Table C.1
3CRR catalog (extract).
| Object name (1) |
RA (J2000) [h:m:s] (2) |
Dec (J2000) [d:m:s] (3) |
z (4) |
S58 MHz [Jy] (5) |
σs [Jy] (6) |
Resolution [″ × ″] (7) |
σrms [mJy beam−1] (8) |
S144 MHz [Jy] (9) |
 (10) |
|---|---|---|---|---|---|---|---|---|---|
| 3C 6.1 | 0:16:31.23 | +79:16:50.38 | 0.840 | 31.0 | 3.1 | 13.8 × 10.5 | 9.2 | ||
| 3C 9 | 0:20:25.22 | +15:40:54.80 | 2.020 | 50.2 | 5.0 | 15.6 × 9.7 | 10.3 | 18.6 | 1.08 |
| 3C 13 | 0:34:14.56 | +39:24:16.67 | 1.351 | 33.1 | 3.3 | 14.1 × 8.3 | 10.4 | 14.5 | 0.91 |
| 3C 14 | 0:36:06.44 | +18:37:59.12 | 1.469 | 31.2 | 3.1 | 16.0 × 9.6 | 8.7 | 13.6 | 0.91 |
| 3C 16 | 0:37:44.57 | +13:19:54.98 | 0.406 | 31.2 | 3.1 | 20.6 × 9.6 | 15.3 | 12.6 | 0.99 |
| 3C 19 | 0:40:55.02 | +33:10:07.32 | 0.482 | 27.5 | 2.8 | 11.1 × 6.0 | 13.7 | 9.6 | 1.15 |
| 3C 20 | 0:43:09.18 | +52:03:36.11 | 0.174 | 86.5 | 8.6 | 13.9 × 9.4 | 9.0 | 46.8 | 0.67 |
| 3C 22 | 0:50:56.22 | +51:12:03.42 | 0.936 | 59.5 | 6.0 | 12.6 × 8.4 | 15.0 | 16.6 | 1.40 |
| 3C 28 | 0:55:50.61 | +26:24:37.48 | 0.195 | 64.3 | 6.4 | 13.6 × 8.7 | 8.8 | 22.6 | 1.14 |
| 3C 31 | 1:07:24.97 | +32:24:45.11 | 0.017 | 43.7 | 4.4 | 26.1 × 16.5 | 10.5 | 22.5 | 0.73 |
| 3C 33 | 1:08:52.87 | +13:20:14.35 | 0.061 | 127.1 | 12.7 | 15.2 × 9.9 | 13.4 | 52.8 | 0.96 |
| 3C 33.1 | 1:09:44.27 | +73:11:57.34 | 0.181 | 44.4 | 4.4 | 14.1 × 12.1 | 10.0 | 24.6 | 0.64 |
| 3C 34 | 1:10:18.67 | +31:47:20.47 | 0.690 | 42.8 | 4.3 | 15.3 × 8.8 | 8.5 | 15.2 | 1.14 |
| 3C 223 | 9:39:52.76 | +35:53:58.96 | 0.137 | 41.0 | 4.1 | 14.5 × 14.5 | 10.5 | 20.1 | 0.78 |
| 3C 225b | 9:42:15.35 | +13:45:49.57 | 0.583 | 55.6 | 5.6 | 31.6 × 8.2 | 14.1 | 17.9 | 1.24 |
| 3C 274a | 12:30:49.42 | +12:23:28.03 | 0.0043 | 2443.0 | 244.3 | 20.2 × 8.0 | 27.5 |
Notes. Illustrative selection of the summary of the entire catalog from this work. (4) The redshift of the object taken from the NASA Extragalactic Database, (5) Measured integrated flux density in Jy on the SH flux scale, (6) 10% total uncertainty on the flux estimate, (7) Resolution of the produced total brightness maps, (8) rms noise of those maps, (9) Dynamic range of final image defined as the ratio of the peak flux to the lowest pixel value, (10) estimated angular size of the sources in our data & (11) integrated spectral index of the source fitted from a power law. (a)Also known as Virgo A or M87
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