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The TAIGA-1 - A hybrid complex for gamma-ray astronomy, cosmic ray physics and astroparticle physics. / TAIGA Collaboration.

2023. Работа представлена на 38th International Cosmic Ray Conference, Nagoya, Япония.

Результаты исследований: Материалы конференцийматериалыРецензирование

Harvard

TAIGA Collaboration 2023, 'The TAIGA-1 - A hybrid complex for gamma-ray astronomy, cosmic ray physics and astroparticle physics', Работа представлена на 38th International Cosmic Ray Conference, Nagoya, Япония, 26.07.2023 - 03.08.2023. https://doi.org/10.22323/1.444.0269

APA

TAIGA Collaboration (2023). The TAIGA-1 - A hybrid complex for gamma-ray astronomy, cosmic ray physics and astroparticle physics. Работа представлена на 38th International Cosmic Ray Conference, Nagoya, Япония. https://doi.org/10.22323/1.444.0269

Vancouver

TAIGA Collaboration. The TAIGA-1 - A hybrid complex for gamma-ray astronomy, cosmic ray physics and astroparticle physics. 2023. Работа представлена на 38th International Cosmic Ray Conference, Nagoya, Япония. doi: 10.22323/1.444.0269

Author

TAIGA Collaboration. / The TAIGA-1 - A hybrid complex for gamma-ray astronomy, cosmic ray physics and astroparticle physics. Работа представлена на 38th International Cosmic Ray Conference, Nagoya, Япония.9 стр.

BibTeX

@conference{ba25feb9d7b94250873747910cb20b5a,
title = "The TAIGA-1 - A hybrid complex for gamma-ray astronomy, cosmic ray physics and astroparticle physics",
abstract = "The physical motivations and performance of the TAIGA (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) project are presented. The TAIGA astrophysical complex addresses ground-based gamma-ray astronomy at energies from a few TeV to several PeV and cosmic ray physics from 100 TeV to several EeV and astroparticle physics. The pilot TAIGA-1 complex is located in the Tunka valley, ~50 km west of the southern tip of lake Baikal. It includes a timing Cherenkov TAIGA-HiSCORE array with 120 wide-angle optical stations distributed over an area of about 1 square kilometer and three 4-m class Imaging Atmospheric Cherenkov Telescopes of the TAIGA-IACT array. The latter array has a shape of a triangle with side lengths of about 300m, 400m and 500m. There are three approaches to selecting gamma quanta from the hadron background in the TAIGA experiment: (1) IACT operation in standalone mode; (2) Stereo mode operation of two or more IACTs; (3) Hybrid mode operation -joint operation of TAIGAHiSCORE and IACTs. The main advantage of the hybrid operation of the IACTs and timing is their good gamma/hadron separation, even with only a few telescopes on the large area. Present status of the project, the first experimental results and plans for the future 10-20 km2 TAIGA are presented.",
author = "{the TAIGA Collaboration} and Arun Vaidyanathan and I Astapov and P Bezyazeekov and E Bonvech and A Borodin and Budnev, {N M} and A Bulan and D Chernov and A Chiavassa and Dyachok, {A N} and Gafarov, {A R} and A Garmash and V Grebenyuk and E Gress and O Gress and Gress, {T I} and A Grinyuk and O Grishin and Alexandra Ivanova and Anna Ivanova and M Iliushin and Kalmykov, {N N} and V Kindin and S Kiryuhin 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 Lagutin and Lavrova, {M V} and Yu Lemeshev and B Lubsandorzhiev and N Lubsandorzhiev and S Malakhov and Mirgazov, {R A} and R Monkhoev and E Okuneva and E Osipova and A Pakhorukov and L Pankov and A Pan and A Panov and A Petrukhin and D Podgrudkov and E Popova and A Sokolov",
note = "The work was performed at the UNU “Astrophysical Complex of MSU-ISU” (agreements 13.UNU.21.0007, EB-075-15-2021-675). The work is supported by the Russian Science Foundation (grants 23-72-00019 (Section 2, 3.1, 5), 23-72-00016 (Section1, 3.2. 4), the Russian Federation Ministry of Science and High Education (projects FZZE-2020-0024, FZZE-2023-0004, FSUS-2022-0015 and FSUS-2020-0039).; 38th International Cosmic Ray Conference, ICRC2023 ; Conference date: 26-07-2023 Through 03-08-2023",
year = "2023",
doi = "10.22323/1.444.0269",
language = "English",
url = "https://www.icrc2023.org/",

