Table 2: Emission-line measurements of Sy2s.

Object
Redshift Ly $\alpha\lambda$1216a N V$\lambda $1240a C IV$\lambda $1549a He II$\lambda $1640a C III]$\lambda $1909a Ref.b

NGC 1068
0.004 713 $\pm$ 100 224 $\pm$ 41 520 $\pm$ 80 187 $\pm$ 29 240 $\pm$ 35 1
NGC 4507c 0.012 75.6 $\pm$ 15.1 5.2 $\pm$ 1.0 13.5 $\pm$ 2.7 5.6 $\pm$ 1.1 5.8 $\pm$ 1.2 2
NGC 5135c 0.014 59.0 $\pm$ 11.8 1.1 $\pm$ 0.2 4.1 $\pm$ 0.8 10.0 $\pm$ 2.0 -- 3
NGC 5506c 0.006 -- -- 4.5 $\pm$ 1.4d 2.0 $\pm$ 0.6d 3.6 $\pm$ 0.7 2
NGC 7674 0.029 47.0 $\pm$ 20.3 -- 11.4 $\pm$ 3.3 5.1 $\pm$ 1.5 7.9 $\pm$ 2.7 4
Mrk 3 0.014 64 $\pm$ 19d 3 $\pm$ 1d 21 $\pm$ 2 9 $\pm$ 1 9 $\pm$ 1 5
Mrk 573 0.017 151.2 $\pm$ 22.7 6.3 $\pm$ 0.9 29.0 $\pm$ 4.3 12.6 $\pm$ 1.9 8.8 $\pm$ 1.3 6
Mrk 1388 0.021 -- -- 8.3 $\pm$ 1.2 3.8 $\pm$ 0.6 3.6 $\pm$ 0.5 6
MCG -3-34-64c 0.017 56 $\pm$ 11 5 $\pm$ 1 14 $\pm$ 3 10 $\pm$ 2 7 $\pm$ 1 7
a
Fluxes are in units of 10-14 erg s-1 cm-2.
b
References. -- (1) Snijders et al. (1986), (2) Bergeron et al. (1981), (3) Thuan (1984), (4) Kraemer et al. (1994),
(5) Malkan & Oke (1983), (6) McAlpine (1988), (7) De Robertis et al. (1988).
c
20% of the line flux is assigned as the flux error.
d
30% of the line flux is assigned as the flux error.


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