Table 1.
Spectroscopically confirmed overdensity members.
| ID | RA | Dec | KAB | zspec | Notes |
|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) |
| m1 | 10:30:27.73 | +05:24:52.3 | 23.97 ± 0.45 | 1.6960 ± 0.0005 | arc |
| m2 | 10:30:26.46 | +05:24:42.4 | 23.14 ± 0.23 | 1.6967 ± 0.0004 | arc |
| m3 | 10:30:26.34 | +05:24:40.5 | 22.21 ± 0.14 | 1.6967 ± 0.0002 | arc |
| m4 | 10:30:26.31 | +05:24:37.4 | 22.67 ± 0.28 | 1.6966 ± 0.0003 | arc |
| m5 | 10:30:25.26 | +05:24:47.6 | 23.34 ± 0.34 | 1.6949 ± 0.0004 | – |
| m6 | 10:30:26.42 | +05:25:07.1 | 22.12 ± 0.21 | 1.6871 ± 0.0003 | – |
| l1 | 10:30:25.20 | +05:24:28.4 | 20.90 ± 0.12 | 1.6987 ± 0.0002 | FRII |
| l2 | 10:30:20.56 | +05:23:28.7 | 22.92 ± 0.30 | 1.6966 ± 0.0004 | – |
Notes. Columns: (1) Source+redshift identifier: m* and l* refer to measurements by MUSE and LUCI, respectively; (2) and (3) source coordinates from either MUSE or LBT/LBC z-band data; (4) K-band magnitude from the MUSYC-deep catalog (Quadri et al. 2007). For m1, l1 and l2 we manually performed K-band photometry on the MUSYC-deep image. (5) Redshift and 1σ error; (6) Notes: Galaxies distributed in the arc-like shape at the edge of component A of the diffuse X-ray emission (see text) are labeled “arc”.
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