Active galactic nuclei (AGN) emit radiation via accretion across the entire energy spectrum. While the standard disk and corona model can somewhat describe this emission, it fails to predict specific features such as the soft X-ray excess, the short-term
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Extragalactic Science with the Orbiting Astronomical Satellite Investigating Stellar Systems (OASIS) Observatory. [PDF]
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24 Micron Properties of X‐Ray–selected Active Galactic Nuclei [PDF]
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The Nuclear Reddening Curve for Active Galactic Nuclei and the Shape of the Infrared to X‐Ray Spectral Energy Distribution [PDF]
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The Cosmic Evolution of Hard X-Ray-selected Active Galactic Nuclei [PDF]
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MCG-6-30-15: long time-scale X-ray variability, black hole mass and active galactic nuclei high states [PDF]
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Radiation induced by relativistic electron showers in the X-ray spectrum of Active Galactic Nuclei [PDF]
A. Antonicci, Ana I. Gómez de Castro
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Proton Acceleration with Relativistic Electromagnetic Shock. [PDF]
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CONfirm: A Spectacular Galactic Scale MHD Powered Wind in ESO~320-G030
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New nearby active galactic nuclei among INTEGRAL and RXTE X-ray sources [PDF]
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