Table A.1.
Radio properties of the 45 detected sources.
| Name | RA | Dec | Beam | BPA |  |
rms |
|---|---|---|---|---|---|---|
| (h:m:s) | (d:m:s) | (arcsec) | (deg) | (mJy beam−1) | (μ Jy beam−1) | |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
| NGC410 | 01:10:58.91 | 33:09:07.1 | 0.18 × 0.13 | −82.6 | 0.72 ± 0.01 | 11.1 |
| NGC488 | 01:21:46.80 | 05:15:24.6 | 0.22 × 0.14 | −58.3 | 0.14 ± 0.01 | 10.7 |
| NGC521 | 01:24:33.77 | 01:43:52.9 | 0.23 × 0.14 | −53.3 | 0.34 ± 0.01 | 10.6 |
| NGC660 | 01:43:02.32 | 13:38:44.9 | 0.21 × 0.14 | −66.2 | 62.80 ± 0.12 | 9.0 |
| NGC777 | 02:00:14.91 | 31:25:45.9 | 0.22 × 0.13 | −76.4 | 0.53 ± 0.01 | 10.7 |
| NGC841 | 02:11:17.37 | 37:29:49.7 | 0.21 × 0.13 | −79.9 | 0.06 ± 0.01 | 7.8 |
| NGC1055 | 02:41:45.20 | 00:26:38.1 | 0.29 × 0.14 | −54.4 | 0.18 ± 0.01 | 10.6 |
| NGC1169 | 03:03:34.74 | 46:23:11.1 | 0.23 × 0.13 | −81.0 | 0.36 ± 0.01 | 9.8 |
| NGC1961 | 05:42:04.65 | 69:22:42.4 | 0.26 × 0.13 | 72.8 | 0.50 ± 0.01 | 9.5 |
| NGC2681 | 08:53:32.72 | 51:18:49.2 | 0.17 × 0.14 | −87.2 | 0.34 ± 0.01 | 9.6 |
| NGC2683 | 08:52:41.30 | 33:25:18.7 | 0.19 × 0.13 | 65.6 | 0.45 ± 0.01 | 10.8 |
| NGC2832 | 09:19:46.85 | 33:44:59.0 | 0.17 × 0.13 | 67.5 | 0.20 ± 0.01 | 9.2 |
| NGC2859 | 09:24:18.53 | 34:30:48.6 | 0.17 × 0.13 | 65.2 | 0.05 ± 0.01 | 8.9 |
| NGC2985 | 09:50:22.18 | 72:16:44.2 | 0.18 × 0.14 | −46.0 | 1.14 ± 0.01 | 12.3 |
| NGC3642 | 11:22:17.90 | 59:04:28.3 | 0.15 × 0.12 | 15.0 | 0.78 ± 0.01 | 10.5 |
| NGC3735 | 11:35:57.22 | 70:32:07.8 | 0.16 × 0.12 | 9.4 | 0.39 ± 0.01 | 9.7 |
| NGC3898 | 11:49:15.24 | 56:05:04.3 | 0.14 × 0.12 | 20.2 | 0.21 ± 0.01 | 9.0 |
| NGC3982 | 11:56:28.14 | 55:07:30.9 | 0.14 × 0.12 | 22.0 | 0.56 ± 0.01 | 10.2 |
| NGC3992 | 11:57:35.96 | 53:22:29.0 | 0.14 × 0.12 | 25.5 | 0.17 ± 0.01 | 9.9 |
| NGC4036 | 12:01:26.75 | 61:53:44.6 | 0.15 × 0.12 | 10.6 | 0.60 ± 0.01 | 11.6 |
| NGC4051 | 12:03:09.61 | 44:31:52.7 | 0.13 × 0.12 | −31.6 | 0.48 ± 0.01 | 12.3 |
| NGC4111 | 12:07:03.13 | 43:03:56.3 | 0.13 × 0.12 | −31.4 | 0.19 ± 0.01 | 12.1 |
| NGC4145 | 12:10:01.56 | 39:53:00.9 | 0.14 × 0.12 | −32.7 | 0.09 ± 0.01 | 9.2 |
