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Table 2:

Other spectroscopic redshifts.
Namea RA Dec $z_{\rm spec}$ Qb Bc zc Kc Notes
  (J2000) (J2000)     (AB) (AB) (AB)  
sBzK.8902 17:57:15.84 65:22:04.07 $0.3347\pm0.0005$ B 24.28 22.93 21.88 [OIII]
AGN.1005 17:57:05.48 65:19:53.75 $0.3658\pm0.0001$ A 22.25 19.51 18.78 CaHK, H$\beta$, H$\alpha$, [NII]
sBzK.4858 17:57:48.87 65:15:31.59 $0.4265\pm0.0001$ A 24.18 22.85 22.14 H$\beta$, [OIII], H$\alpha$
sBzK.9364 17:57:29.28 65:22:42.61 $0.5318\pm0.0008$ B >27.1 23.62 21.06 [OIII]
sBzK.7895 17:57:05.04 65:20:31.57 $0.7529\pm0.0003$ A 22.70 21.75 20.94 [OII], H$\beta$
sBzK.6858 17:56:58.08 65:18:50.05 $0.7533\pm0.0004$ B 23.06 23.11 21.02 [OII]
sBzK.7921 17:56:39.84 65:20:30.52 $1.0196\pm0.0001$ A 22.73 23.67 22.79 [OII], [NeIII]
sBzK.11226 17:57:19.44 65:25:24.60 $1.0505\pm0.0002$ A 24.45 23.83 23.19 [OII], [NeIII], H$\beta$
sBzK.9844 17:57:16.38 65:23:19.85 $1.1227\pm0.0005$ A 26.00 24.18 21.99 [OII]
pBzK.7866 17:56:42.72 65:20:27.97 $1.1825\pm0.0010$ B >27.1 23.11 20.93 [OII]
AGN.1767 17:57:15.33 65:21:56.14 $1.1827\pm0.0004$ A >27.1 >25.0 19.58 MgII, [OII]
sBzK.9430 17:55:53.37 65:22:48.02 $1.2074\pm0.0001$ A 23.44 22.79 21.73 AGN: MgII absn, [OII], [NeIII], H$\zeta$, H$\delta$,
pBzK.7359 17:57:12.44 65:19:45.10 $1.2122\pm0.0002$ A 26.65 22.63 20.18 [OII]
pBzK.4948 17:57:16.54 65:15:44.17 $1.2130\pm0.0003$ A >27.1 22.79 20.49 [OII]
sBzK.11168 17:56:57.97 65:25:20.26 $1.2359\pm0.0001$ A 25.46 23.93 22.37 [OII]
sBzK.12407 17:56:56.58 65:26:36.42 $1.2461\pm0.0001$ A 25.02 24.33 22.99 [OII]
sBzK.8631 17:56:31.31 65:21:41.17 $1.2586\pm0.0002$ A 23.90 23.06 21.36 [OII]
pBzK.10254 17:57:11.04 65:23:56.76 $1.2598\pm0.0001$ A >27.1 23.40 21.20 [NeV], [OII], [NeIII]
sBzK.2137 17:56:52.56 65:11:09.95 $1.2830\pm0.0001$ A 24.09 23.96 22.61 H$\beta$, [OIII], [NII]
sBzK.8410 17:57:25.15 65:21:18.01 $1.4564\pm0.0003$ A 25.37 23.75 21.90 [OII]
sBzK.7159 17:57:28.56 65:19:17.93 $1.4576\pm0.0002$ A 24.70 23.05 22.44 [OII]
sBzK.6886 17:57:37.75 65:18:53.95 $1.4663\pm0.0004$ A 25.82 23.25 21.70 [OII]
sBzK.8761 17:56:57.03 65:21:53.86 $1.4764\pm0.0003$ A 23.35 22.83 20.37 [OII]
sBzK.8799 17:57:11.43 65:21:53.94 $1.5589\pm0.0001$ A 23.59 22.26 21.14 CIII], MgII abns, [OII]
sBzK.2998 17:56:56.40 65:12:32.76 $1.5620\pm0.0004$ A 24.19 23.79 22.88 [OII]
sBzK.9006 17:56:28.73 65:22:10.94 $1.5943\pm0.0002$ A 22.95 22.84 22.27 [OII]
sBzK.9788 17:55:49.35 65:23:16.14 $1.595\pm0.001$ A 23.93 22.98 22.18 FeII+MgII absn
sBzK.11725 17:56:30.31 65:25:31.69 $1.725\pm0.005$ B 22.35 21.78 21.00 AGN: broad MgII
sBzK.5102 17:57:57.61 65:15:55.59 $1.979\pm0.002$ A 23.59 22.84 22.21 AlII, MgII
sBzK.6330 17:57:37.08 65:17:58.83 $2.218\pm0.001$ A 23.82 23.23 21.94 AGN: CIV, CIII], MgII
sBzK.3534 17:58:01.74 65:13:31.73 $2.256\pm0.002$ A 23.73 22.84 21.82 CIV+AlII absn
AGN.1748 17:57:20.07 65:21:56.96 $2.399\pm0.001$ A 23.06 21.39 20.58 Quasar: CIV, CIII]
AGN.1340 17:57:30.88 65:21:22.32 $2.402\pm0.001$ A 24.05 21.80 19.44 Quasar: CIV, CIII]
sBzK.3718 17:58:01.19 65:13:49.25 $2.4020\pm0.0005$ A 22.65 21.75 21.76 CIV+AlII absn
AGN.1213 17:57:33.22 65:20:26.24 $3.702\pm0.002$ A 22.73 19.72 18.95 Quasar: Ly$\alpha$, CIV, CIII]

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. (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.


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