Fig. 8
Comparison of various templates used to model the Fe II pseudo-contunuum in the UV band. Vestergaard & Wilkes (2001): blue line. Tsuzuki et al. (2006): magenta line; our newly proposed template: black line; 11-m20-20.5-735 of Bruhweiler & Verner (2008) convolved with 900 km s-1 Gaussian broadening, as used in the current paper: thick red line.
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