Using X-ray reverberation models, the authors reproduce the SDSS Stripe-82 quasar UV/optical power spectra at 1300-4000 A, favouring an accretion-powered corona, spin below 0.7, and corona height 20-60 Rg.
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X-ray reverberation modelling of the observed UV/optical power spectra of quasars
Using X-ray reverberation models, the authors reproduce the SDSS Stripe-82 quasar UV/optical power spectra at 1300-4000 A, favouring an accretion-powered corona, spin below 0.7, and corona height 20-60 Rg.