Table 1
Parameters of the high-RM candidates.
| Source | RA | Dec |
|
|
|
RMobs | z | RMmw | RMrf |
| [J2000] | [J2000] | [mJy] | [mJy] | [rad/m2] | [rad/m2] | [rad/m2] | |||
|
|
|||||||||
| 0239–0234 | 02:39:45.480 | −02:34:40.98 | 300 ± 10 | 723 ± 6 | 0.44 ± 0.04 | –40 ± 10 | 1.1 | –100 ± 100 | –190 ± 30 |
| 0243–0550 | 02:43:12.464 | −05:50:55.36 | 560 ± 17 | 548 ± 2 | −0.01 ± 0.04 | 600 ± 100 | 1.8 | –100 ± 100 | 4500 ± 400 |
| 0742+4900 | 07:42:02.763 | +49:00:15.65 | 398 ± 12 | 430 ± 1 | 0.04 ± 0.04 | –200 ± 30 | 2.3 | 30 ± 10 | –2170 ± 370 |
| 0751+2716 | 07:51:41.492 | +27:16:31.65 | 590 ± 20 | 82 ± 1 | −0.98 ± 0.04 | 500 ± 100 | 3.2 | −-20 ± 10 | 8800 ± 900 |
| 0845+0439 | 08:45:17.151 | +04:39:46.64 | 380 ± 10 | 682 ± 6 | 0.30 ± 0.04 | 1920 ± 20 | 0.8 | –100 ± 100 | 6230 ± 50 |
| 0925+3159 | 09:25:32.726 | +31:59:52.86 | 551 ± 17 | 97 ± 4 | −0.86 ± 0.06 | –100 ± 100 | 1.5* | –10 ± 10 | –400 ± 300 |
| 0958+3224 | 09:58:20.939 | +32:24:02.16 | 1250 ± 40 | 660 ± 6 | −0.32 ± 0.04 | 2200 ± 100 | 0.5 | –10 ± 10 | 5200 ± 200 |
| 1015+0318 | 10:15:34.024 | +03:18:50.06 | 416 ± 13 | 91 ± 2 | −0.76 ± 0.04 | 200 ± 100 | 1.5* | –40 ± 10 | 1600 ± 300 |
| 1043+2408 | 10:43:09.032 | +24:08:35.45 | 320 ± 10 | 1070 ± 10 | 0.60 ± 0.04 | –60 ± 10 | 0.6 | 30 ± 20 | –150 ± 20 |
| 1044+0655 | 10:44:55.921 | +06:55:37.94 | 490 ± 20 | 295 ± 5 | −0.25 ± 0.06 | –210 ± 20 | 2.1 | 20 ± 40 | –2030 ± 170 |
| 1048+0141 | 10:48:22.850 | +01:41:47.46 | 380 ± 10 | 328 ± 3 | −0.07 ± 0.03 | –2510 ± 30 | 0.7 | –100 ± 100 | –7160 ± 90 |
| 1146+5356 | 11:46:44.186 | +53:56:43.36 | 367 ± 11 | 614 ± 6 | 0.26 ± 0.04 | –450 ± 10 | 2.2 | 10 ± 10 | –4570 ± 90 |
| 1213+1307 | 12:13:32.146 | +13:07:20.43 | 1340 ± 40 | 421 ± 3 | −0.60 ± 0.04 | 20 ± 2 | 1.1 | 20 ± 20 | 90 ± 10 |
| 1246–0730 | 12:46:04.231 | −07:30:46.63 | 550 ± 20 | 1040 ± 10 | 0.32 ± 0.04 | 880 ± 10 | 1.2 | 10 ± 40 | 4610 ± 60 |
| 1311+1417 | 13:11:07.835 | +14:17:46.69 | 734 ± 22 | 207 ± 1 | −0.63 ± 0.03 | 570 ± 10 | 1.9 | 10 ± 10 | 4940 ± 100 |
| 1312+5548 | 13:12:53.193 | +55:48:13.21 | 590 ± 20 | 140 ± 3 | −0.72 ± 0.04 | –1000 ± 200 | 1.5* | 20 ± 10 | –6000 ± 1000 |
| 1351+0830 | 13:51:16.926 | +08:30:39.82 | 350 ± 10 | 308 ± 5 | −0.06 ± 0.05 | 70 ± 20 | 1.4 | 50 ± 30 | 410 ± 120 |
