Comparison of the composite spectrum of “normal” AGN (Shull et al. 2012) with the spectrum of PG 0043+039 and equivalent widths of selected UV lines.
|Emission lines||Equivalent width [Å]|
|O vi λ1038||23 ± 3||26 ± 3|
|Lyα||115 ± 5||120 ± 5|
|N v λ1243||23 ± 2||34 ± 3|
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