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Table 1

Positions, magnitudes at optical (MegaCam), NIR (WIRCam) and MIR (IRAC) wavelengths, and spectroscopic redshifts of the 13 galaxies followed-up with VLT/X-Shooter.

ID RA Dec g i J H K s IRAC IRAC z spec
3.6 μm 4.5 μm

A1 00:00:42.0 01:26:40.2 24.91 ± 0.20 23.39 ± 0.15 21.94 ± 0.04 21.34 ± 0.04 20.92 ± 0.04 20.25 ± 0.04 19.99 ± 0.04 1.677
A2 00:00:42.4 01:26:26.7 24.67 ± 0.15 23.78 ± 0.18 22.08 ± 0.05 21.33 ± 0.04 20.88 ± 0.04 20.13 ± 0.03 19.78 ± 0.03 1.684
B2a 00:00:42.1 01:25:32.1 27.15 ± 1.44 ... 22.71 ± 0.09 22.36 ± 0.09 22.35 ± 0.15 21.54 ± 0.05 21.49 ± 0.08 1.681

A3 00:00:41.8 01:26:21.5 27.44 ± 2.00 24.01 ± 0.23 21.76 ± 0.04 21.28 ± 0.04 21.14 ± 0.05 20.69 ± 0.04 20.54 ± 0.04 2.019
A4a 00:00:42.8 01:26:27.0 24.45 ± 0.13 23.67 ± 0.17 21.98 ± 0.05 21.44 ± 0.04 21.08 ± 0.05 20.32 ± 0.04 20.11 ± 0.04 2.032
B2ca 00:00:41.9 01:25:29.3 25.43 ± 0.30 24.41 ± 0.33 22.51 ± 0.07 21.98 ± 0.06 21.70 ± 0.08 20.69 ± 0.04 20.39 ± 0.04 2.029
C1ab 00:00:44.8 01:26:17.7 24.75 ± 0.16 23.16 ± 0.11 21.23 ± 0.03 20.57 ± 0.02 20.08 ± 0.03 19.25 ± 0.03 18.80 ± 0.03 2.039
C1bb 00:00:44.8 01:26:16.7 24.75 ± 0.16 23.16 ± 0.11 21.23 ± 0.03 20.57 ± 0.02 20.08 ± 0.03 19.25 ± 0.03 18.80 ± 0.03 2.039
D1 00:00:45.0 01:25:36.5 25.56 ± 0.36 24.53 ± 0.40 22.46 ± 0.07 21.78 ± 0.06 21.41 ± 0.07 20.48 ± 0.04 20.31 ± 0.04 2.018

A4c 00:00:43.1 01:26:31.3 22.48 ± 0.03 20.97 ± 0.02 20.43 ± 0.02 20.09 ± 0.02 19.88 ± 0.02 20.08 ± 0.03 20.49 ± 0.04 1.615
A5 00:00:41.9 01:26:13.1 24.85 ± 0.18 24.58 ± 0.40 23.50 ± 0.17 22.20 ± 0.08 22.33 ± 0.13 21.47 ± 0.05 21.36 ± 0.06 2.121
B2ba 00:00:41.9 01:25:29.3 25.43 ± 0.30 24.41 ± 0.33 22.51 ± 0.07 21.98 ± 0.06 21.70 ± 0.08 20.69 ± 0.04 20.39 ± 0.04 1.921
B3 00:00:43.0 01:26:00.3 24.12 ± 0.09 23.47 ± 0.13 22.02 ± 0.05 21.56 ± 0.04 21.23 ± 0.05 20.68 ± 0.04 20.45 ± 0.04 1.976

Notes. All magnitudes are expressed in the AB system. For clarity, the table contains three groups: members of the structure at z ≃ 1.7, members of the structure at z ≃ 2.0, and non-members of either group (and, in all cases, ordered from lower to higher redshift).

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