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Table 1:

Observed line fluxes.
$\lambda$(Å) F($\lambda$)a I($\lambda$)b Err.(%) ID
3727 54.1 26.83 10 [O  II]
3749 10.4 5.73 50 I
3798 13.4 7.37 30 I
3836 18.6 10.20 15 I
3869 48.6 28.05 10 [Ne  III]
3889 24.5 13.54 10 I, He  I
3969 48.5 26.93 10 I, [Ne  III]
4069 6.43 3.66 25 [S  II]+c
4102 51.4 27.75 10 I
4341 95.1 50.43 10 I
4363 15.0 8.32 10 [O  III]
4541 7.46 4.07 40 He  II
4657 5.59 3.02 50 IV, [Fe  III]
4686 182. 98.06 10 He  II
4714 10.1 5.44 30 [Ar  IV]+c
4740 5.06 2.71 35 [Ar  IV]
4861 198. 100 10 I
4959 210. 110 5 [O  III]
5007 651. 341 5 [O  III]
5412 17.2 8.68 20 He  II
5876 5.70 2.77 30 He  I
6312 3.11 1.11 50 [S  III]
6563 630. 284 5 I
6583 19.9 9.37 15 [N  II]
6717 3.57 1.67 50 [S  II]
6731 5.61 2.62 50 [S  II]
7136 5.95 2.73 25 [Ar  III]
a In units of 10-18 erg cm-2 s-1.

b De-reddened and ratioed to H$\beta$ = 100. All H  I lines de-blended from He  II; [O  II] 3727 de-blended from [S  III] and two H  I lines.

c Blends: [S  II] 4069 + [Fe  V] 4071 + C  III 4069; [Ar  IV] 4711 + He  I 4713 + [Ne  IV] 4714+16.


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