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Table 1.

Main properties of the HzRGs sample and observation log.

Name RA Dec z Program Exp. time (s) Reference P500
NVSS J213238-335318 21:32:39.0 −33:53:19 2.900 60.A-9334(A) 6510 28.60
MRC 0943-242 09:45:32.8 −24:28:50 2.922 096.B-0752(A) 15 146 Wang23 28.62
NVSS J151020-352803 15:10:20.8 −35:28:03 2.937 108.22FU.001 5226 This work 28.35
TXS 0952-217 09:54:29.5 −21:56:53 2.950 108.22FU.001 2607 This work 28.08
TN J1112-2948 11:12:23.9 −29:48:06 3.090 108.22FU.001 2595 This work 28.76
NVSS J095751-213321 09:57:51.3 −21:33:21 3.126 108.22FU.001 2605 This work 28.11
MRC 0316-257 03:18:12.1 −25:35:10 3.142 094.B-0699(A) 15 264 Wang23 28.95
MRC 0251-273 02:53:16.7 −27:09:10 3.160 108.22FU.001 2589 This work 28.54
NVSS J230123-364656 23:01:23.5 −36:46:56 3.220 not observed 28.34
NVSS J232100-360223 23:21:00.6 −36:02:25 3.320 not observed 28.22
NVSS J094724-210505 09:47:24.5 −21:05:06 3.377 108.22FU.001 2583 This work 27.43
NVSS J095438-210425 09:54:38.4 −21:04:25 3.431 108.22FU.001 2607 This work 28.13
NVSS J231402-372925 23:14:02.4 −37:29:27 3.450 not observed 28.83
TN J0205+2242 02:05:10.7 +22:42:50 3.506 096.B-0752(B) 15 264 Wang23 28.46
TN J0121+1320 01:21:42.7 +13:20:58 3.517 097.B-0323(C) 19 088 Wang23 28.49
4C+03.24 (4C 1243+036) 12:45:38.4 +03:23:20 3.560 60.A-9100(G) 4500 Wang23 29.23
MG 2141+192 (4C +19.71) 21:44:07.5 +19:29:15 3.592 097.B-0323(B) 20 984 Wang23 29.08
TN J1049-1258 10:49:06.2 −12:58:19 3.697 108.22FU.001 2601 This work 28.94
TN J2007-1316 20:07:53.2 −13:16:44 3.837 not observed 29.13
NVSS J231727-352606 23:17:27.4 −35:26:07 3.874 not observed 28.71
NVSS J021308-322338 02:13:08.0 −32:23:40 3.976 108.22FU.001 2596 This work 28.40
TN J1338-1942 13:38:26.1 −19:42:30 4.105 60.A-9100(B) 24 840 Wang23 28.70
TN J1123-2154 11:23:10.2 −21:54:05 4.109 108.22FU.001 3929 This work 28.45
RC J0311+0507 4C 04.11 03:11:48.0 +05:08:03 4.514 096.B-0752(F) 15 264 Wang23 29.49
TN J0924-2201 09:24:19.9 −22:01:42 5.197 108.22FU.001 2610 This work 28.94

Notes. List of the 25 HzRGs in Miley & De Breuck (2008) with z>2.9 and δ<25° in order of increasing redshift. We report their coordinates and redshifts, the program of MUSE observations, the exposure time, and the reference in which the data are published. The last column includes the logarithm of radio luminosity at the rest frame frequency of 500 MHz, also taken from Miley & De Breuck (2008).

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