Table 4

Radio sources with optical counterparts that have redshifts 0.35 <zphot< 0.50 within the area containing the studied overdense structures.

ID RA Dec Speak zphot L3 GHz gr Overdense structure ID
[h m s] [d m s] [μJy beam-1] [× 1022 W/Hz]
(1) (2) (3) (4) (5) (6) (7) (8)

114 02 11 31.27 –06 14 16.84 59.5 ± 9.5 0.41 3.2 ± 0.5 1.09 ...
75 02 10 57.88 –06 14 00.62 287.0 ± 10.8 0.41 16.1 ± 0.6 1.56 VTA02
115 02 11 32.15 –06 12 49.11 74.5 ± 8.7 0.40 3.9 ± 0.4 1.62 XLSSC 085
72 02 10 56.76 –06 11 58.37 72.2 ± 9.7 0.41 4.0 ± 0.5 1.59 XLSSC 083
87 02 11 08.73 –06 10 10.38 66.6 ± 10.5 0.49 5.5 ± 0.8 1.02 XLSSC 086
93 02 11 13.86 –06 09 39.96 74.9 ± 10.8 0.40 4.0 ± 0.5 1.28 XLSSC 086
137 02 11 48.62 –06 13 27.91 80.6 ± 11.7 0.42 4.6 ± 0.6 0.71 VTA07
134 02 11 46.09 –06 16 36.59 91.7 ± 12.0 0.50 7.9 ± 1.0 1.50 ...

Notes. Sources unassociated with a cluster/group candidate are marked by ellipsis. Source identifiers from the VLA-XXL-N 3 GHz radio catalogue are given in Cols. (1), Col. (2) gives the right ascension (RA) of the source in hours, minutes, and seconds, Col. (3) gives the declination (Dec) of the source in degrees, arcminutes and arcseconds. Peak surface brightness is given in Col. (4) in units of μJy beam-1. Photometric redshifts of optical counterparts of radio sources are given in Col. (5). Radio luminosities at 3 GHz are given in Col. (6) in units of W/Hz, and are divided by 1022. Column (7) provides gr optical colour. If a source is associated with an overdense structure, Col. (8) gives the ID of the source.

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