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A search for ultra-high-energy neutrinos from TXS 0506+056 using the Pierre Auger Observatory

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    0538329 - FZÚ 2021 RIV GB eng J - Journal Article
    Aab, A. - Abreu, A. - Aglietta, M. - Bakalová, Alena - Blažek, Jiří - Boháčová, Martina - Chudoba, Jiří - Ebr, Jan - Juryšek, Jakub - Mandát, Dušan - Palatka, Miroslav - Pech, Miroslav - Prouza, Michael - Řídký, Jan - dos Santos, Eva M. Martins - Schovánek, Petr - Tobiška, Petr - Trávníček, Petr - Vícha, Jakub - Yushkov, Alexey … Total 391 authors
    A search for ultra-high-energy neutrinos from TXS 0506+056 using the Pierre Auger Observatory.
    Astrophysical Journal. Roč. 902, č. 2 (2020), s. 1-8, č. článku 105. ISSN 0004-637X. E-ISSN 1538-4357
    R&D Projects: GA MŠMT LTT18004; GA MŠMT LM2015038; GA MŠMT(CZ) EF18_046/0016010; GA MŠMT EF16_013/0001402; GA MŠMT(CZ) LM2018102
    Grant - others:OP VVV - AUGERII.CZ(XE) CZ.02.1.01/0.0/0.0/18_046/0016010; OP VVV - AUGER-CZ(XE) CZ.02.1.01/0.0/0.0/16_013/0001402
    Institutional support: RVO:68378271
    Keywords : high energy astrophysics * neutrino astronomy * blazars * transient sources * active galaxies
    OECD category: Particles and field physics
    Impact factor: 5.877, year: 2020
    Method of publishing: Limited access
    https://doi.org/10.3847/1538-4357/abb476

    Results of a search for ultra-high-energy neutrinos with the Pierre Auger Observatory from the direction of the blazar TXS 0506+056 are presented. They were obtained as part of the follow-up that stemmed from the detection of high-energy neutrinos and gamma rays with IceCube, Fermi-LAT, MAGIC, and other detectors of electromagnetic radiation in several bands. The Pierre Auger Observatory is sensitive to neutrinos in the energy range from 100 PeV to 100 EeV and in the zenith-angle range from = 60 degrees to = 95 degrees, where the zenith angle is measured from the vertical direction. No neutrinos from the direction of TXS 0506+056 have been found.

    Permanent Link: http://hdl.handle.net/11104/0316147

     
     
Number of the records: 1  

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