &$-$3&~$-$4  &        &\object{1350+432} &    152& 1419&  &   2& 3  \\
$\dag$&\object{0748+413}B&$-$45&[$-$227]&  &$-$1&       &        &\object{1458+433} &$-$  5&$-$52&  &   0&    \\
$\dag$&\object{0754+396} &     4&$-$   49& *&   1&       &        &\object{2304+377} &    96&   956& *&   1&    \\
$\dag$&\object{0800+472} &$-$18&[$-$113]& *&$-$1&~$-$2  &        &\object{2311+469} &    66&   416&  &   1&    \\
      &\object{0805+406} &    23&    [65]& *&   0&       &        &                  &      &      &  &    &    \\
     \hline
     \end{tabular}}
\smallskip
A~$\dag$ marks sources not classified as~$\it CSO$ or~$\it MSO$ (see
Table~\ref{sample}).~$[RM_{\rm sf}]$ is for sources without red-shift
($z = 1.05$ assumed). Note that~$RM_{\rm sf}$ is  corrected for
Galactic~$RM$ whereas~$RM_{\rm{obs}}$ is  not.
The fourth column contains an * for sources for which we obtain good
agreement with Klein et~al. (2003), **~indicates compatible results
when the NVSS~data is included, "no'' indicates plausible agreement
with a fit of our data that gives an excessive chi-square, see
present Sect.~\ref{rot-angl}. 
The sixth column contains alternative, plausible number of turns of
phase to add to the 1.4~GHz polarization angles.
\end{table}