Table 3: Observer's and source's frame three-frequency Rotation Measures and $n_{1.4}\times 180^\circ $ ambiguities.
  Name $RM_{\rm {obs}}$ $RM_{\rm sf}$    n1.4     Name $RM_{\rm {obs}}$ $RM_{\rm sf}$   n1.4  
$\dag $ 0034+444 59 1850   1    $\dag $ 0809+404 -56 -156 no -1  
  0039+412 -98 [-118]   -1     0930+389 33 3800   4 5
$\dag $ 0110+401 -61 55 * 0 1   0951+422 78 533   1 2
  0120+405 -378 - 1043   -5     0955+390 16 [29] no 0  
  0137+401 -235 - 1133   -3 -4,-5  $\dag $ 1039+424 13 [17]   0  
  0144+432 -56 72   -1  -2  $\dag $ 1055+404A 9 [0]   0  
  0213+412 -67 7 ** -1  -2   1201+394 33 50   0 1
  0222+422A 75 2940   1 2,3   1216+402 -117 -347   -1 -2
  0228+409A -14 [235]   0  -1   1220+408 25 [67] * 1  
  0254+406 -25 221   0 1   1233+418 - 10 -8   0  
  0701+392 254 1230   4 5,6  $\dag $ 1343+386 68 476 no 0 1
  0744+464 -276 - 4400   -3  -4   1350+432 152 1419   2 3
$\dag $ 0748+413B -45 [-227]   -1     1458+433 - 5 -52   0  
$\dag $ 0754+396 4 - 49 * 1     2304+377 96 956 * 1  
$\dag $ 0800+472 -18 [-113] * -1  -2   2311+469 66 416   1  
  0805+406 23 [65] * 0                
A $\dag $ marks sources not classified as $\it CSO$ or $\it MSO$ (see Table A.1).  $[RM_{\rm sf}]$ 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. 4.3. The sixth column contains alternative, plausible number of turns of phase to add to the 1.4 GHz polarization angles.

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