\begin{table}%t2
\caption{\label{others}Other spectroscopic redshifts.}
%\centering
\par
\begin{tabular}{l l l c l c c c l}
\hline\hline
Name\tablefootmark{a}	& RA		& Dec	&$z_{\rm spec}$&Q\tablefootmark{b}&$B$\tablefootmark{c}&	$z$\tablefootmark{c}	&	$K$\tablefootmark{c}	&	Notes	\\
			& (J2000)	& (J2000)	&		&		&	(AB)	&	(AB)	&	(AB)	&		\\
\hline
s$BzK$.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]		\\  
s$BzK$.4858		& 17:57:48.87	& 65:15:31.59	&	$0.4265\pm0.0001$	&	A	&	$24.18$	&	$22.85$	&	$22.14$	&	H$\beta$, [OIII], H$\alpha$		\\  	
s$BzK$.9364		& 17:57:29.28	& 65:22:42.61	&	$0.5318\pm0.0008$	&	B	&	$>$$27.1$	&	$23.62$	&	$21.06$	&	[OIII]				\\ 
s$BzK$.7895		& 17:57:05.04	& 65:20:31.57	&	$0.7529\pm0.0003$	&	A	&	$22.70$	&	$21.75$	&	$20.94$	&	[OII], H$\beta$		\\ 	
s$BzK$.6858		& 17:56:58.08	& 65:18:50.05	&	$0.7533\pm0.0004$	&	B	&	$23.06$	&	$23.11$	&	$21.02$	&	[OII]				\\  
s$BzK$.7921		& 17:56:39.84	& 65:20:30.52	&	$1.0196\pm0.0001$	&	A	&	$22.73$	&	$23.67$	&	$22.79$	&	[OII], [NeIII]		\\  
s$BzK$.11226		& 17:57:19.44	& 65:25:24.60	&	$1.0505\pm0.0002$	&	A	&	$24.45$	&	$23.83$	&	$23.19$	&	[OII], [NeIII], H$\beta$\\  	
s$BzK$.9844		& 17:57:16.38  	& 65:23:19.85	&	$1.1227\pm0.0005$	&	A	&	$26.00$	&	$24.18$	&	$21.99$	&	[OII]				\\  
p$BzK$.7866		& 17:56:42.72	& 65:20:27.97	&	$1.1825\pm0.0010$	&	B	&	$>$$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]		\\  
s$BzK$.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$\delta$, \\  
p$BzK$.7359		& 17:57:12.44	& 65:19:45.10	&	$1.2122\pm0.0002$	&	A	&	$26.65$	&	$22.63$	&	$20.18$	&	[OII]			\\  
p$BzK$.4948		& 17:57:16.54	& 65:15:44.17 	&	$1.2130\pm0.0003$	&	A	&	$>$$27.1$	&	$22.79$	&	$20.49$	&	[OII]			\\  	 
s$BzK$.11168		& 17:56:57.97  	& 65:25:20.26	&	$1.2359\pm0.0001$	&	A	&	$25.46$	&	$23.93$	&	$22.37$	&	[OII]			\\  
s$BzK$.12407		& 17:56:56.58  	& 65:26:36.42	&	$1.2461\pm0.0001$	&	A	&	$25.02$	&	$24.33$	&	$22.99$	&	[OII]			\\  	
s$BzK$.8631		& 17:56:31.31	& 65:21:41.17	&	$1.2586\pm0.0002$	&	A	&	$23.90$	&	$23.06$	&	$21.36$	& 	[OII]				\\  	
p$BzK$.10254		& 17:57:11.04	& 65:23:56.76	&	$1.2598\pm0.0001$	&	A	&	$>$$27.1$	&	$23.40$	&	$21.20$	&	[NeV], [OII], [NeIII]	\\  
s$BzK$.2137		& 17:56:52.56	& 65:11:09.95	&	$1.2830\pm0.0001$	&	A	&	$24.09$	&	$23.96$	&	$22.61$	&	H$\beta$, [OIII], [NII]	\\  
s$BzK$.8410		& 17:57:25.15  	& 65:21:18.01	&	$1.4564\pm0.0003$	&	A	&	$25.37$	&	$23.75$	&	$21.90$	&	[OII]				\\  
s$BzK$.7159		& 17:57:28.56	& 65:19:17.93	&	$1.4576\pm0.0002$	&	A	&	$24.70$	&	$23.05$	&	$22.44$	&	[OII]				\\  	
s$BzK$.6886		& 17:57:37.75  	& 65:18:53.95	&	$1.4663\pm0.0004$	&	A	&	$25.82$	&	$23.25$	&	$21.70$	&	[OII]				\\  
s$BzK$.8761		& 17:56:57.03	& 65:21:53.86	&	$1.4764\pm0.0003$	&	A	&	$23.35$	&	$22.83$	&	$20.37$	&	[OII]				\\  	
s$BzK$.8799		& 17:57:11.43  	& 65:21:53.94	&	$1.5589\pm0.0001$	&	A	&	$23.59$	&	$22.26$	&	$21.14$	&	CIII], MgII abns, [OII]	\\  	
s$BzK$.2998		& 17:56:56.40	& 65:12:32.76	&	$1.5620\pm0.0004$	&	A	&	$24.19$	&	$23.79$	&	$22.88$	&	[OII]				\\  	
s$BzK$.9006		& 17:56:28.73	& 65:22:10.94	&	$1.5943\pm0.0002$	&	A	&	$22.95$	&	$22.84$	&	$22.27$	&	[OII]				\\  
s$BzK$.9788		& 17:55:49.35	& 65:23:16.14	&	$1.595\pm0.001$	&	A	&	$23.93$	&	$22.98$	&	$22.18$	&	FeII+MgII absn	\\  	
s$BzK$.11725		& 17:56:30.31  	& 65:25:31.69	&	$1.725\pm0.005$	&	B	&	$22.35$	&	$21.78$	&	$21.00$	&	AGN: broad MgII			\\  
s$BzK$.5102		& 17:57:57.61	& 65:15:55.59	&	$1.979\pm0.002$	&	A	&	$23.59$	&	$22.84$	&	$22.21$	&	AlII, MgII			\\ 	%LBG: ISM abs., AlII, MgII		\\  
s$BzK$.6330		& 17:57:37.08	& 65:17:58.83	&	$2.218\pm0.001$	&	A	&	$23.82$	&	$23.23$	&	$21.94$	&	AGN: CIV, CIII], MgII	\\  
s$BzK$.3534		& 17:58:01.74	& 65:13:31.73	&	$2.256\pm0.002$	&	A	&	$23.73$	&	$22.84$	&	$21.82$	&	CIV+AlII absn			\\	%LBG: ISM abs., CIV, AlII		\\ 	
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]	\\  
s$BzK$.3718		& 17:58:01.19	& 65:13:49.25	&	$2.4020\pm0.0005$	&	A	&	$22.65$	&	$21.75$	&	$21.76$	&	CIV+AlII absn			\\	%LBG: ISM abs., CIV, AlII		\\ 	
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]	\\  
\hline
\end{tabular} 
\tablefoot{\tablefoottext{a}{The names are composed of the selection technique for the source --  AGN, s$BzK$ or p$BzK$ ($\equiv$p$BzK$* here) --  followed by the identification number in our $K$-band ($3.6~\mu$m) catalogue for $BzK$ (AGN) targets.}
\tablefoottext{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).}
\tablefoottext{c}{Magnitudes were derived using SExtractor MAG\_AUTO and are therefore slightly different from the aperture magnitudes used to derive colours for candidate selection.}}
\end{table}