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Table 2.
Foreground rotation measure RMfg, distances, linear resolutions that correspond to 12″, and range of observed RMs observed at C-band in the disk and/or halo of the galaxies.
| Galaxy | RMfg | Distance | Lin. res. at 12″ | RMdisk/halo range | Remarks |
|---|---|---|---|---|---|
| [rad m−2] | [Mpc] | [pc] | [rad m−2] | ||
| NGC 660 | −4 ± 10 | 12.3 | 720 | −204 to 330 | Polar ring galaxy |
| NGC 891 | −80 ± 18 | 9.1 | 530 | −209 to 466 | |
| NGC 2613 | 209 ± 27 | 23.4 | 1360 | −328 to 242 | |
| NGC 2683 | 21 ± 7 | 6.3 | 360 | PI too weak | |
| NGC 2820 | −20 ± 9 | 26.5 | 1540 | −173 to 156 | |
| NGC 2992 | −20 ± 16 | 34.0 | 1980 | Central source only | |
| NGC 3003 | 23 ± 7 | 25.4 | 1480 | PI too weak | |
| NGC 3044 | −13 ± 8 | 20.3 | 1180 | −238 to 372 | |
| NGC 3079 | 10 ± 6 | 20.6 | 1200 | −331 to 239 | Strong central source |
| NGC 3432 | 13 ± 5 | 9.4 | 550 | PI too weak | |
| NGC 3448 | 16 ± 5 | 24.5 | 1430 | −232 to 217 | |
| NGC 3556 | 11 ± 6 | 14.9 | 820 | −226 to 362 | |
| NGC 3628 | 9 ± 4 | 8.5 | 490 | −339 to 319 | Strong central source |
| NGC 3735 | −14 ± 7 | 42.0 | 2440 | −216 to 249 | |
| NGC 3877 | 19 ± 5 | 17.7 | 1030 | PI too weak | |
| NGC 4013 | 3 ± 3 | 16.0 | 930 | −248 to 163 | |
| NGC 4096 | 14 ± 4 | 10.3 | 600 | PI too weak | |
| NGC 4157 | 20 ± 4 | 15.6 | 910 | −422 to 255 | |
| NGC 4192 | −8 ± 4 | 13.6 | 790 | −184 to 263 | |
| NGC 4217 | 7 ± 5 | 20.6 | 1200 | −179 to 189 | |
| NGC 4244 | −8 ± 3 | 4.4 | 260 | No polarization at all | |
| NGC 4302 | −6 ± 4 | 19.4 | 1130 | −287 to 214 | |
| NGC 4388 | −2 ± 4 | 16.6 | 970 | −164 to 295 | nuclear outflow(a) |
| NGC 4438 | −3 ± 4 | 10.4 | 600 | Core plus radio lobe only | |
| NGC 4565 | 6 ± 3 | 11.9 | 690 | −204 to 342 | |
| NGC 4594 | −2 ± 6 | 12.7 | 740 | Central source only | |
| NGC 4631 | 0 ± 3 | 7.4 | 430 | −551 to 823 | |
| NGC 4666 | −7 ± 6 | 27.5 | 1600 | −190 to 358 | |
| NGC 4845 | −15 ± 4 | 17.9 | 990 | Central source only(b) | |
| NGC 5084 | −8 ± 10 | 23.4 | 1360 | −49 to 322 | Central source only |
| NGC 5297 | 4 ± 4 | 40.4 | 2350 | PI too weak | |
| NGC 5775 | 17 ± 6 | 28.9 | 1680 | −271 to 335 | |
| NGC 5792 | 1 ± 7 | 32.7 | 1840 | PI too weak | |
| NGC 5907 | 2 ± 7 | 16.8 | 980 | −152 to 126 | |
| UGC 10288 | 3 ± 11 | 34.1 | 1980 | Background radio source only(c) |
Notes.
(a)
See CHANG-ES VII paper (Damas-Segovia et al. 2016).
(b)
See CHANG-ES V paper (Irwin et al. 2015).
(c)
See CHANG-ES III paper (Irwin et al. 2013).
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