Table 4: Rest wavelength, along with the observed luminosity and the luminosity predicted by the LOC model of the broad UV lines as measured by FUSE (labeled 1) and HST-STIS (labeled 2). For each observed blended-line, the value of Lum $_{\rm LOC}$ consistently refers to the summed contribution of the lines in the blend.
Ion Wavelength Lum $_{\rm obs}$ Lum $_{\rm LOC}$ Inst Notes
  (Å) (1041 erg s-1) (1041 erg s-1)    
S  VI 933+944 <2.9 5.7 1  
C  III 977 10.7 $\pm$ 2.5 68.0 1  
N  III 989+991 <2.52 2.2 1  
Ly$\beta$ + O  VI 1025+1032+1038 31 $\pm$ 6 30.4 1  
He  II 1085 1.6 $\pm$ 0.6 2.4 1  
Ly$\alpha$ 1216 75.7 $\pm$ 19.4 75.7 2 1
N  V 1238+1242 13.6 $\pm$ 6.0 13.4 2  
O  I +Si  II 1304 3.1 $\pm$ 0.6 3.7 2  
C  II 1335 1.3 $\pm$ 0.4 2.0 2  
Si  IV 1393+1403 11 $\pm$ 2 13.7 2 2
C  IV 1548+1551 70 $\pm$ 12 42.9 2  
He  II 1640 17 $\pm$ 4 13.8 2 3
Notes: (1) Blended with O V] (1218 Å) and He II (1216 Å); (2) blended also with the O IV] quintuplet (1402 Å) and the S IV] quintuplet (1406 Å); (3) blended with the O III] doublet (1661+1666 Å).

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