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Search for High-Energy Gamma Quanta from the Cygnus Cocoon Source in October–November 2020. / Okuneva, E.; Sveshnikova, L.; Astapov, I. et al.

In: Physics of Atomic Nuclei, Vol. 87, No. 3, 06.07.2024, p. 165-171.

Research output: Contribution to journal › Article › peer-review

Harvard

Okuneva, E, Sveshnikova, L, Astapov, I, Bezyazykov, P, Blinov, A, Borodin, A, Bonvech, E, Budnev, N, Bulan, A, Busygin, P, Vaidyanatan, A, Volkov, N, Volchugov, P, Voronin, D, Gafarov, A, Gres, Е, Gres, O, Gres, T, Grishin, O, Garmash, A, Grebenyuk, V, Grinyuk, A, Dyachok, A, Zhurov, D, Zagorodnikov, A, Ivanova, A, Ivanova, A, Ilyushin, M, Kindin, V, Kiryukhin, V, Kokoulin, R, Kolosov, N, Kompaniets, K, Korosteleva, E, Kozhin, V, Kravchenko, E, Kryukov, A, Kuzmichev, L, Chiavassa, A, Lavrova, M, Lagutin, A, Lemeshev, Y, Lubsandorzhiev, B, Lubsandorzhiev, N, Malakhov, S, Mirgazov, R, Monkhoev, R, Osipova, E, Pakhorukov, A, Pan, A, Panov, A, Pankov, L, Petrukhin, A, Podgrudkov, D, Poddubny, I, Popova, E, Postnikov, E, Prosin, V, Ptuskin, V, Pushnin, A, Razumov, A, Raikin, R, Rubtsov, G, Ryabov, E, Samoliga, V, Satyshev, I, Silaev, A, Silaev, A, Sidorenkov, A, Skurikhin, A, Sokolov, A, Tabolenko, V, Tanaev, A, Ternovoy, M, Tkachev, L, Ushakov, N, Chernov, D, Yashin, I & Kalmykov, NN 2024, 'Search for High-Energy Gamma Quanta from the Cygnus Cocoon Source in October–November 2020', Physics of Atomic Nuclei, vol. 87, no. 3, pp. 165-171. https://doi.org/10.1134/S1063778824700194

APA

Okuneva, E., Sveshnikova, L., Astapov, I., Bezyazykov, P., Blinov, A., Borodin, A., Bonvech, E., Budnev, N., Bulan, A., Busygin, P., Vaidyanatan, A., Volkov, N., Volchugov, P., Voronin, D., Gafarov, A., Gres, Е., Gres, O., Gres, T., Grishin, O., ... Kalmykov, N. N. (2024). Search for High-Energy Gamma Quanta from the Cygnus Cocoon Source in October–November 2020. Physics of Atomic Nuclei, 87(3), 165-171. https://doi.org/10.1134/S1063778824700194

Vancouver

Okuneva E, Sveshnikova L, Astapov I, Bezyazykov P, Blinov A, Borodin A et al. Search for High-Energy Gamma Quanta from the Cygnus Cocoon Source in October–November 2020. Physics of Atomic Nuclei. 2024 Jul 6;87(3):165-171. doi: 10.1134/S1063778824700194

Author

Okuneva, E. ; Sveshnikova, L. ; Astapov, I. et al. / Search for High-Energy Gamma Quanta from the Cygnus Cocoon Source in October–November 2020. In: Physics of Atomic Nuclei. 2024 ; Vol. 87, No. 3. pp. 165-171.

