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The hybrid installation TAIGA: design, status and preliminary results. / TAIGA Collaboration.

в: Proceedings of Science, Том 358, 729, 02.07.2021.

Результаты исследований: Научные публикации в периодических изданияхстатья по материалам конференцииРецензирование

Harvard

TAIGA Collaboration 2021, 'The hybrid installation TAIGA: design, status and preliminary results', Proceedings of Science, Том. 358, 729.

APA

TAIGA Collaboration (2021). The hybrid installation TAIGA: design, status and preliminary results. Proceedings of Science, 358, [729].

Vancouver

TAIGA Collaboration. The hybrid installation TAIGA: design, status and preliminary results. Proceedings of Science. 2021 июль 2;358:729.

Author

TAIGA Collaboration. / The hybrid installation TAIGA: design, status and preliminary results. в: Proceedings of Science. 2021 ; Том 358.

BibTeX

@article{98132f2f2cc8470dbb3f58f652ee8d50,
title = "The hybrid installation TAIGA: design, status and preliminary results",
abstract = "The hybrid installation TAIGA (Tunka Advanced Instrument for cosmic rays and Gamma Astronomy) is under construction to study cosmic and gamma rays at energies 1013-1018 eV. It will incorporate timing wide-angle EAS Cherenkov array (TAIGA-HiSCORE) and number of imaging atmospheric Cherenkov telescopes (TAIGA-IACT). The first stage of TAIGA will include ~100 wide-angle non-imaging optical stations of TAIGA-HiSCORE, distributed over an area of ~1 km2 and three imaging telescopes at a distance of 300-500 m from each other. A combined method will be used to distinguish gamma-rays namely EAS parameters will be reconstructed by TAIGA-HiSCORE and a gamma-hadron separation will be carried out by TAIGA-IACT. With such an approach a hybrid detector will be built with a large area but with a relatively small number of telescopes.",
author = "{the TAIGA Collaboration} and N. Lubsandorzhiev and I. Astapov and P. Bezyazeekov and A. Borodin and M. Brueckner and N. Budnev and V. Chernykh and A. Chiavassa and A. Dyachok and O. Fedorov and A. Gafarov and A. Garmash and V. Grebenyuk and O. Gress and T. Gress and A. Grinyuk and O. Grishin and D. Horns and A. Igoshin and A. Ivanova and N. Kalmykov and Y. Kazarina and V. Kindin and P. Kirilenko and S. Kiryuhin and R. Kokoulin and K. Kompaniets and E. Korosteleva and V. Kozhin and E. Kravchenko and A. Kryukov and L. Kuzmichev and A. Lagutin and Y. Lemeshev and V. Lenok and B. Lubsandorzhiev and R. Mirgazov and R. Mirzoyan and R. Monkhoev and E. Osipova and A. Pakhorukov and A. Pan and M. Panasyuk and L. Pankov and A. Petrukhin and V. Poleschuk and M. Popesku and G. Rubtsov and A. Sokolov and A. Vaidyanathan",
note = "Funding Information: This work was supported by the Russian Foundation for Basic Research, grant 16-29-13035, and the Russian Science Foundation (grant 19-72-20230, Section 4), grant 19-72-20067 of the Russian Science Foundation (Section 3), the Russian Foundation for Basic research (grant 18-32-00460), the Russian Federation Ministry of Education and Science (agreem.: 3.9678.2017/8.9, 3.904.2017/4.6, 3.6787.2017/7.8, 3.6790.2017/7.8, 3.5917.2017/Bch, 19-72-20173) and by the European Union's Horizon 2020 programme (Grant No 653477). 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); 36th International Cosmic Ray Conference, ICRC 2019 ; Conference date: 24-07-2019 Through 01-08-2019",
year = "2021",
month = jul,
day = "2",
language = "English",
volume = "358",
journal = "Proceedings of Science",
issn = "1824-8039",
publisher = "Sissa Medialab Srl",

}

RIS

TY - JOUR

T1 - The hybrid installation TAIGA: design, status and preliminary results

AU - the TAIGA Collaboration

AU - Lubsandorzhiev, N.

AU - Astapov, I.

AU - Bezyazeekov, P.

AU - Borodin, A.

