Multi-wavelength analysis of Compton-thick AGNs shows they favor higher Eddington ratios and are driven by intense accretion and heavy obscuration instead of simple viewing-angle effects.
K., Silk J., 2007, Monthly Notices of the Royal Astronomical Society, 382, 1415 SecrestN.,DudikR.,DorlandB.,ZachariasN.,MakarovV.,FeyA.,Frouard MNRAS000, 1–16 (2026) 16M
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Compton-thick AGN Characterisation in a Multi-wavelength Context: Insights from the 70-Month \textit{SWIFT}/BAT Catalogue
Multi-wavelength analysis of Compton-thick AGNs shows they favor higher Eddington ratios and are driven by intense accretion and heavy obscuration instead of simple viewing-angle effects.