BibTeX

@article{9e08e80a652c4f548fe7cdca8e954939,
title = "Search for High-Energy Gamma Quanta from the Cygnus Cocoon Source in October–November 2020",
abstract = "Abstract: In November 2020, the IceCube Neutrino Observatory registered a neutrino event with an energy of 150 TeV directed at the Cygnus Cocoon gamma-ray source. In the Carpet-2 experiment, as part of the Baksan Neutrino Observatory (BNO), a sharp increase in the flow of events with an energy above 300 TeV was recorded from the same direction within the angular accuracy of the events. This flux is 4 orders of magnitude higher than the expected intensity of gamma quanta of this energy region according to data in the region of less than 100 TeV. It was expected that such a powerful flare could be registered by the TAIGA-HiSCORE installation of the TAIGA astrophysical complex. We analyzed the events of the EAS recorded by the installation of TAIGA-HiSCORE for 18 h in October–November 2020 from the Cygnus Cocoon source. This article provides the upper limit of the expected excess flow.",
author = "E. Okuneva and L. Sveshnikova and I. Astapov and P. Bezyazykov and A. Blinov and A. Borodin and E. Bonvech and N. Budnev and A. Bulan and P. Busygin and A. Vaidyanatan and N. Volkov and P. Volchugov and D. Voronin and A. Gafarov and Е. Gres and O. Gres and T. Gres and O. Grishin and A. Garmash and V. Grebenyuk and A. Grinyuk and A. Dyachok and D. Zhurov and A. Zagorodnikov and A. Ivanova and A. Ivanova and M. Ilyushin and V. Kindin and V. Kiryukhin and R. Kokoulin and N. Kolosov and K. Kompaniets and E. Korosteleva and V. Kozhin and E. Kravchenko and A. Kryukov and L. Kuzmichev and A. Chiavassa and M. Lavrova and A. Lagutin and Y. Lemeshev and B. Lubsandorzhiev and N. Lubsandorzhiev and S. Malakhov and R. Mirgazov and R. Monkhoev and E. Osipova and A. Pakhorukov and A. Pan and A. Panov and L. Pankov and A. Petrukhin and D. Podgrudkov and I. Poddubny and E. Popova and E. Postnikov and V. Prosin and V. Ptuskin and A. Pushnin and A. Razumov and R. Raikin and G. Rubtsov and E. Ryabov and V. Samoliga and I. Satyshev and A. Silaev, and A. Silaev, and A. Sidorenkov and A. Skurikhin and A. Sokolov and V. Tabolenko and A. Tanaev and M. Ternovoy and L. Tkachev and N. Ushakov and D. Chernov and I. Yashin and Kalmykov, {N. N.}",
note = "Сведения о финансировании Ministry of Education and Science of the Russian Federation FZZE-2020-0017,EB-075-15-2021-675,FZZE-2020-0024,FSUS-2020-0039 Russian Science Foundation 23-72-00019",
year = "2024",
month = jul,
day = "6",
doi = "10.1134/S1063778824700194",
language = "English",
volume = "87",
pages = "165--171",
journal = "Physics of Atomic Nuclei",
issn = "1063-7788",
publisher = "Maik Nauka-Interperiodica Publishing",
number = "3",

}

RIS

TY - JOUR

T1 - Search for High-Energy Gamma Quanta from the Cygnus Cocoon Source in October–November 2020

AU - Okuneva, E.

AU - Sveshnikova, L.

AU - Astapov, I.

AU - Bezyazykov, P.

AU - Blinov, A.

AU - Borodin, A.

AU - Bonvech, E.

AU - Budnev, N.

AU - Bulan, A.

AU - Busygin, P.

AU - Vaidyanatan, A.

AU - Volkov, N.

AU - Volchugov, P.

AU - Voronin, D.

AU - Gafarov, A.

AU - Gres, Е.

AU - Gres, O.

AU - Gres, T.

AU - Grishin, O.

AU - Garmash, A.

AU - Grebenyuk, V.

AU - Grinyuk, A.

AU - Dyachok, A.

AU - Zhurov, D.

AU - Zagorodnikov, A.

AU - Ivanova, A.

AU - Ivanova, A.

AU - Ilyushin, M.

AU - Kindin, V.

AU - Kiryukhin, V.

AU - Kokoulin, R.

AU - Kolosov, N.

AU - Kompaniets, K.

AU - Korosteleva, E.

