The TAIGA experiment: from cosmic ray to gamma-ray astronomy in the Tunka valley

被引：19

作者：

Budnev, N. ^{[2
]}

Astapov, I. ^{[10
]}

Bezyazeekov, P. ^{[2
]}

Bogdanov, A. ^{[10
]}

Boreykom, V. ^{[11
]}

Bueker, M. ^{[7
]}

Brueckner, M. ^{[12
]}

Chiavassa, A. ^{[4
,5
]}

Chvalaev, O. ^{[2
]}

Gress, O. ^{[2
]}

Gress, T. ^{[2
]}

Grishin, O. ^{[2
]}

Dyachok, A. ^{[2
]}

Epimakhov, S. ^{[7
]}

Fedorov, O. ^{[2
]}

Gafarov, A. ^{[2
]}

Gorbunovi, N. ^{[11
]}

Grebenyukm, V. ^{[11
]}

Grinuk, A. ^{[11
]}

Haungsu, A. ^{[13
]}

Hilleru, R. ^{[13
]}

Horns, D. ^{[7
]}

Huege, T. ^{[1
]}

Ivanova, A. ^{[2
]}

Kalinin, A. ^{[11
]}

Karpov, N. ^{[1
]}

Kalmykovi, N. ^{[1
]}

Kazarina, Y. ^{[2
]}

Kirichkov, N. ^{[2
]}

Kiryuhin, S. ^{[2
]}

Kleifges, M. ^{[14
]}

Kokoulin, R. ^{[10
]}

Komponiest, K. ^{[10
]}

Konstantinovi, A. ^{[1
]}

Korosteleva, E. ^{[1
]}

Kostunin, D. ^{[2
,13
]}

Kozhini, V. ^{[1
]}

Kromer, O.

Kunnas, M. ^{[7
]}

Kuzmichevi, L. ^{[1
,2
]}

Lenok, V. ^{[2
]}

Lubsandorzhiev, B. ^{[3
]}

Lubsandorzhiev, N. ^{[1
]}

Mirgazov, R. ^{[2
]}

Mirzoyan, R. ^{[2
,6
]}

Monkhoev, R. ^{[2
]}

Nachtigall, R. ^{[7
]}

Pakhorukov, A. ^{[2
]}

Panasyuki, M. ^{[1
]}

Pankov, L. ^{[2
]}

机构：

[1] MSU, Skobeltsyn Inst Nucl Phys, Moscow, Russia

[2] ISU, Inst Appl Phys, Irkutsk, Russia

[3] RAN, Inst Nucl Res, Moscow, Russia

[4] Univ Torino, Dipartimento Fis Gen, Turin, Italy

[5] Ist Nazl Fis Nucl, Turin, Italy

[6] Max Planck Inst Phys & Astrophys, Munich, Germany

[7] Univ Hamburg, Inst Expt Phys, Hamburg, Germany

[8] IZMIRAN, Troitsk, Moscow Region, Russia

[9] DESY, Zeuthen, Germany

[10] NRNU, MEPhI, Moscow, Russia

[11] JINR, Dubna, Russia

[12] Humboldt Univ, Inst Comp Sci, Berlin, Germany

[13] KIT, Inst Kernphys, Karlsruhe, Germany

[14] KIT, Inst Prozessdatenverarbeitung & Elekt, Karlsruhe, Germany

来源：

XIV INTERNATIONAL CONFERENCE ON TOPICS IN ASTROPARTICLE AND UNDERGROUND PHYSICS (TAUP 2015), PTS 1-7 | 2016年 / 718卷

关键词：

D O I：

10.1088/1742-6596/718/5/052006

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The physical motivations and advantages of the new gamma-observatory TAIGA (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) is presented. The TAIGA array is a complex, hybrid detector for ground-based gamma-ray astronomy for energies from a few TeV to several PeV as well as for cosmic ray studies from 100 TeV to several EeV. The TAIGA will include the wide angle Cherenkov array TAIGA-HiSCORE with similar to 5 km(2) area, a net of 16 IACT telescopes (with FOV of about 10x10 degree), muon detectors with a total area of up to 2000-3000 m(2) and the radio array Tunka- Rex.

引用

页数：5

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