| NGC4346 | 12:23:27.96 | 46:59:37.6 | 0.14 × 0.12 | −32.6 | 0.06 ± 0.01 | 8.3 |
| NGC4395 | 12:25:48.88 | 33:32:48.7 | 0.13 × 0.12 | −17.9 | 0.17 ± 0.01 | 11.1 |
| NGC4750 | 12:50:07.32 | 72:52:28.6 | 0.17 × 0.12 | 15.6 | 0.86 ± 0.01 | 12.5 |
| NGC5194 | 13:29:52.71 | 47:11:42.8 | 0.26 × 0.15 | 70.5 | 0.25 ± 0.01 | 14.2 |
| NGC5195 | 13:29:59.53 | 47:15:58.3 | 0.27 × 0.14 | 69.5 | 0.25 ± 0.01 | 14.3 |
| NGC5273 | 13:42:08.38 | 35:39:15.5 | 0.24 × 0.14 | 67.5 | 0.19 ± 0.01 | 12.0 |
| NGC5395 | 13:58:37.96 | 37:25:28.2 | 0.23 × 0.13 | 67.2 | 0.11 ± 0.01 | 12.3 |
| NGC5448 | 14:02:50.05 | 49:10:21.2 | 0.25 × 0.14 | 71.8 | 0.06 ± 0.01 | 12.3 |
| NGC5485 | 14:07:11.35 | 55:00:06.0 | 0.22 × 0.15 | 80.4 | 0.56 ± 0.01 | 13.1 |
| NGC5566 | 14:20:19.89 | 03:56:01.4 | 0.28 × 0.13 | 48.6 | 1.40 ± 0.01 | 29.3 |
| NGC5631 | 14:26:33.29 | 56:34:57.4 | 0.17 × 0.14 | −86.1 | 0.64 ± 0.01 | 11.8 |
| NGC5746 | 14:44:55.98 | 01:57:18.1 | 0.28 × 0.13 | 46.5 | 1.35 ± 0.02 | 22.6 |
| NGC5850 | 15:07:07.68 | 01:32:39.3 | 0.25 × 0.13 | 45.4 | 0.10 ± 0.01 | 11.1 |
| NGC5921 | 15:21:56.49 | 05:04:14.3 | 0.22 × 0.13 | 44.2 | 0.13 ± 0.01 | 11.7 |
| NGC5985 | 15:39:37.06 | 59:19:55.2 | 0.21 × 0.15 | −86.4 | 0.53 ± 0.01 | 11.6 |
| NGC6340 | 17:10:24.84 | 72:18:15.9 | 0.19 × 0.12 | −41.8 | 0.59 ± 0.01 | 10.2 |
| NGC6482 | 17:51:48.83 | 23:04:18.9 | 0.14 × 0.14 | 34.5 | 0.42 ± 0.01 | 9.0 |
| NGC6703 | 18:47:18.82 | 45:33:02.3 | 0.14 × 0.12 | −20.7 | 0.63 ± 0.01 | 9.2 |
| NGC6951 | 20:37:14.12 | 66:06:20.0 | 0.16 × 0.12 | 24.0 | 0.26 ± 0.01 | 11.2 |
| NGC7814 | 00:03:14.90 | 16:08:43.2 | 0.16 × 0.14 | −77.3 | 1.19 ± 0.01 | 9.5 |
| IC356 | 04:07:46.89 | 69:48:44.7 | 0.25 × 0.13 | −81.8 | 1.28 ± 0.01 | 16.2 |
| IC520 | 08:53:42.25 | 73:29:27.4 | 0.20 × 0.13 | −60.1 | 0.15 ± 0.01 | 9.3 |
Notes. Columns are: (1) galaxy name; (2) and (3) observed radio position (RA and Dec) of the detected source; (4) and (5) the beam size and beam position angle of the maps from which the previous columns data are derived; (6) peak 15 GHz radio flux density in mJy beam−1 with errors on the flux; (7) rms in μ Jy beam−1.
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