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The Optical Throughput Calibration of the TAIGA-IACT Facility. / the TAIGA Collaboration.

In: Physics of Particles and Nuclei, Vol. 56, No. 3, 27.06.2025, p. 643-646.

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

Harvard

the TAIGA Collaboration 2025, 'The Optical Throughput Calibration of the TAIGA-IACT Facility', Physics of Particles and Nuclei, vol. 56, no. 3, pp. 643-646. https://doi.org/10.1134/S1063779624702058

APA

the TAIGA Collaboration (2025). The Optical Throughput Calibration of the TAIGA-IACT Facility. Physics of Particles and Nuclei, 56(3), 643-646. https://doi.org/10.1134/S1063779624702058

Vancouver

the TAIGA Collaboration. The Optical Throughput Calibration of the TAIGA-IACT Facility. Physics of Particles and Nuclei. 2025 Jun 27;56(3):643-646. doi: 10.1134/S1063779624702058

Author

the TAIGA Collaboration. / The Optical Throughput Calibration of the TAIGA-IACT Facility. In: Physics of Particles and Nuclei. 2025 ; Vol. 56, No. 3. pp. 643-646.

BibTeX

@article{24f49d81a5554ea4a203c27e74bb5136,
title = "The Optical Throughput Calibration of the TAIGA-IACT Facility",
abstract = "Abstract: The optical throughput of Imaging Atmospheric Cherenkov Telescopes (IACTs) is an important detector characteristic used to reconstruct the parameters of detected events. The TAIGA astrophysical complex includes TAIGA-IACT facility—an array of three IACTs and 120 TAIGA-HiSCORE wide-angle Cherenkov detectors on an area of 1 km2. The complex is aimed at solving the relevant problems in gamma-astronomy of very high energies (VHE) and ultra high energies (UHE). The TAIGA-HiSCORE complex makes it possible to reconstruct the lateral distribution function (LDF) of Cherenkov photons in an extensive air shower (EAS). This information makes it possible to determine the number of Cherenkov photons reaching IACT reflectors and, eventually, to determine the efficiency of their detection. The present paper describes this approach to calibrating the optical throughput of the TAIGA-IACT facility.",
author = "{the TAIGA Collaboration} and Blinov, {A. V.} and Borodin, {A. N.} and Bonvech, {E. A.} and Budnev, {N. M.} and Bulan, {A. V.} and Volkov, {N. V.} and Voronin, {D. M.} and Gafarov, {A. R.} and Gres{\textquoteright}, {E. O.} and Gres{\textquoteright}, {O. A.} and Gres{\textquoteright}, {T. I.} and Grishin, {O. G.} and Garmash, {A. Yu} and Grebenyuk, {V. M.} and Grinyuk, {A. A.} and Dyachok, {A. N.} and Zhurov, {D. P.} and Zagorodnikov, {A. V.} and Zirakashvili, {V. N.} and Ivanova, {A. L.} and Ivanova, {A. D.} and Ilyushin, {M. A.} and Kalmykov, {N. N.} and Kindin, {V. V.} and Kiryuhin, {S. N.} and Kokoulin, {R. P.} and Kolosov, {N. I.} and Kompaniets, {K. G.} and Korosteleva, {E. E.} and Kozhin, {V. A.} and Kravchenko, {E. A.} and Kryukov, {A. P.} and Kuzmichev, {L. A.} and A. Chiavassa and Lavrova, {M. V.} and Lagutin, {A. A.} and Monkhoev, {R. D.} and Osipova, {E. A.} and Panov, {A. D.} and Popova, {E. G.} and Rubtsov, {G. I.} and Ryabov, {E. V.} and Samoliga, {V. S.} and Skurikhin, {A. V.} and Sokolov, {A. V.} and Ushakov, {N. A.} and Chernov, {D. V.}",
note = "This study was supported by the Russian Science Foundation (project no. 23-72-00016, section 2 and project no. 23-72-00019, section 3) and state assignments from the Ministry of Science and Higher Education (projects nos. FZZE-2023-0004 and FZZE-2024-0005). The Optical Throughput Calibration of the TAIGA-IACT Facility / P. A. Volchugov, I. I. Astapov, P. A. Bez''yazykov [et al.] // Physics of Particles and Nuclei. – 2025. – Vol. 56, No. 3. – P. 643-646. – DOI 10.1134/S1063779624702058.",
year = "2025",
month = jun,
day = "27",
doi = "10.1134/S1063779624702058",
language = "English",
volume = "56",
pages = "643--646",
journal = "Physics of Particles and Nuclei",
issn = "1063-7796",
publisher = "Maik Nauka-Interperiodica Publishing",
number = "3",

}

RIS

TY - JOUR

T1 - The Optical Throughput Calibration of the TAIGA-IACT Facility

AU - the TAIGA Collaboration

AU - Blinov, A. V.

