0636910 - FZÚ 2026 RIV IT eng C - Konferenční příspěvek (zahraniční konf.)
Sergijenko, O. - Brown, A. M. - Fiorillo, D. - Abe, K. - Abe, S. - Acharyya, A. - Blažek, Jiří - Chudoba, Jiří - Ebr, Jan - Hamal, Petr - Janeček, Petr - Juryšek, Jakub - Karas, Vladimír - Mandát, Dušan - Pech, Miroslav - Schovánek, Petr - Trávníček, Petr - Vacula, Martin … celkem 568 autorů
Sensitivity of the Cherenkov Telescope Array to the gamma-ray emission from neutrino sources detected by IceCube.
Proceedings of Science. Vol. 444. Trieste: Sissa Medilab srl, 2024 - (Saito, T.), č. článku 1531. ISSN 1824-8039.
[International Cosmic Ray Conference ICRC2023 /38./. Nagoya (JP), 26.07.2023-03.08.2023]
Grant CEP: GA MŠMT LTT17006; GA MŠMT EF16_013/0001403; GA MŠMT(CZ) EF18_046/0016007; GA MŠMT(CZ) EH22_008/0004632
Výzkumná infrastruktura: CTA-CZ II - 90105; CTA-CZ III - 90247
Institucionální podpora: RVO:68378271 ; RVO:67985815
Klíčová slova: CTA * neutrino sources * gamma-ray emission
Obor OECD: Particles and field physics; Astronomy (including astrophysics,space science) (ASU-R)
Web výsledku:
https://pos.sissa.it/444/1531/pdf
DOI: https://doi.org/10.22323/1.444.1531

Gamma-ray observations of the astrophysical neutrino sources are fundamentally important for understanding the underlying neutrino production mechanism. We investigate the Cherenkov Telescope Array (CTA) ability to detect the very-high-energy (VHE) gamma-ray counterparts to the neutrino-emitting Active Galaxies. The CTA performance under different configurations and array layouts is computed based on the neutrino and gamma-ray simulations of steady and transient types of sources, assuming that the neutrino events are detected with the IceCube neutrino telescope. The CTA detection probability is calculated for both CTA sites taking into account the visibility constraints. We find that, under optimal observing conditions, CTA could observe the VHE gamma-ray emission from at least 3 neutrino events per year.
Trvalý link: https://hdl.handle.net/11104/0367869