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Sensitivity of the Cherenkov Telescope Array to emission from the gamma-ray counterparts of neutrino events

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    0568934 - ASÚ 2023 RIV IT eng C - Conference Paper (international conference)
    Abdalla, H. - Abe, H. - Abe, S. - Araudo, Anabella - Karas, Vladimír … Total 1344 authors
    Sensitivity of the Cherenkov Telescope Array to emission from the gamma-ray counterparts of neutrino events.
    Proceedings of Science. Vol. 395. Trieste: Sissa Medilab srl, 2022, č. článku 975. ISSN 1824-8039.
    [International Cosmic Ray Conference /37./. Berlin (DE), 12.07.2021-23.07.2021]
    Grant - others:AV ČR(CZ) CONICET-22-06
    Program: Bilaterální spolupráce
    Institutional support: RVO:67985815
    Keywords : astrophysics * high energy * astrophysical phenomena
    OECD category: Particles and field physics
    https://pos.sissa.it/395/975/pdf

    We investigate the possibility of detection of the VHE gamma-ray counterparts to the neutrino astrophysical sources within the Neutrino Target of Opportunity (NToO) program of CTA using the populations simulated by the FIRESONG software to resemble the diffuse astrophysical neutrino flux measured by IceCube. We derive the detection probability for different zenith angles and
    geomagnetic field configurations. The difference in detectability of sources between CTA-North and CTA-South for the average geomagnetic field is not substantial. We investigate the effect of a higher night-sky background and the preliminary CTA Alpha layout on the detection probability.
    Permanent Link: https://hdl.handle.net/11104/0340211

     
     
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