Table 7
Galactic coordinates and RMs for the SVC fields.
| Field | l (deg) | b (deg) |  |
 |
 |
 |
RMmw (rad m–2) |
|---|---|---|---|---|---|---|---|
| SVC1 | 95.681 | −22.349 | −126.19 ±85.31 | −103.81 ±87.77 | −155.42 ±54.08 | −123.29 ±93.68 | −131.07 ±25.95 |
| SVC2 | 100.939 | 60.546 | 9.71 ±33.68 | 15.41 ±35.36 | 8.41 ±30.19 | 16.94 ± 11.79 | 11.82 ± 4.8l |
| SVC3 | 137.785 | −27.078 | −46.59 ± 38.21 | −41.46 ±40.30 | −48.34 ±33.11 | −55.40 ± 29.75 | −47.87 ± 14.88 |
| SVC4 | 97.789 | −17.882 | −159.78 ± 104.27 | −156.20 ± 108.58 | −168.15 ±96.96 | −127.87 ±99.84 | −220.52 ± 22.77 |
| SVC5 | 65.517 | 69.869 | 0.28 ± 30.02 | 0.55 ± 29.72 | −0.73 ± 30.88 | 0.75 ±25.12 | 2.84 ±3.54 |
Notes. l and b are the Galactic longitude and latitude coordinates for each SVC field calculated from the RA-/Dec-coordinates given in Table 4, respectively. 
, and 
are the median rotation measures and their standard derivation of all polarised sources, unresolved polarised sources and resolved polarised sources of a single SVC field, respectively. 
is the median rotation measure and its standard deviation of all sources where an NVSS counterpart could be identified. 
is the rotation measure and its error extracted from the map of Oppermann et al. (2012) for the given l- and b-coordinates.
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