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Table A.1.

Our observations with detection (top part of the table, tagged with “Our observations”) and proto-cluster members information given from the literature and used in our analysis (bottom part of the table, tagged with “Proto-cluster members from the literature”).

Our observations
ID Name RA (J2000) (h m s) Dec (J2000) (° ′ ″) Redshifta (this work) Lines (this work) Redshifta (G 10) Lines (G 10) Notesb
Protocluster members
slit1 AGN1110 17:56:52.56 65:16:56.65 1.4148 ± 0.0001 (Bc) Hα 1.3935 ± 0.0012 (B) [O II]3727 AGN
slit2 AGN1317 17:56:55.76 65:19:07.00 1.4147 ± 0.0010 (Ac) Hα, Hβ, [O III]4959, 5007, [N II]6549, 6583 1.4162 ± 0.0005 (A) [Ne V]3426, [O II]3727 AGN
slit3a AGN1354 17:57:05.28 65:19:53.62 1.4177 ± 0.0009 (Ac) Hα, Hβ, [N II]6583 1.4153 ± 0.0003 (B) Mg II 2800 AGN
slit3b 7C 1756+6520 17:57:05.48 65:19:53.75 1.4152 ± 0.0009 (Ac) Hα, Hβ 1.4150 ± 0.0001 (A) [Ne V]3426, [O II]3727, [Ne III]3869 HzRG, AGN
slit5 CMC 1 17:56:58.12 65:18:18.09 1.4055 ± 0.0047 (Ac) Hβ, [O III]5007

Possible protocluster members
slit4 CMC 2 17:56:56.84 65:18:10.29 1.4079 ± 0.0004 (Bc) [O III]5007 Galaxy
slit6 CMC 3 17:56:53.19 65:17:47.93 1.4067 ± 0.0002 (Bc) [O III]5007 Galaxy
slit7 CMC 4 17:56:51.86 65:17:38.91 1.3845 ± 0.0001 (Bc) [O III]5007 Galaxy
slit8 CMC 5 17:56:46.60 65:17:49.40 1.4039 ± 0.0002 (Bc) [O III]5007 Galaxy
slit12 CMC 6 17:57:08.25 65:18:49.88 1.3950 ± 0.0001 (Bc) [O III]5007 Galaxy
slit14 CMC 7 17:57:00.34 65:19:09.47 1.4233 ± 0.0001 (Bc) Hβ Galaxy
slit16 CMC 8 17:56:48.46 65:17:05.60 1.3999 ± 0.0001 (Bc) [O III]5007 Galaxy
slit17 CMC 9 17:57:09.17 65:19:52.75 1.4336 ± 0.0001 (Bc) [O III]5007 Galaxy

Non protocluster members
slit9 CMC 10 17:57:08.56 65:19:00.29 1.3683 ± 0.0001 (B) Hβ Galaxy
slit18 CMC 11 17:56:57.60 65:18:34.43 1.3673 ± 0.0001 (B) Hβ Galaxy
Protocluster members from the literature
ID Name RA (J2000) (h m s) Dec (J2000) (° ′ ″) Redshiftd Linesc Ref.
Cl 1756.2 sBzK.6355 17:57:59.55 65:18:00.64 1.4020 ± 0:0001 (A) [O II] G 10 Galaxy
Cl 1756.3 sBzK.9622 17:57:21.75 65:23:05.04 1.4064 ± 0:0005 (A) [O II] G 10 Galaxy
Cl 1756.4 sBzK.7556c 17:57:46.54 65:20:00.48 1.4081 ± 0:0007 (A) Broad Mg II, [O II] G 10 AGN
Cl 1756.5 pBzK.5858 17:57:44.40 65:17:14.30 1.4110 ± 0:0010 (B) [O II] G 10 Galaxy
Cl 1756.6 serendip.1 17:56:57.67 65:18:49.45 1.4150 ± 0:0005 (A) [O II] G 10 Galaxy
Cl 1756.8 serendip.2 17:57:25.00 65:19:04.83 1.4157 ± 0:0010 (A) [O II] G 10 Galaxy
Cl 1756.9 sBzK.6997 17:57:24.43 65:19:03.87 1.4157 ± 0:0006 (A) [O II] G 10 Galaxy
Cl 1756.11 sBzK.7624 17:56:33.16 65:20:04.46 1.4236 ± 0:0001 (A) Fe II+Mg II absn, [O II] G 10 Galaxy
Cl 1756.12 pBzK.7523 17:57:05.04 65:19:54.50 1.4244 ± 0:0004 (A) [O II] G 10 Galaxy
Cl 1756.13 sBzK.5860c 17:57:35.34 65:17:14.39 1.4268 ± 0:0005 (A) Broad Mg II, [O II] G 10 AGN
Cl 1756.14 sBzK.5699 17:57:44.06 65:16:57.11 1.4274 ± 0:0004 (A) [O II] G 10 Galaxy
Cl 1756.15 pBzK.10235 17:57:25.20 65:23:58.19 1.4277 ± 0:0010 (B) [O II] G 10 Galaxy
Cl 1756.16 sBzK.4449 17:57:47.40 65:14:52.17 1.4326 ± 0:0002 (A) [O II] G 10 Galaxy
Cl 1756.17 sBzK.7625 17:57:14.41 65:20:02.40 1.4366 ± 0:0001 (A) [O II] G 10 Galaxy
Cl 1756.18 AGN.1206 17:57:13.08 65:19:08.37 1.4371 ± 0:0002 (A) [O II] G 10 AGN
Cl 1756.19 sBzK.7208 17:57:18.31 65:19:24.94 1.4374 ± 0:0002 (A) [O II] G 10 Galaxy
Cl 1756.20 serendip.3 17:57:20.76 65:19:39.14 1.4379 ± 0:0007 (A) [O II] G 10 Galaxy
MSC2 17:57:10.16 65:19:28.09 1.4556 ± 0:0005 (A) Hα, [N II] M 12 Galaxy

Notes.

(a)

The assignment of the quality flags to the redshifts is the same as was adopted by G10 and M12. We also adopted the flag “c” for the redshifts corresponding to galaxies belonging to the protocluster. The flag “c” is not present for the redshifts from G10 and M12, although the galaxies from G10 and M12 are all defined as protocluster members.

(b)

Spectroscopic classification, AGN vs. galaxy, based on spectra acquired so far.

(c)

sBzK.7556 and sBzK.5860 from G10, both targeted as sBzK galaxies, are classified as AGN because their spectra show AGN signatures such as strong, broad Mg II emission lines.

(d)

Redshifts derived from G10 based on [O II] and with quality flag “A” mean that the [O II]λ 3727Å emission has been clearly detected as a doublet.

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