Table 4: Identifiers, positions, peak flux and integrated flux densities for BRC sources detected at 13 or 20 cm. 3$\sigma $ upper limits for non-detections are indicated.
      Peak flux Integrated flux  
Source ID $\alpha$(2000) $\delta$(2000) 13 cm 20 cm 13 cm 20 cm Type
SFO 47a 07:32:10.0 -19:28:48 11.7 14.4 15.0 24.9 4
SFO 47b 07:31:49.0 -19:24:38 28.8 13.5 93.8 186 4
SFO 49a 07:36:02.5 -18:53:16 242 316 274 357 4
SFO 49b 07:35:34.5 -18:45:32 194 294.2 463 568 4
SFO 56 08:42:57.0 -40:00:26 <3.6 5.2a <3.6 5.2a 4
SFO 58a 08:45:15.8 -41:13:33 2.7 <1.0 2.7 <1.0 4
SFO 58b 08:45:19.5 -41:15:13 6.9 <1.0 8.7 <1.0 1
SFO 59 08:58:9.1 -47:21:51 3100 <305 10400 <305 3
SFO 64 11:12:13.7 -58:46:45 14.4 45.6 117 236 1
SFO 69 11:41:04.9 -63:22:05 25.4 <15.0 133 <15.0 4
SFO 74 14:19:40.9 -61:25:17 9.9 25.0 26.3 37.3 3
SFO 75 15:55:43.4 -54:39:07 115.0 443 247 479 1
SFO 82a 16:47:22.1 -41:13:06 3.0a 12.3 3.0a 36.7 1
SFO 82b 16:47:19.4 -41:15:43 5.1 23.2 6.7 63.6 1
SFO 84 16:53:51.9 -40:08:09 ...b 11.7 ...b 28.6 1
SFO 85a 16:59:04.0 -42:41:46 40.3b <201 40.3a <201 3
SFO 85b 16:59:12.0 -42:43:15 67.4 <201 97.2 <201 4
SFO 89 18:09:48.9 -24:04:56 63.2 102 28.6 369 1
a Source is unresolved at this wavelength
b In the cleaned 13 cm image SFO 84 lies in an area affected by a striping artefact caused by the cleaning process.
It is not possible to set a sensible flux limit for this source at 13 cm.


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