Two X-ray lamps at different heights above an AGN disk produce UV/optical delays at most 20 percent different from a single lamp, and simulated ICCFs are indistinguishable.
M., Gelbord, J., Barth, A
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Testing the extended corona model with the optical/UV reverberation mapping of the accretion disk
Two X-ray lamps at different heights above an AGN disk produce UV/optical delays at most 20 percent different from a single lamp, and simulated ICCFs are indistinguishable.