Table 2.
Known background and cluster member radio galaxies listed with their corresponding redshift.
| T1 | zspec = 0.0954 | M | (1) | ||||||
| T2 | zspec = 0.0895 | M | (1) | ||||||
| W1 | zphot = 0.5740 | B | (2) | ||||||
| W2 | / | B | (*) | ||||||
| Group G | zspec = 0.0940 | B | (3) | ||||||
| Group C | / | M | (*) | ||||||
| FR II | zphot = 0.8560 | B | (4) |
Notes. M: cluster member; B: background; (*) for these sources the redshift is not known, but according to Venturi et al. (2017), W2 is not a cluster member, whereas Group C is associated with other cluster galaxies with similar optical magnitude.
References: (1) Ahumada et al. (2020); (2) Venturi et al. (2017); (3) Eckert et al. (2014); (4) Duncan (2022).
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