AU - Brueckner, M.

AU - Budnev, N.

AU - Chernykh, V.

AU - Chiavassa, A.

AU - Dyachok, A.

AU - Fedorov, O.

AU - Gafarov, A.

AU - Garmash, A.

AU - Grebenyuk, V.

AU - Gress, O.

AU - Gress, T.

AU - Grinyuk, A.

AU - Grishin, O.

AU - Horns, D.

AU - Igoshin, A.

AU - Ivanova, A.

AU - Kalmykov, N.

AU - Kazarina, Y.

AU - Kindin, V.

AU - Kirilenko, P.

AU - Kiryuhin, S.

AU - Kokoulin, R.

AU - Kompaniets, K.

AU - Korosteleva, E.

AU - Kozhin, V.

AU - Kravchenko, E.

AU - Kryukov, A.

AU - Kuzmichev, L.

AU - Lagutin, A.

AU - Lemeshev, Y.

AU - Lenok, V.

AU - Lubsandorzhiev, B.

AU - Mirgazov, R.

AU - Mirzoyan, R.

AU - Monkhoev, R.

AU - Osipova, E.

AU - Pakhorukov, A.

AU - Pan, A.

AU - Panasyuk, M.

AU - Pankov, L.

AU - Petrukhin, A.

AU - Poleschuk, V.

AU - Popesku, M.

AU - Rubtsov, G.

AU - Sokolov, A.

AU - Vaidyanathan, A.

N1 - Funding Information: This work was supported by the Russian Foundation for Basic Research, grant 16-29-13035, and the Russian Science Foundation (grant 19-72-20230, Section 4), grant 19-72-20067 of the Russian Science Foundation (Section 3), the Russian Foundation for Basic research (grant 18-32-00460), the Russian Federation Ministry of Education and Science (agreem.: 3.9678.2017/8.9, 3.904.2017/4.6, 3.6787.2017/7.8, 3.6790.2017/7.8, 3.5917.2017/Bch, 19-72-20173) and by the European Union's Horizon 2020 programme (Grant No 653477). 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 - 2021/7/2

Y1 - 2021/7/2

N2 - The hybrid installation TAIGA (Tunka Advanced Instrument for cosmic rays and Gamma Astronomy) is under construction to study cosmic and gamma rays at energies 1013-1018 eV. It will incorporate timing wide-angle EAS Cherenkov array (TAIGA-HiSCORE) and number of imaging atmospheric Cherenkov telescopes (TAIGA-IACT). The first stage of TAIGA will include ~100 wide-angle non-imaging optical stations of TAIGA-HiSCORE, distributed over an area of ~1 km2 and three imaging telescopes at a distance of 300-500 m from each other. A combined method will be used to distinguish gamma-rays namely EAS parameters will be reconstructed by TAIGA-HiSCORE and a gamma-hadron separation will be carried out by TAIGA-IACT. With such an approach a hybrid detector will be built with a large area but with a relatively small number of telescopes.

AB - The hybrid installation TAIGA (Tunka Advanced Instrument for cosmic rays and Gamma Astronomy) is under construction to study cosmic and gamma rays at energies 1013-1018 eV. It will incorporate timing wide-angle EAS Cherenkov array (TAIGA-HiSCORE) and number of imaging atmospheric Cherenkov telescopes (TAIGA-IACT). The first stage of TAIGA will include ~100 wide-angle non-imaging optical stations of TAIGA-HiSCORE, distributed over an area of ~1 km2 and three imaging telescopes at a distance of 300-500 m from each other. A combined method will be used to distinguish gamma-rays namely EAS parameters will be reconstructed by TAIGA-HiSCORE and a gamma-hadron separation will be carried out by TAIGA-IACT. With such an approach a hybrid detector will be built with a large area but with a relatively small number of telescopes.

UR - http://www.scopus.com/inward/record.url?scp=85086264565&partnerID=8YFLogxK

M3 - Conference article

AN - SCOPUS:85086264565

VL - 358

JO - Proceedings of Science

JF - Proceedings of Science

SN - 1824-8039

M1 - 729

T2 - 36th International Cosmic Ray Conference, ICRC 2019

Y2 - 24 July 2019 through 1 August 2019

ER -

ID: 35853259