AU - Borodin, A. N.

AU - Bonvech, E. A.

AU - Budnev, N. M.

AU - Bulan, A. V.

AU - Volkov, N. V.

AU - Voronin, D. M.

AU - Gafarov, A. R.

AU - Gres’, E. O.

AU - Gres’, O. A.

AU - Gres’, T. I.

AU - Grishin, O. G.

AU - Garmash, A. Yu

AU - Grebenyuk, V. M.

AU - Grinyuk, A. A.

AU - Dyachok, A. N.

AU - Zhurov, D. P.

AU - Zagorodnikov, A. V.

AU - Zirakashvili, V. N.

AU - Ivanova, A. L.

AU - Ivanova, A. D.

AU - Ilyushin, M. A.

AU - Kalmykov, N. N.

AU - Kindin, V. V.

AU - Kiryuhin, S. N.

AU - Kokoulin, R. P.

AU - Kolosov, N. I.

AU - Kompaniets, K. G.

AU - Korosteleva, E. E.

AU - Kozhin, V. A.

AU - Kravchenko, E. A.

AU - Kryukov, A. P.

AU - Kuzmichev, L. A.

AU - Chiavassa, A.

AU - Lavrova, M. V.

AU - Lagutin, A. A.

AU - Monkhoev, R. D.

AU - Osipova, E. A.

AU - Panov, A. D.

AU - Popova, E. G.

AU - Rubtsov, G. I.

AU - Ryabov, E. V.

AU - Samoliga, V. S.

AU - Skurikhin, A. V.

AU - Sokolov, A. V.

AU - Ushakov, N. A.

AU - Chernov, D. V.

N1 - This study was supported by the Russian Science Foundation (project no. 23-72-00016, section 2 and project no. 23-72-00019, section 3) and state assignments from the Ministry of Science and Higher Education (projects nos. FZZE-2023-0004 and FZZE-2024-0005). The Optical Throughput Calibration of the TAIGA-IACT Facility / P. A. Volchugov, I. I. Astapov, P. A. Bez''yazykov [et al.] // Physics of Particles and Nuclei. – 2025. – Vol. 56, No. 3. – P. 643-646. – DOI 10.1134/S1063779624702058.

PY - 2025/6/27

Y1 - 2025/6/27

N2 - Abstract: The optical throughput of Imaging Atmospheric Cherenkov Telescopes (IACTs) is an important detector characteristic used to reconstruct the parameters of detected events. The TAIGA astrophysical complex includes TAIGA-IACT facility—an array of three IACTs and 120 TAIGA-HiSCORE wide-angle Cherenkov detectors on an area of 1 km2. The complex is aimed at solving the relevant problems in gamma-astronomy of very high energies (VHE) and ultra high energies (UHE). The TAIGA-HiSCORE complex makes it possible to reconstruct the lateral distribution function (LDF) of Cherenkov photons in an extensive air shower (EAS). This information makes it possible to determine the number of Cherenkov photons reaching IACT reflectors and, eventually, to determine the efficiency of their detection. The present paper describes this approach to calibrating the optical throughput of the TAIGA-IACT facility.

AB - Abstract: The optical throughput of Imaging Atmospheric Cherenkov Telescopes (IACTs) is an important detector characteristic used to reconstruct the parameters of detected events. The TAIGA astrophysical complex includes TAIGA-IACT facility—an array of three IACTs and 120 TAIGA-HiSCORE wide-angle Cherenkov detectors on an area of 1 km2. The complex is aimed at solving the relevant problems in gamma-astronomy of very high energies (VHE) and ultra high energies (UHE). The TAIGA-HiSCORE complex makes it possible to reconstruct the lateral distribution function (LDF) of Cherenkov photons in an extensive air shower (EAS). This information makes it possible to determine the number of Cherenkov photons reaching IACT reflectors and, eventually, to determine the efficiency of their detection. The present paper describes this approach to calibrating the optical throughput of the TAIGA-IACT facility.

UR - https://www.mendeley.com/catalogue/4cd4e56b-3d97-3fdc-936f-0ffbd00cd813/

UR - https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=105009333095&origin=inward

UR - https://www.elibrary.ru/item.asp?id=82558452

U2 - 10.1134/S1063779624702058

DO - 10.1134/S1063779624702058

M3 - Article

VL - 56

SP - 643

EP - 646

JO - Physics of Particles and Nuclei

JF - Physics of Particles and Nuclei

SN - 1063-7796

IS - 3

ER -

ID: 68293127