}

RIS

TY - CONF

T1 - The TAIGA-1 - A hybrid complex for gamma-ray astronomy, cosmic ray physics and astroparticle physics

AU - the TAIGA Collaboration

AU - Vaidyanathan, Arun

AU - Astapov, I

AU - Bezyazeekov, P

AU - Bonvech, E

AU - Borodin, A

AU - Budnev, N M

AU - Bulan, A

AU - Chernov, D

AU - Chiavassa, A

AU - Dyachok, A N

AU - Gafarov, A R

AU - Garmash, A

AU - Grebenyuk, V

AU - Gress, E

AU - Gress, O

AU - Gress, T I

AU - Grinyuk, A

AU - Grishin, O

AU - Ivanova, Alexandra

AU - Ivanova, Anna

AU - Iliushin, M

AU - Kalmykov, N N

AU - Kindin, V

AU - Kiryuhin, S

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 - Lagutin, A

AU - Lavrova, M V

AU - Lemeshev, Yu

AU - Lubsandorzhiev, B

AU - Lubsandorzhiev, N

AU - Malakhov, S

AU - Mirgazov, R A

AU - Monkhoev, R

AU - Okuneva, E

AU - Osipova, E

AU - Pakhorukov, A

AU - Pankov, L

AU - Pan, A

AU - Panov, A

AU - Petrukhin, A

AU - Podgrudkov, D

AU - Popova, E

AU - Sokolov, A

N1 - Conference code: 38

PY - 2023

Y1 - 2023

N2 - The physical motivations and performance of the TAIGA (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) project are presented. The TAIGA astrophysical complex addresses ground-based gamma-ray astronomy at energies from a few TeV to several PeV and cosmic ray physics from 100 TeV to several EeV and astroparticle physics. The pilot TAIGA-1 complex is located in the Tunka valley, ~50 km west of the southern tip of lake Baikal. It includes a timing Cherenkov TAIGA-HiSCORE array with 120 wide-angle optical stations distributed over an area of about 1 square kilometer and three 4-m class Imaging Atmospheric Cherenkov Telescopes of the TAIGA-IACT array. The latter array has a shape of a triangle with side lengths of about 300m, 400m and 500m. There are three approaches to selecting gamma quanta from the hadron background in the TAIGA experiment: (1) IACT operation in standalone mode; (2) Stereo mode operation of two or more IACTs; (3) Hybrid mode operation -joint operation of TAIGAHiSCORE and IACTs. The main advantage of the hybrid operation of the IACTs and timing is their good gamma/hadron separation, even with only a few telescopes on the large area. Present status of the project, the first experimental results and plans for the future 10-20 km2 TAIGA are presented.

AB - The physical motivations and performance of the TAIGA (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) project are presented. The TAIGA astrophysical complex addresses ground-based gamma-ray astronomy at energies from a few TeV to several PeV and cosmic ray physics from 100 TeV to several EeV and astroparticle physics. The pilot TAIGA-1 complex is located in the Tunka valley, ~50 km west of the southern tip of lake Baikal. It includes a timing Cherenkov TAIGA-HiSCORE array with 120 wide-angle optical stations distributed over an area of about 1 square kilometer and three 4-m class Imaging Atmospheric Cherenkov Telescopes of the TAIGA-IACT array. The latter array has a shape of a triangle with side lengths of about 300m, 400m and 500m. There are three approaches to selecting gamma quanta from the hadron background in the TAIGA experiment: (1) IACT operation in standalone mode; (2) Stereo mode operation of two or more IACTs; (3) Hybrid mode operation -joint operation of TAIGAHiSCORE and IACTs. The main advantage of the hybrid operation of the IACTs and timing is their good gamma/hadron separation, even with only a few telescopes on the large area. Present status of the project, the first experimental results and plans for the future 10-20 km2 TAIGA are presented.

UR - https://www.mendeley.com/catalogue/b69e7e3b-aae9-37e1-b5f3-02b06d9d86b8/

U2 - 10.22323/1.444.0269

DO - 10.22323/1.444.0269

M3 - Paper

T2 - 38th International Cosmic Ray Conference

Y2 - 26 July 2023 through 3 August 2023

ER -

ID: 60224391