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A. Notes on individual sources

0206+35 Using the 2.7 GHz polarization position angle in Parma & Weiler (1981), we obtain a rotation measure of 70 rad tex2html_wrap_inline2640 (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 tex2html_wrap_inline2720 (n= -1, see Sect. 4.1).

0913+38 The rotation of the polarization angle between the two wavelengths is rather large (tex2html_wrap_inline2724).

1108+27 Using the 2.7 GHz polarization position angle in Parma & Weiler (1981), we obtain a rotation measure of tex2html_wrap_inline2726 (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 tex2html_wrap_inline2730 and tex2html_wrap_inline2732 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 tex2html_wrap_inline2734 (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 tex2html_wrap_inline2738.

1357+28 The difference in polarization rotation angle between the two lobes is tex2html_wrap_inline2740.

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 tex2html_wrap_inline2640 (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 tex2html_wrap_inline2746 (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 tex2html_wrap_inline2640 (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 tex2html_wrap_inline2640 (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 tex2html_wrap_inline2640 (tex2html_wrap_inline2762, see Sect. 4.1).


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