Very High Energy Active Galactic Nuclei Synchrotron self-Compton Modeling Tour
J.-P. Lenain (1, 2), M. K. Daniel (2), C. Boisson (1), P. M., Chadwick (2), H. Sol (1), M. J. Ward (2) ((1) LUTH Observatoire de, Paris-Meudon, (2) Department of Physics, Astronomy Durham University)
TL;DR
This paper reviews VHE-emitting active galactic nuclei using synchrotron self-Compton models, analyzing their properties and potential correlations to better understand their emission mechanisms.
Contribution
It provides a comprehensive modeling tour of known VHE AGN sources and explores correlations among their intrinsic and derived parameters.
Findings
Identification of parameter correlations in VHE AGN
Enhanced understanding of emission mechanisms in AGN
Compilation of a catalog of modeled VHE AGN
Abstract
The current very high energy (VHE; E>100GeV) experiments have tremendously increased the number of detected extragalactic sources. We present a synchrotron self-Compton modeling tour of the active galactic nuclei currently established as VHE emitters so far, and investigate possible correlations among the intrinsic and derived parameters.
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Particle Detector Development and Performance · Particle Accelerators and Free-Electron Lasers