The wide-aperture gamma-ray telescope TAIGA-HiSCORE in the Tunka Valley: Design, composition and commissioning

被引：38

作者：

Gress, O. ^{[2
]}

Astapov, I. ^{[9
]}

Budnev, N. ^{[2
]}

Bezyazeekov, P. ^{[2
]}

Bogdanov, A. ^{[2
,9
]}

Boreyko, V. ^{[10
]}

Brueckner, M. ^{[11
]}

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

Chvalaev, O. ^{[2
]}

Dyachok, A. ^{[2
]}

Gress, T. ^{[2
]}

Epimakhov, S. ^{[7
]}

Fedoseev, E. ^{[2
]}

Gafarov, A. ^{[2
]}

Gorbunov, N. ^{[10
]}

Grebenyuk, V. ^{[10
]}

Grinuk, A. ^{[10
]}

Grishin, O. ^{[2
]}

Horns, D. ^{[7
]}

Ivanova, A. ^{[2
]}

Kalinin, A. ^{[10
]}

Karpov, N. ^{[1
]}

Kalmykov, N. ^{[1
]}

Kazarina, Yu. ^{[2
]}

Kirichkov, N. ^{[2
]}

Kiryuhin, S. ^{[2
]}

Kokoulin, R. ^{[9
]}

Komponiest, K. ^{[9
]}

Korosteleva, E. ^{[1
]}

Kozhin, V. ^{[1
]}

Kunnas, M. ^{[7
]}

Kuzmichev, L. ^{[1
]}

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
]}

Panasyuk, M. ^{[1
]}

Pankov, L. ^{[2
]}

Petrukhin, A. ^{[9
]}

Platonov, V. ^{[2
]}

Poleschuk, V. ^{[2
]}

Popova, E. ^{[1
]}

Porelli, A. ^{[8
]}

Prosin, V. ^{[1
]}

Rubtsov, G. ^{[3
]}

Pushnin, A. ^{[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 Phys Expt, Hamburg, Germany

[8] DESY, Zeuthen, Germany

[9] NRNU MEPhI, Moscow, Russia

[10] JINR, Dubna, Russia

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

来源：

NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 2017年 / 845卷

基金：

俄罗斯科学基金会;

关键词：

Cosmic ray; Gamma-ray sources; Cherenkov light; Data acquisition system; COSMIC-RAY;

D O I：

10.1016/j.nima.2016.08.031

中图分类号：

TH7 [仪器、仪表];

学科分类号：

0804 ; 080401 ; 081102 ;

摘要：

The new TAIGA-HiSCORE non-imaging Cherenkov array aims to detect air showers induced by gamma rays above 30 TeV and to study cosmic rays above 100 TeV. TAIGA-HiSCORE is made of integrating air Cherenkov detector stations with a wide field of view (0.6 sr), placed at a distance of about 100 m. They cover an area of initially similar to 0.25 km(2) (prototype array), and of similar to 5 km(2) at the final phase of the experiment. Each station includes 4 PMTs with 20 or 25 cm diameter, equipped with light guides shaped as Winstone cones. We describe the design, specifications of the read-out, DAQand control and monitoring systems of the array. The present 28 detector stations of the TAIGA-HiSCORE engineering setup are in operation since September 2015. (C) 2016 Elsevier B.V. All rights reserved.

引用

页码：367 / 372

页数：6

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