Relativistic reflection modeling in AGN and related variability from PCA: a brief review

X-ray observations of active galactic nuclei (AGNs) reveal relativistic reflections from the innermost regions of accretion disks, which contain general-relativistic footprints caused by spinning supermassive black holes (SMBH). We anticipate the spin of a SMBH to be stable over the human timeframe,...

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Bibliographic Details
Main Author: A. Danehkar
Format: Article
Language:English
Published: Frontiers Media S.A. 2024-10-01
Series:Frontiers in Astronomy and Space Sciences
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Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2024.1479301/full
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