**Table 3:** Ultraviolet (IUE) and optical line fluxes (Keyes & Aller 1990). Keyes fluxes were dereddened fluxes using an interstellar extinction of E_B-V=0.85.
Wavelength	Ident.	Measured	Dereddened
(nm)		Fluxes¹	Intensities¹
123.83	N V	0.12	240
140.06	O IV	0.61	271
148.50	N IV]	0.70	415
154.83	C IV	20.80	12100
157.57	[Ne V]	0.21	17.4
164.20	He II	5.00	2700
174.95	N III]	0.62	275
189.20	Si III]	0.17	87.5
190.67	C III]	4.23	2300
190.88	C III]	6.85	3700
232.55	C II	0.61	526
232.75	C II	0.48	411
242.14	[Ne IV]	1.32	609
242.45	[Ne IV]	0.43	198
278.23	[Mg V]	0.83	98.4
334.68	[Ne V]		700
342.68	[Ne V]		2100
372.62	[O II]	5.98	220
372.88	[O II]	2.19	80.2
386.98	[Ne III]	43.34	1500
396.86	[Ne III]	15.56	500
436.44	[O III]	13.36	340
447.10	He I	1.90	45.4
468.60	He II	32.3	660
471.14	[Ar IV]	1.91	38.1
474.00	[Ar IV]	6.74	131.7
486.10	H $_{\beta}$	75.9	1360
493.26	[O III]	0.17	2.9
496.03	[O III]	388.61	6400
500.82	[O III]	1178.73	19000
551.70	[Cl III]	0.20	2.23
553.80	[Cl III]	0.77	8.6
658.40	[N II]	202.65	1500
671.63	[S II]	3.57	24.1
673.10	[S II]	8.20	56
857.70	[Cl II]	1.01	3.6

¹ Units: $10^{-12}\,{\rm erg~cm^{-2}~s^{-1}}$ .

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