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Search for nanosecond-fast optical transients with TAIGA-HiSCORE array. / the TAIGA Collaboration.

In: Proceedings of Science, Vol. 395, 951, 18.03.2022.

Research output: Contribution to journal › Conference article › peer-review

Harvard

the TAIGA Collaboration 2022, 'Search for nanosecond-fast optical transients with TAIGA-HiSCORE array', Proceedings of Science, vol. 395, 951.

APA

the TAIGA Collaboration (2022). Search for nanosecond-fast optical transients with TAIGA-HiSCORE array. Proceedings of Science, 395, [951].

Vancouver

the TAIGA Collaboration. Search for nanosecond-fast optical transients with TAIGA-HiSCORE array. Proceedings of Science. 2022 Mar 18;395:951.

Author

the TAIGA Collaboration. / Search for nanosecond-fast optical transients with TAIGA-HiSCORE array. In: Proceedings of Science. 2022 ; Vol. 395.

BibTeX

@article{337ae306457c4e96b563872f53f5213e,
title = "Search for nanosecond-fast optical transients with TAIGA-HiSCORE array",
abstract = "The wide-angle Cherenkov array TAIGA-HiSCORE (FOV ∼0.6 ster), was originally buit as part of the TAIGA installation for high-energy gamma-ray astronomy and cosmic ray physics. It was proven that the array can also be used to search for nanosecond events in the optical range. This report discusses the method of searching for optical transients using the HiSCORE array and demonstrates its performance on a real example of detecting signals from a man-made Earth satellite. Search for short flares in the HiSCORE data of winter season 2018-2019 is carried out. One candidate for double optical repeater has been detected, but the estimated probability of a random chance of such a transient by background EAS is 78%. An upper limit on the probability of optical spikes with flux density of more than 10−4 erg/sec/cm2 and a duration more than 5 ns is established as ∼ 2 × 10−3 events/sr/hour.",
author = "{the TAIGA Collaboration} and Panov, {A. D.} and Astapov, {I. I.} and Awad, {A. K.} and Beskin, {G. M.} and Bezyazeekov, {P. A.} and M. Blank and Bonvech, {E. A.} and Borodin, {A. N.} and M. Br{\"u}ckner and Budnev, {N. M.} and Bulan, {A. V.} and Chernov, {D. V.} and A. Chiavassa and Dyachok, {A. N.} and Gafarov, {A. R.} and Garmash, {A. Yu} and Grebenyuk, {V. M.} and Gress, {O. A.} and Gress, {T. I.} and Grinyuk, {A. A.} and Grishin, {O. G.} and D. Horns and Ivanova, {A. L.} and Kalmykov, {N. N.} and Kindin, {V. V.} and Kiryuhin, {S. N.} and Kokoulin, {R. P.} and Kompaniets, {K. G.} and Korosteleva, {E. E.} and Kozhin, {V. A.} and Kravchenko, {E. A.} and Krivopalova, {A. A.} and Kuzmichev, {L. A.} and Kryukov, {A. P.} and Lagutin, {A. A.} and Lavrova, {M. V.} and Yu Lemeshev and Lubsandorzhiev, {B. K.} and Lubsandorzhiev, {N. B.} and Lukanov, {A. D.} and D. Lukyantsev and Mirgazov, {R. R.} and R. Mirzoyan and Monkhoev, {R. D.} and Osipova, {E. A.} and Pakhorukov, {A. L.} and Panasenko, {L. A.} and Rubtsov, {G. I.} and Sokolov, {A. V.} and A. Vaidyanathan",
note = "Funding Information: The work was performed at the UNU “Astrophysical Complex of MSU-ISU” (agreement 13.UNU.21.0007). The work is supported by the Russian Science Foundation (grant 19-72-20067 (Section 3), the Russian Federation Ministry of Science and High Education (projects FZZE-2020-0017, FZZE-2020-0024). The work was (partially) performed as part of the government contract of the SAO RAS approved by the Ministry of Science and Higher Education of the Russian Federation. G. Beskin acknowledges the support of Ministry of Science and Higher Education of the Russian Federation under the grant 075-15-2020-780 (N13.1902.21.0039). Publisher Copyright: {\textcopyright} Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0); 37th International Cosmic Ray Conference, ICRC 2021 ; Conference date: 12-07-2021 Through 23-07-2021",
year = "2022",
month = mar,
day = "18",
language = "English",
volume = "395",
journal = "Proceedings of Science",
issn = "1824-8039",
publisher = "Sissa Medialab Srl",

}

RIS

TY - JOUR

T1 - Search for nanosecond-fast optical transients with TAIGA-HiSCORE array

AU - the TAIGA Collaboration

AU - Panov, A. D.

