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TAIGA experiment : Present status and perspectives. / the TAIGA Collaboration.

In: Journal of Instrumentation, Vol. 12, No. 8, C08018, 16.08.2017.

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Harvard

the TAIGA Collaboration 2017, 'TAIGA experiment: Present status and perspectives', Journal of Instrumentation, vol. 12, no. 8, C08018. https://doi.org/10.1088/1748-0221/12/08/C08018

APA

the TAIGA Collaboration (2017). TAIGA experiment: Present status and perspectives. Journal of Instrumentation, 12(8), [C08018]. https://doi.org/10.1088/1748-0221/12/08/C08018

Vancouver

the TAIGA Collaboration. TAIGA experiment: Present status and perspectives. Journal of Instrumentation. 2017 Aug 16;12(8):C08018. doi: 10.1088/1748-0221/12/08/C08018

Author

the TAIGA Collaboration. / TAIGA experiment : Present status and perspectives. In: Journal of Instrumentation. 2017 ; Vol. 12, No. 8.

BibTeX

@article{c72167f063c045b0992c507620f7be5f,
title = "TAIGA experiment: Present status and perspectives",
abstract = "The TAIGA observatory addresses ground-based gamma-ray astronomy at energies from a few TeV to several PeV, as well as cosmic ray physics from 100 TeV to several EeV . TAIGA will be located in the Tunka valley, ∼ 50 km West from Lake Baikal. The different detectors of the TAIGA will be grouped in 6 arrays to measure Cherenkov and radio emission as well as electron and muon components of atmospheric showers. The combination of the wide angle Cherenkov detectors of the TAIGA-HiSCORE array and the 4-m Imaging Atmospheric Cherenkov Telescopes of the TAIGA-IACT array with their FoV of 10×10 degrees and underground muon detectors offers a very cost effective way to construct a 5 km2 array for gamma-ray astronomy.",
keywords = "Cherenkov detectors, Gamma telescopes, Image processing, HISCORE, RAY",
author = "{the TAIGA Collaboration} and N. Budnev and I. Astapov and P. Bezyazeekov and V. Boreyko and A. Borodin and M. Br{\"u}ckner and A. Chiavassa and A. Gafarov and V. Grebenyuk and O. Gress and T. Gress and A. Grinyuk and O. Grishin and A. Dyachok and O. Fedorov and A. Haungs and D. Horns and T. Huege and A. Ivanova and N. Kalmykov and Y. Kazarina and V. Kindin and S. Kiryuhin and R. Kokoulin and K. Kompaniets and D. Kostunin and E. Korosteleva and V. Kozhin and E. Kravchenko and M. Kunnas and L. Kuzmichev and Yu Lemeshev and V. Lenok and B. Lubsandorzhiev and N. Lubsandorzhiev and R. Mirgazov and R. Mirzoyan and R. Monkhoev and R. Nachtigall and E. Osipova and A. Pakhorukov and M. Panasyuk and L. Pankov and V. Poleschuk and M. Popesku and E. Popova and A. Porelli and E. Postnikov and V. Prosin and A. Sokolov",
year = "2017",
month = aug,
day = "16",
doi = "10.1088/1748-0221/12/08/C08018",
language = "English",
volume = "12",
journal = "Journal of Instrumentation",
issn = "1748-0221",
publisher = "IOP Publishing Ltd.",
number = "8",

}

RIS

TY - JOUR

T1 - TAIGA experiment

T2 - Present status and perspectives

AU - the TAIGA Collaboration

AU - Budnev, N.

AU - Astapov, I.

AU - Bezyazeekov, P.

AU - Boreyko, V.

AU - Borodin, A.

AU - Brückner, M.

AU - Chiavassa, A.

AU - Gafarov, A.

AU - Grebenyuk, V.

AU - Gress, O.

AU - Gress, T.

AU - Grinyuk, A.

AU - Grishin, O.

AU - Dyachok, A.

AU - Fedorov, O.

AU - Haungs, A.

AU - Horns, D.

AU - Huege, T.

AU - Ivanova, A.

AU - Kalmykov, N.

AU - Kazarina, Y.

AU - Kindin, V.

AU - Kiryuhin, S.

AU - Kokoulin, R.

AU - Kompaniets, K.

AU - Kostunin, D.

AU - Korosteleva, E.

AU - Kozhin, V.

AU - Kravchenko, E.

AU - Kunnas, M.

AU - Kuzmichev, L.

AU - Lemeshev, Yu

AU - Lenok, V.

AU - Lubsandorzhiev, B.

AU - Lubsandorzhiev, N.

AU - Mirgazov, R.

AU - Mirzoyan, R.

AU - Monkhoev, R.

AU - Nachtigall, R.

AU - Osipova, E.

AU - Pakhorukov, A.

AU - Panasyuk, M.

AU - Pankov, L.

AU - Poleschuk, V.

AU - Popesku, M.

AU - Popova, E.

AU - Porelli, A.

AU - Postnikov, E.

AU - Prosin, V.

AU - Sokolov, A.

PY - 2017/8/16

Y1 - 2017/8/16

N2 - The TAIGA observatory addresses ground-based gamma-ray astronomy at energies from a few TeV to several PeV, as well as cosmic ray physics from 100 TeV to several EeV . TAIGA will be located in the Tunka valley, ∼ 50 km West from Lake Baikal. The different detectors of the TAIGA will be grouped in 6 arrays to measure Cherenkov and radio emission as well as electron and muon components of atmospheric showers. The combination of the wide angle Cherenkov detectors of the TAIGA-HiSCORE array and the 4-m Imaging Atmospheric Cherenkov Telescopes of the TAIGA-IACT array with their FoV of 10×10 degrees and underground muon detectors offers a very cost effective way to construct a 5 km2 array for gamma-ray astronomy.

AB - The TAIGA observatory addresses ground-based gamma-ray astronomy at energies from a few TeV to several PeV, as well as cosmic ray physics from 100 TeV to several EeV . TAIGA will be located in the Tunka valley, ∼ 50 km West from Lake Baikal. The different detectors of the TAIGA will be grouped in 6 arrays to measure Cherenkov and radio emission as well as electron and muon components of atmospheric showers. The combination of the wide angle Cherenkov detectors of the TAIGA-HiSCORE array and the 4-m Imaging Atmospheric Cherenkov Telescopes of the TAIGA-IACT array with their FoV of 10×10 degrees and underground muon detectors offers a very cost effective way to construct a 5 km2 array for gamma-ray astronomy.

KW - Cherenkov detectors

KW - Gamma telescopes

KW - Image processing

KW - HISCORE

KW - RAY

UR - http://www.scopus.com/inward/record.url?scp=85030996004&partnerID=8YFLogxK

U2 - 10.1088/1748-0221/12/08/C08018

DO - 10.1088/1748-0221/12/08/C08018

M3 - Article

AN - SCOPUS:85030996004

VL - 12

JO - Journal of Instrumentation

JF - Journal of Instrumentation

SN - 1748-0221

IS - 8

M1 - C08018

ER -

ID: 12669628