\begin{table}%t2
\par
\caption{\label{tab:optical-lines}Intensities of optical lines, corrected for stellar absorption, but not for reddening, with respect to H$\beta=100$.}
\small%%\centering

{
\begin{tabular}{rrrrrr}       
\hline\hline  \noalign{\smallskip}
	 & 			 & 	 	SDSS			 & 	 	Kitt Peak			 & 	 	CFHT 2003		 	 & 		CFHT 2001	 	\\
\hline
\par
	  & 	[Ne V]	3426	 & 					 & 					 & 		55.54	 $\pm$ 	5.19	 & 		84.05	 $\pm$ 	13.07	\\
	 & 	[O II]	3727	 & 	 				 & 	 				 & 	 $<$0.60			 & 	 $<$1.55			\\
	 & 	H I	3735	 & 					 & 					 & 		1.07	 $\pm$ 	0.31	 & 					\\
	 & 	H I	3751	 & 					 & 		4.94	 $\pm$ 	1.18	 & 		1.70	 $\pm$ 	0.32	 & 					\\
	 & 	H I	3772	 & 					 & 		4.36	 $\pm$ 	1.30	 & 		2.30	 $\pm$ 	0.35	 & 					\\
	 & 	H I	3798	 & 					 & 	 $<$3.0		 	 & 		2.64	 $\pm$ 	0.38	 & 					\\
	 & 	H I	3836	 & 		6.73	 $\pm$ 	0.53	 & 		3.71	 $\pm$ 	0.82	 & 		4.67	 $\pm$ 	0.37	 & 					\\
	 & 	[Ne III]	3869	 & 	 $<$1.2		 	 & 	 $<$1.5			 & 		0.77	 $\pm$ 	0.31	 & 		1.67	 $\pm$ 	0.48	\\
	 & 	H I	3889	 & 		9.06	 $\pm$ 	0.43	 & 		7.81	 $\pm$ 	0.87	 & 		9.28	 $\pm$ 	0.45	 & 		2.37	 $\pm$ 	0.47	\\
	 & 	H I	3970	 & 		13.29	 $\pm$ 	0.44	 & 		13.24	 $\pm$ 	0.79	 & 		12.70	 $\pm$ 	0.47	 & 		5.85	 $\pm$ 	0.58	\\
	 & 	He II	4027	 & 	 $<$1.2			 & 	 $<$1.5			 & 		0.56	 $\pm$ 	0.21	 & 					\\
	 & 	C III	4069	 & 	 	2.1	::		 & 	 $<$1.5			 & 	 $<$0.58			 & 					\\
	 & 	H I	4102	 & 		25.11	 $\pm$ 	0.42	 & 		25.49	 $\pm$ 	0.62	 & 		25.16	 $\pm$ 	0.43	 & 		19.79	 $\pm$ 	1.06	\\
	 & 	He II	4201	 & 	 $<$1.2			 & 	 $<$1			 & 		1.04	 $\pm$ 	0.19	 & 					\\
	 & 	C II	4267	 & 	 $<$1.2			 & 	 $<$1			 & 	 $<$0.32			 & 					\\
	 & 	H I	4340	 & 		46.09	 $\pm$ 	0.38	 & 		48.06	 $\pm$ 	0.44	 & 		47.19	 $\pm$ 	0.50	 & 		42.49	 $\pm$ 	0.80	\\
	 & 	[O III]	4363	 & 	 $<$1.2			 & 	 $<$1			 & 	 $<$0.41		 	 & 					\\
	 & 	N III	4379	 & 	 $<$1.2			 & 	 $<$1			 & 	 $<$0.09			 & 					\\
	 & 	He I	4471	 & 	 $<$1.2			 & 	 $<$1			 & 	 $<$0.11			 & 					\\
	 & 	He II	4543	 & 		2.97	 $\pm$ 	0.33	 & 		2.91	 $\pm$ 	0.35	 & 		2.46	 $\pm$ 	0.22	 & 					\\
	 & 	[Ar V]	4626	 & 	 $<$1.2			 & 	 $<$1			 & 	 $<$0.38			 & 					\\
	 & 	O IV	4632	 & 	 $<$1.2			 & 	 $<$1			 & 	 $<$0.38			 & 					\\
	 & 	C III	4650	 & 	 $<$1.2			 & 	 $<$1			 & 	 $<$0.38			 & 					\\
	 & 	C IV	4659	 & 	 $<$1.2			 & 	 $<$1			 & 	 $<$0.38			 & 					\\
	 & 	C IV	4659	 & 	 $<$1.2			 & 	 $<$1			 & 	 $<$0.24			 & 					\\
	 & 	He II	4686	 & 		75.13	 $\pm$ 	0.31	 & 		79.02	 $\pm$ 	0.28	 & 		77.50	 $\pm$ 	0.95	 & 		79.06	 $\pm$ 	1.11	\\
	 & 	[Ar IV]	4711	 & 	 $<$1.2			 & 	 $<$1			 & 	 $<$0.15			 & 					\\
	 & 	[Ne IV]	4715	 & 	 $<$1.2			 & 	 $<$1			 & 		0.32	 $\pm$ 	0.08	 & 					\\
