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Evaluation of Angular Resolution and Effective Area of the TAIGA-HiSCORE Installation Using Peripheral Stations. / the TAIGA Collaboration; Lemeshev, Yu E.; Lubsandorzhiev, Bayarto et al.

In: Bulletin of the Russian Academy of Sciences: Physics, 10.06.2025.

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

Harvard

the TAIGA Collaboration, Lemeshev, YE, Lubsandorzhiev, B, Lubsandorzhiev, NB, Lukanov, A, Malakhov, SD, Mirgazov, R, Okuneva, E, Pakhorukov, AL, Pankov, L, Pan, A, Petrukhin, AA, Poddubny, I, Podgrudkov, D, Poleschuk, VA, Postnikov, EB, Prosin, V, Pushnin, A, Raikin, R, Satyshev, I, Silaev, A, Silaev Junior, AA, Sidorenkov, A, Sveshnikova, LG, Tabolenko, VA, Tkachev, LG, Tanaev, AB, Ternovoy, M, Volchugov, P, Zagorodnikov, AV, Zhurov, D, Zirakashvili, V & Yashin, I 2025, 'Evaluation of Angular Resolution and Effective Area of the TAIGA-HiSCORE Installation Using Peripheral Stations', Bulletin of the Russian Academy of Sciences: Physics. https://doi.org/10.1134/S1062873825712164

APA

the TAIGA Collaboration, Lemeshev, Y. E., Lubsandorzhiev, B., Lubsandorzhiev, N. B., Lukanov, A., Malakhov, S. D., Mirgazov, R., Okuneva, E., Pakhorukov, A. L., Pankov, L., Pan, A., Petrukhin, A. A., Poddubny, I., Podgrudkov, D., Poleschuk, V. A., Postnikov, E. B., Prosin, V., Pushnin, A., Raikin, R., ... Yashin, I. (2025). Evaluation of Angular Resolution and Effective Area of the TAIGA-HiSCORE Installation Using Peripheral Stations. Bulletin of the Russian Academy of Sciences: Physics. https://doi.org/10.1134/S1062873825712164

Vancouver

the TAIGA Collaboration, Lemeshev YE, Lubsandorzhiev B, Lubsandorzhiev NB, Lukanov A, Malakhov SD et al. Evaluation of Angular Resolution and Effective Area of the TAIGA-HiSCORE Installation Using Peripheral Stations. Bulletin of the Russian Academy of Sciences: Physics. 2025 Jun 10. doi: 10.1134/S1062873825712164

Author

the TAIGA Collaboration ; Lemeshev, Yu E. ; Lubsandorzhiev, Bayarto et al. / Evaluation of Angular Resolution and Effective Area of the TAIGA-HiSCORE Installation Using Peripheral Stations. In: Bulletin of the Russian Academy of Sciences: Physics. 2025.

BibTeX

@article{56fb8b1a5d5a4c26aa72e21b12eb582e,
title = "Evaluation of Angular Resolution and Effective Area of the TAIGA-HiSCORE Installation Using Peripheral Stations",
abstract = "Abstract: We presented the results of a computer modeling of the TAIGA-HiSCORE installation in an extended configuration. TAIGA-HiSCORE is a 1 km2 grid of 120 optical stations designed for EAS detection with angular resolution of ∼0.1°. High angular resolution is necessary for gamma-ray astronomy because it allows better suppression of the cosmic ray background and better determination of the location of the sources. The further the EAS axis is from the perimeter of the installation, the worse the angular resolution. It is shown that the placement of additional peripheral stations not only increases the effective area of the installation, but also significantly improves the angular resolution of edge and outer events from 0.4°–1° to 0.15°–0.3°.",
keywords = "CORSIKA, TAIGA-HiSCORE, angular resolution, extensive air showers",
author = "{the TAIGA Collaboration} and V. Samoliga and I. Astapov and P. Bezyazeekov and A. Blinov and Bonvech, {E. A.} and A. Borodin and N. Budnev and A. Bulan and P. Busygin and A. Chernov and A. Chiavassa and A. Dyachok and V. Erofeeva and A. Gafarov and A. Garmash and V. Grebenyuk and E. Gress and O. Gress and T. Gress and A. Grinyuk and O. Grishin and Ivanova, {A. D.} and Ivanova, {A. L.} and M. Iliushin and I. Kabannik and N. Kalmykov and V. Kindin and S. Kiryuhin 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 M. Lavrova and R. Monkhoev and E. Osipova and A. Panov and E. Popova and A. Razumov and G. Rubtsov and E. Ryabov and M. Shulga and A. Skurikhin and A. Sokolov and N. Ushakov and N. Volkov and D. Voronin and Lemeshev, {Yu E.} and Bayarto Lubsandorzhiev and Lubsandorzhiev, {N. B.} and Arslan Lukanov and Malakhov, {S. D.} and R. Mirgazov and E. Okuneva and Pakhorukov, {A. L.} and L. Pankov and A. Pan and A.A. Petrukhin and I. Poddubny and D. Podgrudkov and Poleschuk, {V. A.} and Postnikov, {E. B.} and V. Prosin and A. Pushnin and R. Raikin and I. Satyshev and A. Silaev and {Silaev Junior}, {A. A.} and Andrei Sidorenkov and Sveshnikova, {L. G.} and Tabolenko, {V. A.} and Tkachev, {L. G.} and Tanaev, {A. B.} and M. Ternovoy and P. Volchugov and Zagorodnikov, {A. V.} and D. Zhurov and V. Zirakashvili and I. Yashin",
note = "The work was carried out at the unique scientific installation “Astrophysical Complex MSU-ISU”. Supported by the Russian Federation Ministry of Science and Higher Education (project nos. FZZE-2023-0004, FZZE-2024-0005, and FSUS- 2022-0015) and Russian Science Foundation (project no. 23-72-00016 (section “Modeling and data analysis”)). ",
year = "2025",
month = jun,
day = "10",
doi = "10.1134/S1062873825712164",
language = "English",
journal = "Bulletin of the Russian Academy of Sciences: Physics",
issn = "1062-8738",
publisher = "Pleiades Publishing",

