Table 1
Summarised characteristics of our sample.
Name | z | Ref. | RA | Dec | Morph. peculiarities | Radio jet axis | log L3 GHz | Polarisation | Ref. |
spec. | [J2000] | [J2000] | [W Hz-1] | [%] | |||||
|
|||||||||
3C 368 | 1.132 | a | 18:05:06.37 | +11:01:33.1 | two components | aligned | 27.63 | 7.6 ± 0.9 (V) | g |
3C 470 | 1.653 | b | 23:58:36.00 | +44:04:45.0 | two components | misaligned | 28.24 | ... | ... |
MRC 0324-228 | 1.894 | c | 03:27:04.54 | −22:39:42.1 | one close companion | ... | 28.49 | ![]() |
h |
PKS 1138-262 | 2.156 | c | 11:40:48.38 | −26:29:08.8 | multiple companions | aligned | 28.14 | ... | ... |
MRC 0406-244 | 2.427 | d | 04:08:51.46 | −24:18:16.4 | multiple components | aligned | 28.11 | ![]() |
h |
MRC 2104-242 | 2.491 | e | 21:06:58.28 | −24:05:09.1 | two components | misaligned | 27.88 | ... | ... |
USS 0828+193 | 2.572 | c | 08:30:53.42 | +19:13:15.7 | multiple components | aligned | 27.47 | 10.0± 2.0 (spec) | i |
4C 28.58 | 2.891 | c | 23:51:59.20 | +29:10:29.0 | multiple components | aligned | 27.89 | ... | ... |
USS 0943-242 | 2.923 | c | 09:45:32.73 | −24:28:49.7 | one close companion | aligned | 27.95 | 6.6 ± 0.9 (spec) | i |
4C 41.17a | 3.792 | c | 06:50:52.23 | +41:30:30.1 | multiple components | aligned | 28.17 | <2.4 (spec) | j |
TN J2007-1316a | 3.840 | f | 20:07:53.26 | −13:16:43.6 | one close companion | ... | 27.79 | ~3 (spec) | k |
Notes. Columns 2 and 3 indicate the spectroscopically confirmed redshifts and their references. Column 6 refers to morphological peculiarities at optical/NIR wavelengths: companion: source close to the object identified as the radio galaxy (few arcsecond) and components: potential substructures when detected in the images. Column 7 indicates the alignment of the radio jet axis compared to the optical/NIR extension when detectable in the images. Column 8 lists the restframe 3GHz luminosity from De Breuck et al. (2010). The penultimate column indicates the polarisation and the band.
Reference. (a) Meisenheimer & Hippelein (1992); (b) Hewitt & Burbidge (1991); (c) Roettgering et al. (1997); (d) McCarthy et al. (1996); (e) McCarthy et al. (1990); (f) Bornancini et al. (2007); (g) di Serego Alighieri et al. (1989); (h) Buchard (2008); (i) Vernet et al. (2001); (j) Dey et al. (1995); (k) Rocca-Volmerange et al. (2013).
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