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Fermi detection of gamma-ray emission from the hot coronae of radio-quiet active galactic nuclei
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TeV Neutrinos and Hard X-Rays from Relativistic Reconnection in the Corona of NGC 1068
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A Magnetized Strongly Turbulent Corona as the Source of Neutrinos from NGC 1068
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Extragalactic observatory science with the ASTRI mini-array at the Observatorio del Teide
F.G. Saturni, C.H.E. Arcaro, B. Balmaverde, J. Becerra González, A. Caccianiga, M. Capalbi, A. Lamastra, S. Lombardi, F. Lucarelli, R. Alves Batista, L.A. Antonelli, E.M. de Gouveia Dal Pino, R. Della Ceca, J.G. Green, A. Pagliaro, C. Righi, F. Tavecchio, S. Vercellone, A. Wolter, E. Amato, C. Bigongiari, M. Böttcher, G. Brunetti, P. Bruno, A. Bulgarelli, et al. Journal of High Energy Astrophysics 35 91 (2022) https://doi.org/10.1016/j.jheap.2022.06.004
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Evaluation of hadronic emission in starburst galaxies and star-forming galaxies
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Luigi Foschini, Matthew L. Lister, Sonia Antón, Marco Berton, Stefano Ciroi, Maria J. M. Marchã, Merja Tornikoski, Emilia Järvelä, Patrizia Romano, Stefano Vercellone and Elena Dalla Bontà Universe 7(10) 372 (2021) https://doi.org/10.3390/universe7100372
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Optical Spectroscopic Survey of a Sample of Unidentified Fermi Objects: II
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γ-Ray emission from Arp 220: indications of an active galactic nucleus
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Star-forming galaxies significantly contribute to the isotropic gamma-ray background
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Active Galactic Nuclei under the scrutiny of CTA
H. Sol, A. Zech, C. Boisson, U. Barres de Almeida, J. Biteau, J.-L. Contreras, B. Giebels, T. Hassan, Y. Inoue, K. Katarzyński, H. Krawczynski, N. Mirabal, J. Poutanen, F. Rieger, T. Totani, W. Benbow, M. Cerruti, M. Errando, L. Fallon, E. de Gouveia Dal Pino, J.A. Hinton, S. Inoue, J.-P. Lenain, A. Neronov, K. Takahashi, et al. Astroparticle Physics 43 215 (2013) https://doi.org/10.1016/j.astropartphys.2012.12.005
MODELING THE MOLECULAR COMPOSITION IN AN ACTIVE GALACTIC NUCLEUS DISK
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The AT20G view of Swift/BAT selected AGN: high-frequency radio waves meet hard X-rays
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PROPERTIES OF NEARBY STARBURST GALAXIES BASED ON THEIR DIFFUSE GAMMA-RAY EMISSION
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