Table A.1
Catalogue of the detected Faraday sources.
| Name | RA | Dec | φ [rad/m2] | PI [mJy] | p [%] | RM [rad/m2] | PI [mJy] | p [%] | RM [rad/m2] | PI [mJy] | p [%] |
| (Han et al. 1998) | (Taylor et al. 2009) | ||||||||||
|
|
|||||||||||
| J005058+420637 | 00h50m58.2s | 42d 6m37.1s | 28.0 ± 0.3 | 4.18 ± 0.15 | 1.63 | ||||||
| J005000+414836 | 00h50m00.8s | 41d48m36.0s | −94.0 ± 0.6 | 2.36 ± 0.15 | 1.73 | ||||||
| T1421 | 00h48m43.9s | 40d45m36.7s | −86.0 ± 0.2 | 9.12 ± 0.15 | 1.48 | −81.9 ± 1.6 | 23.46 ± 0.18 | 13.83 ± 0.11 | |||
| T1407(5) | 00h48m13.0s | 40d22m57.2s | −42.0 ± 0.1 | 26.38 ± 0.15 | 1.41 | −96.7 ± 1.8 | 28.28 ± 0.23 | 6.12 ± 0.05 | |||
| T1375? | 00h46m56.1s | 40d32m54.5s | −94.0 ± 0.5 | 3.03 ± 0.15 | 1.36 | −88.2 ± 12.9 | 4.95 ± 0.37 | 9.51 ± 0.71 | |||
| T1379? | 00h46m55.1s | 40d37m24.6s | −86.0 ± 0.1 | 10.02 ± 0.15 | 4.46 | −91.3 ± 14.4 | 5.0 ± 0.39 | 9.49 ± 0.74 | |||
| 37W235?T1373(1) | 00h46m42.2s | 42d10m11.9s | −104.0 ± 0.9 | 1.61 ± 0.15 | ↓0.47 | −199.9 ± 119 | 4.56 ± 0.26 | 3.39 ± 0.19 | |||
| 37W219 | 00h45m40.2s | 41d12m334s | −72.0 ± 0.8 | 1.87 ± 0.15 | 1.46 | −83 ± 9 | 0.5 ± 0.05 | 4 | |||
| 37W211/T1332 | 00h45m12.3s | 41d12m20.8s | −86.0 ± 0.8 | 1.81 ± 0.15 | 1.35 | −86 ± 1 | 4.2 ± 0.06 | 20 | −85.9 ± 15.4 | 3.61 ± 0.29 | 11.67 ± 0.94 |
| 37W207B(2) | 00h45m04.7s | 41d23m21.4s | −50.0 ± 0.4 | 3.99 ± 0.15 | 2.22 | −129 ± 7 | 0.55 ± 0.1 | 15 | |||
| J004440+424938 | 00h44m40.6s | 42d49m38.9s | −68.0 ± 0.4 | 3.82 ± 0.15 | ↓0.27 | ||||||
| 37W175b | 00h43m58.7s | 41d57m40.3s | −124.0 ± 0.9 | 1.67 ± 0.15 | ↓0.37 | −127 ± 3 | 2.09 ± 0.06 | 5 | |||
| 37W172(8) | 00h43m54.7s | 40d46m40.3s | −150.0 ± 1.1 | 1.25 ± 0.15 | ↓0.31 | −68 ± 3 | 2.7 ± 0.14 | 2 | |||
| 37W154? | 00h43m12.3s | 40d27m41.3s | −22.0 ± 0.2 | 6.12 ± 0.15 | 21.62 | ||||||
| 37W131 | 00h42m36.6s | 41d58m11.7s | −90.0 ± 1.0 | 1.43 ± 0.15 | ↓0.76 | −93 ± 2 | 1.88 ± 006 | 3 | |||
| 37W115/T1237?(6) | 00h42m22.0s | 41d28m56.5s | −30.0 ± 0.3 | 4.95 ± 0.15 | ↓0.47 | −92 ± 1 | 8.58 ± 0.06 | 3 | −71.1 ± 10.4 | 6.82 ± 0.34 | 1.86 ± 0.09 |
| 37W114 | 00h42m17.3s | 40d10m41.2s | −52.0 ± 0.2 | 8.22 ± 0.15 | ↓0.39 | ||||||