	 & 	[Ne IV]	4725	 & 	 $<$1.2			 & 	 $<$1			 & 		0.26	 $\pm$ 	0.08	 & 					\\
	 & 	[Ar IV]	4740	 & 	 $<$1.2			 & 	 $<$1			 & 	 $<$0.15			 & 					\\
	 & 	H$\beta$	4861	 & 		100.00	 $\pm$ 	0.29	 & 		100.00	 $\pm$ 	0.26	 & 		100.00	 $\pm$ 	0.78	 & 		100.00	 $\pm$ 	1.59	\\
	 & 	O V	4930	 & 	 $<$1.2			 & 	 $<$0.8			 & 	 $<$0.28			 & 					\\
	 & 	N V	4945	 & 	 $<$1.2			 & 	 $<$0.8			 & 	 $<$0.28			 & 					\\
	 & 	[O III]	4959	 & 	 $<$1.2			 & 	 $<$0.99	 $\pm$ 	0.29	 & 		0.59	 $\pm$ 	0.13	 & 		0.69	 $\pm$ 	0.69	\\
	 & 	[O III]	5007	 & 		1.82	 $\pm$ 	0.28	 & 		2.16	 $\pm$ 	0.26	 & 		2.53	 $\pm$ 	0.16	 & 		1.81	 $\pm$ 	0.79	\\
	 & 	[Fe VI]	5146	 & 	 $<$10.0			 & 	 $<$0.8			 & 	 $<$0.28			 & 					\\
	 & 	He II	5411	 & 		5.8	 $\pm$ 	0.22	 & 		6.49	 $\pm$ 	0.28	 & 					 & 		5.12	 $\pm$ 	0.31	\\
	 & 	He I	5876	 & 	 $<$0.8			 & 	 $<$0.8			 & 					 & 	 $<$0.19			\\
	 & 	[Fe VII]	6087	 & 	 $<$0.8			 & 	 $<$0.8			 & 	 				 & 					\\
	 & 	H$\alpha$	6563	 & 	 	322.03	 $\pm$ 	0.15	 & 	 	306.38	 $\pm$ 	0.22	 & 	 				 & 		248.54	 $\pm$ 	2.63	\\
	 & 	[N II]	6584	 & 	 $<$1.6			 & 	 				 & 	 				 & 					\\
	 & 	[S II]	6716	 & 	 $<$1.6			 & 	 				 & 	 				 & 					\\
	 & 	[S II]	6731	 & 	 $<$1.6			 & 	 				 & 	 				 & 					\\
	 & 	[Ar V]	7006	 & 	 $<$1.6			 & 	 				 & 	 				 & 					\\
	 & 	He I	7065	 & 	 $<$1.6			 & 	 				 & 	 				 & 					\\
	 & 	[Ar III]	7136	 & 	 $<$1.6			 & 	 				 & 	 				 & 					\\
	 & 	[O II]	7320	 & 	 $<$1.6			 & 	 				 & 					 & 					\\
	 & 	[O II]	7330	 & 	 $<$1.6			 & 	 				 & 					 & 					\\
	 & 	[O II]	7333	 & 	 $<$1.6			 & 	 				 & 					 & 					\\
	 & 	??	7408	 & 		0.82	 $\pm$ 	0.24	 & 	 				 & 					 & 					\\
	 & 	[Cl IV]	7530	 & 	 $<$1.6			 & 	 				 & 					 & 					\\
%	 & 	??	7593	 & 		1.66	 $\pm$ 	0.26	 & 	 				 & 					 & 					\\
	 & 	He II	7600	 & 	 $<$1.6			 & 	 				 & 	 				 & 					\\
	 & 	O V	7611	 & 	 $<$1.6			 & 	 				 & 	 				 & 					\\
	 & 	O IV	7713	 & 	 $<$1.6			 & 	 				 & 	 				 & 					\\
	 & 	C IV	7726	 & 	 $<$1.6			 & 	 				 & 	 				 & 					\\
	 & 	[Ar III]	7751	 & 	 $<$1.6			 & 	 				 & 					 & 					\\
	 & 	[Cl IV]	8046	 & 	 $<$1.6			 & 	 				 & 					 & 					\\
	 & 	CIII	8196	 & 	 $<$1.6			 & 	 				 & 					 & 					\\
	 & 	He II	8237	 & 		1.76	 $\pm$ 	0.16	 & 	 				 & 					 & 					\\
	 & 	H P16	8502	 & 	 $<$1.6			 & 	 				 & 					 & 					\\
	 & 	H P15	8545	 & 	 $<$1.6			 & 	 				 & 					 & 					\\
	 & 	H P14	8598	 & 	 $<$1.6			 & 	 				 & 					 & 					\\
	 & 	H P13	8665	 & 	 $<$1.6			 & 	 				 & 					 & 					\\
	 & 	H P12	8750	 & 		1.29	 $\pm$ 	0.26	 & 	 				 & 					 & 					\\
	 & 	H P10	9014	 & 		1.7	:		 & 	 				 & 					 & 					\\
	 & 	[S III]	9069	 & 	 $<$1.6			 & 	 				 & 					 & 					\\
\hline 
\end{tabular}}
\end{table}