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Fig. A.6.
Fit of the source MRK 335. HST data around the Lyα-CIV region are also available, in good agreement with IUE data. The spectrum rise at Log ν/Hz < 14.4 is caused by the IR emission of the dusty torus. Other BH mass estimates are from Haas et al. (2011) (Log 
) and Grier et al. (2017) (Log M/M⊙ = 7.25 ± 0.10).
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