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Table 1:

Spectroscopic members of the structure around 7C 1756+6520.
ID Namea RA Dec $z_{\rm spec}$ Qb Bc zc Kc Notes
    (J2000) (J2000)     (AB) (AB) (AB)  
Cl 1756.1 AGN.1110 17:56:52.56 65:16:56.65 $1.3935\pm0.0012$ B 23.21 22.14 20.89 B2900, B3260, [OII]
Cl 1756.2 sBzK.6355 17:57:59.55 65:18:00.64 $1.4020\pm0.0001$ A 24.36 23.34 21.54 [OII]
Cl 1756.3 sBzK.9622 17:57:21.75 65:23:05.04 $1.4064\pm0.0005$ A 24.00 22.78 20.38 [OII]
Cl 1756.4 sBzK.7556 17:57:46.54 65:20:00.48 $1.4081\pm0.0007$ A 20.97 20.77 20.35 AGN: broad MgII, [OII]
Cl 1756.5 pBzK.5858 17:57:44.40 65:17:14.30 $1.4110\pm0.0010$ B >27.1 23.80 21.62 [OII]; ID31 in G09
Cl 1756.6 serendip.1 17:56:57.67 65:18:49.45 $1.4150\pm0.0005$ A - - - [OII]
Cl 1756.7d AGN.1354 17:57:04.98 65:19:51.00 $1.4153\pm0.0003$ B 26.34 22.03 - AGN: broad MgII
HzRG 7C 1756+6520 17:57:05.48 65:19:53.75 $1.4156\pm0.0001$ A >27.1 21.40 20.17 AGN: [NeV], [OII], [NeIII]
Cl 1756.8 serendip.2 17:57:25.00 65:19:04.83 $1.4157\pm0.0010$ A 26.32 24.34 >23.4 [OII]
Cl 1756.9 sBzK.6997 17:57:24.43 65:19:03.87 $1.4157\pm0.0006$ A 25.21 24.21 22.56 [OII]
Cl 1756.10 AGN.1317 17:56:55.75 65:19:07.00 $1.4162\pm0.0005$ A 20.16 19.46 19.01 AGN: broad MgII, [NeV], [OII]
Cl 1756.11 sBzK.7624 17:56:33.16 65:20:04.46 $1.4236\pm0.0001$ A 22.51 22.39 21.30 FeII+MgII absn, [OII ]
Cl 1756.12e pBzK.7523 17:57:05.04 65:19:54.50 $1.4244\pm0.0004$ A >27.1 23.47 21.31 [OII]; ID43 in G09
Cl 1756.13 sBzK.5860 17:57:35.34 65:17:14.39 $1.4268\pm0.0005$ A 22.96 22.35 21.31 AGN: broad MgII, [OII]
Cl 1756.14 sBzK.5699 17:57:44.06 65:16:57.11 $1.4274\pm0.0004$ A 25.89 24.20 22.71 [OII]
Cl 1756.15 pBzK.10235 17:57:25.20 65:23:58.19 $1.4277\pm0.0010$ B >27.1 23.45 21.76 [OII]; ID63 in G09
Cl 1756.16 sBzK.4449 17:57:47.40 65:14:52.17 $1.4326\pm0.0002$ A 24.93 23.89 23.02 [OII]
Cl 1756.17 sBzK.7625 17:57:14.41 65:20:02.40 $1.4366\pm0.0001$ A >27.1 24.46 22.95 [OII]
Cl 1756.18 AGN.1206 17:57:13.08 65:19:08.37 $1.4371\pm0.0002$ A >27.1 >25.0 21.49 [OII]
Cl 1756.19 sBzK.7208 17:57:18.31 65:19:24.94 $1.4374\pm0.0002$ A 24.93 23.46 22.00 [OII]
Cl 1756.20 serendip.3 17:57:20.76 65:19:39.14 $1.4379\pm0.0007$ A 25.29 23.18 21.50 [OII]

Notes. (a) The names are composed of the selection technique for the source - AGN, sBzK or pBzK ($\equiv$pBzK* here) - followed by the identification number in our K-band ($3.6~\mu$m) catalogue for BzK (AGN) targets. Sources serendipitously identified are given a simple ``serendip.'' designation. (b) Q indicates the quality of the redshift, either ``A'' indicating a highly certain redshift, or ``B'' indicating a high level of confidence (see Sect. 3.2). (c) Magnitudes were derived using SExtractor MAG_AUTO and are therefore slightly different from the aperture magnitudes used to derive colours for candidate selection. (d) AGN found within $6\hbox{$^{\prime\prime}$ }$ of 7C 1756+6520. No accurate magnitude is available in K due to an artifact caused by a bright star in the near-infrared data. See Fig. 12 in G09. (e) pBzK* galaxy found within $3\hbox{$^{\prime\prime}$ }$ of 7C 1756+6520.


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