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X-ray Coronal Properties of Swift/BAT-Selected Seyfert 1 Active Galactic Nuclei

By Nikita Kamraj and others
The corona is an integral component of Active Galactic Nuclei (AGN) which produces the bulk of the X-ray emission above 1--2 keV. However, many of its physical properties and the mechanisms powering this emission remain a mystery. In particular, the temperature of the coronal plasma has been difficult to constrain... Show more
February 2, 2022
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X-ray Coronal Properties of Swift/BAT-Selected Seyfert 1 Active Galactic Nuclei
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