AU - Astapov, I. I.

AU - Awad, A. K.

AU - Beskin, G. M.

AU - Bezyazeekov, P. A.

AU - Blank, M.

AU - Bonvech, E. A.

AU - Borodin, A. N.

AU - Brückner, M.

AU - Budnev, N. M.

AU - Bulan, A. V.

AU - Chernov, D. V.

AU - Chiavassa, A.

AU - Dyachok, A. N.

AU - Gafarov, A. R.

AU - Garmash, A. Yu

AU - Grebenyuk, V. M.

AU - Gress, O. A.

AU - Gress, T. I.

AU - Grinyuk, A. A.

AU - Grishin, O. G.

AU - Horns, D.

AU - Ivanova, A. L.

AU - Kalmykov, N. N.

AU - Kindin, V. V.

AU - Kiryuhin, S. N.

AU - Kokoulin, R. P.

AU - Kompaniets, K. G.

AU - Korosteleva, E. E.

AU - Kozhin, V. A.

AU - Kravchenko, E. A.

AU - Krivopalova, A. A.

AU - Kuzmichev, L. A.

AU - Kryukov, A. P.

AU - Lagutin, A. A.

AU - Lavrova, M. V.

AU - Lemeshev, Yu

AU - Lubsandorzhiev, B. K.

AU - Lubsandorzhiev, N. B.

AU - Lukanov, A. D.

AU - Lukyantsev, D.

AU - Mirgazov, R. R.

AU - Mirzoyan, R.

AU - Monkhoev, R. D.

AU - Osipova, E. A.

AU - Pakhorukov, A. L.

AU - Panasenko, L. A.

AU - Rubtsov, G. I.

AU - Sokolov, A. V.

AU - Vaidyanathan, A.

N1 - Funding Information: The work was performed at the UNU “Astrophysical Complex of MSU-ISU” (agreement 13.UNU.21.0007). The work is supported by the Russian Science Foundation (grant 19-72-20067 (Section 3), the Russian Federation Ministry of Science and High Education (projects FZZE-2020-0017, FZZE-2020-0024). The work was (partially) performed as part of the government contract of the SAO RAS approved by the Ministry of Science and Higher Education of the Russian Federation. G. Beskin acknowledges the support of Ministry of Science and Higher Education of the Russian Federation under the grant 075-15-2020-780 (N13.1902.21.0039). Publisher Copyright: © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)

PY - 2022/3/18

Y1 - 2022/3/18

N2 - The wide-angle Cherenkov array TAIGA-HiSCORE (FOV ∼0.6 ster), was originally buit as part of the TAIGA installation for high-energy gamma-ray astronomy and cosmic ray physics. It was proven that the array can also be used to search for nanosecond events in the optical range. This report discusses the method of searching for optical transients using the HiSCORE array and demonstrates its performance on a real example of detecting signals from a man-made Earth satellite. Search for short flares in the HiSCORE data of winter season 2018-2019 is carried out. One candidate for double optical repeater has been detected, but the estimated probability of a random chance of such a transient by background EAS is 78%. An upper limit on the probability of optical spikes with flux density of more than 10−4 erg/sec/cm2 and a duration more than 5 ns is established as ∼ 2 × 10−3 events/sr/hour.

AB - The wide-angle Cherenkov array TAIGA-HiSCORE (FOV ∼0.6 ster), was originally buit as part of the TAIGA installation for high-energy gamma-ray astronomy and cosmic ray physics. It was proven that the array can also be used to search for nanosecond events in the optical range. This report discusses the method of searching for optical transients using the HiSCORE array and demonstrates its performance on a real example of detecting signals from a man-made Earth satellite. Search for short flares in the HiSCORE data of winter season 2018-2019 is carried out. One candidate for double optical repeater has been detected, but the estimated probability of a random chance of such a transient by background EAS is 78%. An upper limit on the probability of optical spikes with flux density of more than 10−4 erg/sec/cm2 and a duration more than 5 ns is established as ∼ 2 × 10−3 events/sr/hour.

UR - http://www.scopus.com/inward/record.url?scp=85143884430&partnerID=8YFLogxK

M3 - Conference article

AN - SCOPUS:85143884430

VL - 395

JO - Proceedings of Science

JF - Proceedings of Science

SN - 1824-8039

M1 - 951

T2 - 37th International Cosmic Ray Conference, ICRC 2021

Y2 - 12 July 2021 through 23 July 2021

ER -

ID: 40912389