0206+35 Using the 2.7 GHz polarization position angle in Parma & Weiler (1981), we obtain a rotation measure of 70 rad (n= 1, see Sect. 4.1).
0755+37 Using the 2.7 GHz polarization position angle in Parma & Weiler (1981), we obtain a rotation measure of (n= -1, see Sect. 4.1).
0913+38 The rotation of the polarization angle between the two wavelengths is rather large ().
1108+27 Using the 2.7 GHz polarization position angle in Parma & Weiler (1981), we obtain a rotation measure of (n=- 1, see Sect. 4.1).
1141+47 The core of the source is now detected in the 4.8 GHz map.
1243+26 The bright spot at and is the radio core of another galaxy. In the southern lobe there is very likely a mixture of the radio emission from the two galaxies.
1254+27 Using the 2.7 GHz polarization position angle in Parma & Weiler (1981), we obtain a rotation measure of (n= -2, see Sect. 4.1).
1300+32 Head-tail source (see Fanti et al. 1986).
1303+31 Head-tail source (see Fanti et al. 1986)
1322+36 The difference in polarization rotation angle between the two lobes is .
1357+28 The difference in polarization rotation angle between the two lobes is .
1430+25 Head-tail source (see Parma et al. 1986).
1441+26 Using the 10.8 GHz polarization position angle in Mack et al.\ (1994), we obtain a rotation measure of 87 rad (n= 1, see Sect. 4.1).
1455+28 The source core is detected in the 4.8 GHz map.
1528+29 Using the 10.8 GHz polarization position angle in Mack et al.\ (1994), we obtain a rotation measure of (n= -1, see Sect. 4.1).
1615+32 (3C 332)
A jet in the southern lobe, not visible in our maps, has been found by Christiansen (1988).
1626+39 Using the 2.7 GHz polarization position angle in Parma & Weiler (1981), we obtain a rotation measure of 116 rad (n= 1, see Sect. 4.1).
1833+32 (3C 382) A bright jet is visible in the northern lobe in the map by Black et al.\ (1992). Using the 2.7 GHz polarization position angle in Parma & Weiler (1981), we obtain a rotation measure of 64 rad (n= 1, see Sect. 4.1).
2116+26 Using the 2.7 GHz polarization position angle in Parma & Weiler (1981), we have two equally acceptable values for the rotation measure: -165 or 178 rad (, see Sect. 4.1).