Radio Galaxies with the Cherenkov Telescope Array

R. Angioni; P. Grandi; E. Torresi; C. Vignali; J. Knödlseder

doi:10.1016/j.astropartphys.2017.02.010

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arXiv · 1702.05926

Radio Galaxies with the Cherenkov Telescope Array

R. Angioni·P. Grandi·E. Torresi·C. Vignali·J. Knödlseder

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Abstract

Misaligned AGN (MAGNs), i.e., radio-loud AGNs with the jet not pointing directly towards us, represent a new class of GeV emitters revealed by the Fermi space telescope. Although they comprise only a small fraction of the high-energy sources, MAGNs are extremely interesting objects offering a different perspective to study high-energy processes with respect to blazars. The aim of this work is to evaluate the impact of the new-generation Cherenkov Telescope Array (CTA) on the MAGN class and propose possible observational strategies to optimize their detection.

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R. Angioni, P. Grandi, E. Torresi, C. Vignali, J. Knödlseder. 2017-02-20. Radio Galaxies with the Cherenkov Telescope Array. https://doi.org/10.1016/j.astropartphys.2017.02.010

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