Fig. 10
Stacked spectra of BLAGN (Class 1 objects) in three λ(= Lbol/LEdd) ranges: a) log λ ≤ −1.3; b) −1.3 < log λ ≤ −0.6 and c) log λ > −0.6 (see Table 2 for details). The rest energies of 6.4 keV and 6.9 keV are indicated by dotted lines. The stacked spectrum of objects with high accretion rates shows a strong Fe K line at 6.9 keV.
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