| 37W074A/B(4) | 00h41m11.4s | 41d25m09.2s | −54.0 ± 0.7 | 2.04 ± 0.15 | 2.05 | −105 ± 5 | |||||
| 37W058 | 00h40m33.3s | 40d28m06.7s | 28.0 ± 0.6 | 2.22 ± 0.15 | 3.65 | ||||||
| 37W045/T1126 | 00h39m55.9s | 41d11m48.8s | −100.0 ± 0.5 | 2.72 ± 0.15 | 1.32 | −113 ± 6 | 0.55 ± 0.06 | 4 | −103.2 ± 13.9 | 4.63 ± 0.3 | 6.69 ± 0.43 |
| 37W033 | 00h39m28.9s | 41d46m31.2s | −122.0 ± 0.6 | 2.38 ± 0.15 | ↓0.86 | ||||||
| J003901+410928 | 00h39m01.6s | 41d 9m28.0s | −32.0 ± 0.5 | 2.91 ± 0.15 | |||||||
| J003847+412056 | 00h38m47.6s | 41d20m56.3s | −36.0 ± 0.5 | 2.76 ± 0.15 | |||||||
| 37W021 | 00h38m46.6s | 41d16m11.1s | −62.0 ± 1.0 | 1.48 ± 0.15 | ↓0.99 | ||||||
| J003825+411538 | 00h38m25.3s | 41d15m38.2s | −36.0 ± 0.6 | 2.3 ± 0.15 | |||||||
| J003830+415409 | 00h38m30.8s | 41d54m09.2s | −42.0 ± 0.3 | 5.35 ± 0.15 | 3.39 | ||||||
| 37W019? | 00h38m36.5s | 41d28m09.8s | −38.0 ± 0.4 | 3.19 ± 0.15 | 8.8 | ||||||
| 37W014/T1119 | 00h38m25.1s | 41d37m53.3s | −110.0 ± 0.3 | 4.26 ± 015 | ↓0.72 | −94.1 ± 6.9 | 8.78 ± 0.28 | 1.35 ± 0.04 | |||
| 37W008 | 00h37m45.1s | 40d26m16.7s | −32.0 ± 0.3 | 5.26 ± 0.15 | 1.79 | ||||||
| T1067 | 00h37m09.1s | 41d34m56.1s | −96.0 ± 0.4 | 3.52 ± 0.15 | 1.4 | −91.7 ± 14.4 | 4.29 ± 0.28 | 11.17 ± 0.73 | |||
| T1061(3) | 00h37m05.0s | 41d36m10.3s | −48.0 ± 0.4 | 3.85 ± 0.15 | 1.14 | −107.6 ± 12.8 | 4.81 ± 0.29 | 8.63 ± 0.52 | |||
| T1006 | 00h35m25.2s | 39d43m32.2s | −102.0 ± 0.4 | 3.37 ± 0.15 | ↓0.85 | −110.8 ± 11.4 | 5.86 ± 0.29 | 4.4 ± 0.22 | |||
| T974(7) | 00h34m29.2s | 40d37m34.2s | −104.0 ± 0.3 | 5.17 ± 0.15 | 1.24 | −58.2 ± 14.5 | 4.15 ± 0.31 | 3.53 ± 0.26 | |||
Notes. Numbers in brackets behind the names ((1)(2)(3)(4)(5)(6)(7)(8)) are sources with deviating values with regard to the literature, see Sect. 5.2.2 and Figs. 6 and 7. J003901+410928, J003847+412056 and J003825+411538 from the triplet (see Sect. 5.2.1) a peculiar foreground pattern with no counterpart in Stokes I (hence there are no values for p given). Values of p marked with ↓ denote upper limits, assuming a reasonable calibration limit of p = 1%. The sources are ordered from east to west.
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