The Great Slump: Mrk 926 reveals discrete and varying Balmer line satellite components during a drastic phase of decline

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Fig. 2.

Reduced and [O III] λ5007-intercalibrated optical spectra of Mrk 926 taken with the HET telescope during our variability campaign in 2010. The continuum bands and the broad-line integration intervals are marked according to Table 2. The spectra shown here are not corrected for Galactic foreground extinction.

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