AU - Kozhin, V.

AU - Kravchenko, E.

AU - Kryukov, A.

AU - Kuzmichev, L.

AU - Chiavassa, A.

AU - Lavrova, M.

AU - Lagutin, A.

AU - Lemeshev, Y.

AU - Lubsandorzhiev, B.

AU - Lubsandorzhiev, N.

AU - Malakhov, S.

AU - Mirgazov, R.

AU - Monkhoev, R.

AU - Osipova, E.

AU - Pakhorukov, A.

AU - Pan, A.

AU - Panov, A.

AU - Pankov, L.

AU - Petrukhin, A.

AU - Podgrudkov, D.

AU - Poddubny, I.

AU - Popova, E.

AU - Postnikov, E.

AU - Prosin, V.

AU - Ptuskin, V.

AU - Pushnin, A.

AU - Razumov, A.

AU - Raikin, R.

AU - Rubtsov, G.

AU - Ryabov, E.

AU - Samoliga, V.

AU - Satyshev, I.

AU - Silaev,, A.

AU - Silaev,, A.

AU - Sidorenkov, A.

AU - Skurikhin, A.

AU - Sokolov, A.

AU - Tabolenko, V.

AU - Tanaev, A.

AU - Ternovoy, M.

AU - Tkachev, L.

AU - Ushakov, N.

AU - Chernov, D.

AU - Yashin, I.

AU - Kalmykov, N. N.

N1 - Сведения о финансировании Ministry of Education and Science of the Russian Federation FZZE-2020-0017,EB-075-15-2021-675,FZZE-2020-0024,FSUS-2020-0039 Russian Science Foundation 23-72-00019

PY - 2024/7/6

Y1 - 2024/7/6

N2 - Abstract: In November 2020, the IceCube Neutrino Observatory registered a neutrino event with an energy of 150 TeV directed at the Cygnus Cocoon gamma-ray source. In the Carpet-2 experiment, as part of the Baksan Neutrino Observatory (BNO), a sharp increase in the flow of events with an energy above 300 TeV was recorded from the same direction within the angular accuracy of the events. This flux is 4 orders of magnitude higher than the expected intensity of gamma quanta of this energy region according to data in the region of less than 100 TeV. It was expected that such a powerful flare could be registered by the TAIGA-HiSCORE installation of the TAIGA astrophysical complex. We analyzed the events of the EAS recorded by the installation of TAIGA-HiSCORE for 18 h in October–November 2020 from the Cygnus Cocoon source. This article provides the upper limit of the expected excess flow.

AB - Abstract: In November 2020, the IceCube Neutrino Observatory registered a neutrino event with an energy of 150 TeV directed at the Cygnus Cocoon gamma-ray source. In the Carpet-2 experiment, as part of the Baksan Neutrino Observatory (BNO), a sharp increase in the flow of events with an energy above 300 TeV was recorded from the same direction within the angular accuracy of the events. This flux is 4 orders of magnitude higher than the expected intensity of gamma quanta of this energy region according to data in the region of less than 100 TeV. It was expected that such a powerful flare could be registered by the TAIGA-HiSCORE installation of the TAIGA astrophysical complex. We analyzed the events of the EAS recorded by the installation of TAIGA-HiSCORE for 18 h in October–November 2020 from the Cygnus Cocoon source. This article provides the upper limit of the expected excess flow.

UR - https://www.mendeley.com/catalogue/bef43995-3520-338e-a50e-5a105a2d7de5/

UR - https://www.scopus.com/record/display.uri?eid=2-s2.0-85197737100&origin=inward&txGid=c394cb8c42f443a160708cf8dd63ae19

U2 - 10.1134/S1063778824700194

DO - 10.1134/S1063778824700194

M3 - Article

VL - 87

SP - 165

EP - 171

JO - Physics of Atomic Nuclei

JF - Physics of Atomic Nuclei

SN - 1063-7788

IS - 3

ER -

ID: 61414244