| 1405+0415 | 14:05:01.113 | +04:15:35.87 | 930 ± 30 | 712 ± 10 | −0.13 ± 0.04 | 1153 ± 4 | 3.2 | 30 ± 60 | 20420 ± 80 |
| 1435–0414 | 14:35:39.884 | −04:14:55.20 | 480 ± 10 | 146 ± 1 | −0.60 ± 0.03 | 1080 ± 30 | 0.8 | 100 ± 100 | 3500 ± 80 |
| 1549+5038 | 15:49:17.447 | +50:38:05.87 | 630 ± 20 | 813 ± 1 | 0.135 ± 0.04 | 100 ± 100 | 2.2 | 20 ± 10 | 1400 ± 500 |
| 1616+0459 | 16:16:37.530 | +04:59:31.96 | 330 ± 10 | 1035 ± 10 | 0.57 ± 0.04 | 2530 ± 40 | 3.2 | 150 ± 10 | 44630 ± 720 |
| 1616+2647 | 16:16:38.340 | +26:47:01.39 | 1480 ± 50 | 294 ± 5 | −0.80 ± 0.06 | –140 ± 30 | 1.5* | 10 ± 10 | –880 ± 190 |
| 1647+3752 | 16:47:25.735 | +37:52:18.32 | 630 ± 20 | 152 ± 2 | −0.70 ± 0.04 | 80 ± 10 | 1.5* | –20 ± 10 | 490 ± 80 |
| 1713+2813 | 17:13:25.930 | +28:13:07.10 | 1030 ± 40 | 124 ± 2 | −1.05 ± 0.05 | 84 ± 2 | 1.5* | 3 ± 8 | 530 ± 20 |
| 1723+3417 | 17:23:20.801 | +34:17:57.85 | 520 ± 20 | 162 ± 1 | −0.58 ± 0.04 | 83 ± 2 | 0.2 | –30 ± 10 | 120 ± 10 |
| 2050+0407 | 20:50:06.240 | +04:07:49.22 | 565 ± 17 | 566 ± 2 | 0.01 ± 0.06 | 60 ± 10 | 1.5* | 100 ± 100 | 380 ± 60 |
| 2101+0341 | 21:01:38.833 | +03:41:31.29 | 630 ± 20 | 969 ± 1 | 0.21 ± 0.04 | 70 ± 10 | 1.0 | 200 ± 100 | 260 ± 40 |
| 2147+0929 | 21:47:10.162 | +09:29:46.63 | 930 ± 30 | 760 ± 5 | −0.10 ± 0.04 | 1400 ± 20 | 1.1 | –10 ± 40 | 6260 ± 110 |
| 2200+0708 | 22:00:57.607 | +07:08:29.01 | 896 ± 32 | 113 ± 1 | −1.03 ± 0.04 | –15 ± 2 | 1.5* | –20 ± 100 | –90 ± 20 |
| 2245+0324 | 22:45:28.284 | +03:24:08.71 | 480 ± 10 | 379 ± 7 | −0.12 ± 0.04 | –800 ± 100 | 1.3 | –40 ± 100 | –4400 ± 500 |
Notes. The source name, the source coordinates’ right ascension, declination [J2000] taken from the FIRST catalogue, the flux density at 1.4 GHz from the NVSS catalogue, the measured flux density at 10.45 GHz with Effelsberg, the spectral index among these two frequencies α1.4−10.45, the observed RM (RMobs), the contribution of the RM from the Milky Way (RMmw), the redshifts of the sources taken from the literature (where this information was not available, its mean value was considered; marked here with an asterisk), and the rest frame RM (RMrf).
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