Methodological Issues of Gamma-Ray and Neutrino Searches at the Yakutsk Array


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The method used to perform searches for extensive air showers (EAS) generated by neutral particles, such as high-energy gamma rays and astrophysical neutrinos, and the results of such searches are presented. A comprehensive analysis of relevant data, including those on EAS electrons, muons, and Cherenkov light and their time responses in scintillation and Cherenkov detectors, is performed for this purpose. An upper limit on the gamma-ray flux at the energies of 3 × 1018, 1019, and 3 × 1019 eV is set. A multivariate analysis of EAS properties of neutrino-induced air showers does not reveal neutrino-induced showers.

作者简介

S. Knurenko

Institute of Cosmophysical Research and Aeronomy, Siberian Branch

编辑信件的主要联系方式.
Email: s.p.knurenko@ikfia.ysn.ru
俄罗斯联邦, pr. Lenina 31, Yakutsk, 677980

Z. Petrov

Institute of Cosmophysical Research and Aeronomy, Siberian Branch

Email: s.p.knurenko@ikfia.ysn.ru
俄罗斯联邦, pr. Lenina 31, Yakutsk, 677980

I. Petrov

Institute of Cosmophysical Research and Aeronomy, Siberian Branch

Email: s.p.knurenko@ikfia.ysn.ru
俄罗斯联邦, pr. Lenina 31, Yakutsk, 677980

Yu. Egorov

Institute of Cosmophysical Research and Aeronomy, Siberian Branch

Email: s.p.knurenko@ikfia.ysn.ru
俄罗斯联邦, pr. Lenina 31, Yakutsk, 677980

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