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Fig. 9


Summary of determinations of the black hole mass in RE J1034+396: from LF or HF higher or lower resonance interpretation of the X-ray QPO, from the broadband fitting of the optical/UV/X-ray spectra with starlight and disk/corona model, from line stellar absorption feature width, from emission lines from NLR ([OIII)] and BLR (Hβ and Mg II), and from the X-ray excess variance method.

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