}

RIS

TY - JOUR

T1 - Evaluation of Angular Resolution and Effective Area of the TAIGA-HiSCORE Installation Using Peripheral Stations

AU - the TAIGA Collaboration

AU - Samoliga, V.

AU - Astapov, I.

AU - Bezyazeekov, P.

AU - Blinov, A.

AU - Bonvech, E. A.

AU - Borodin, A.

AU - Budnev, N.

AU - Bulan, A.

AU - Busygin, P.

AU - Chernov, A.

AU - Chiavassa, A.

AU - Dyachok, A.

AU - Erofeeva, V.

AU - Gafarov, A.

AU - Garmash, A.

AU - Grebenyuk, V.

AU - Gress, E.

AU - Gress, O.

AU - Gress, T.

AU - Grinyuk, A.

AU - Grishin, O.

AU - Ivanova, A. D.

AU - Ivanova, A. L.

AU - Iliushin, M.

AU - Kabannik, I.

AU - Kalmykov, N.

AU - Kindin, V.

AU - Kiryuhin, S.

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.

AU - Monkhoev, R.

AU - Osipova, E.

AU - Panov, A.

AU - Popova, E.

AU - Razumov, A.

AU - Rubtsov, G.

AU - Ryabov, E.

AU - Shulga, M.

AU - Skurikhin, A.

AU - Sokolov, A.

AU - Ushakov, N.

AU - Volkov, N.

AU - Voronin, D.

AU - Lemeshev, Yu E.

AU - Lubsandorzhiev, Bayarto

AU - Lubsandorzhiev, N. B.

AU - Lukanov, Arslan

AU - Malakhov, S. D.

AU - Mirgazov, R.

AU - Okuneva, E.

AU - Pakhorukov, A. L.

AU - Pankov, L.

AU - Pan, A.

AU - Petrukhin, A.A.

AU - Poddubny, I.

AU - Podgrudkov, D.

AU - Poleschuk, V. A.

AU - Postnikov, E. B.

AU - Prosin, V.

AU - Pushnin, A.

AU - Raikin, R.

AU - Satyshev, I.

AU - Silaev, A.

AU - Silaev Junior, A. A.

AU - Sidorenkov, Andrei

AU - Sveshnikova, L. G.

AU - Tabolenko, V. A.

AU - Tkachev, L. G.

AU - Tanaev, A. B.

AU - Ternovoy, M.

AU - Volchugov, P.

AU - Zagorodnikov, A. V.

AU - Zhurov, D.

AU - Zirakashvili, V.

AU - Yashin, I.

N1 - The work was carried out at the unique scientific installation “Astrophysical Complex MSU-ISU”. Supported by the Russian Federation Ministry of Science and Higher Education (project nos. FZZE-2023-0004, FZZE-2024-0005, and FSUS- 2022-0015) and Russian Science Foundation (project no. 23-72-00016 (section “Modeling and data analysis”)).

PY - 2025/6/10

Y1 - 2025/6/10

N2 - Abstract: We presented the results of a computer modeling of the TAIGA-HiSCORE installation in an extended configuration. TAIGA-HiSCORE is a 1 km2 grid of 120 optical stations designed for EAS detection with angular resolution of ∼0.1°. High angular resolution is necessary for gamma-ray astronomy because it allows better suppression of the cosmic ray background and better determination of the location of the sources. The further the EAS axis is from the perimeter of the installation, the worse the angular resolution. It is shown that the placement of additional peripheral stations not only increases the effective area of the installation, but also significantly improves the angular resolution of edge and outer events from 0.4°–1° to 0.15°–0.3°.

AB - Abstract: We presented the results of a computer modeling of the TAIGA-HiSCORE installation in an extended configuration. TAIGA-HiSCORE is a 1 km2 grid of 120 optical stations designed for EAS detection with angular resolution of ∼0.1°. High angular resolution is necessary for gamma-ray astronomy because it allows better suppression of the cosmic ray background and better determination of the location of the sources. The further the EAS axis is from the perimeter of the installation, the worse the angular resolution. It is shown that the placement of additional peripheral stations not only increases the effective area of the installation, but also significantly improves the angular resolution of edge and outer events from 0.4°–1° to 0.15°–0.3°.

KW - CORSIKA

KW - TAIGA-HiSCORE

KW - angular resolution

KW - extensive air showers

UR - https://www.mendeley.com/catalogue/9195fbe1-6d4d-3934-80b3-7523841fdb75/

UR - https://www.scopus.com/record/display.uri?eid=2-s2.0-105007603256&origin=inward&txGid=a1f8b4887b5b033c8ae857745bdbd664

U2 - 10.1134/S1062873825712164

DO - 10.1134/S1062873825712164

M3 - Article

JO - Bulletin of the Russian Academy of Sciences: Physics

JF - Bulletin of the Russian Academy of Sciences: Physics

SN - 1062-8738

ER -

ID: 67894038