The new Tunka-133 EAS Cherenkov array: Status of 2009

B V Antokhonov ,S.F Beregnev,R Wischnewski,L Pankov ,A V Zablotsky ,В С Птускин ,Р Р Миргазов ,Yu Semeney ,L A Kuzmichev ,I V Yashin ,Б Лубсандоржиев ,M I Panasyuk ,Е Е Коростелева ,А В Скурихин ,В А Кожин ,C Spiering ,Н Буднев ,O Chvalaev ,N Karpov ,А Чиавасса ,O Gress ,Б А Шайбонов ,Н Н Калмыков ,В В Просин ,А Силаев ,А Загородников

doi:10.1016/j.nima.2010.11.027

The new Tunka-133 EAS Cherenkov array: Status of 2009

B V Antokhonov , S.F Beregnev + Show 24 more

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https://doi.org/10.1016/j.nima.2010.11.027

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Journal: Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment	Publication Date: Nov 10, 2010
Citations: 8	License type: other-oa

Affiliation: Lomonosov Moscow State University, Deutsches Elektronen-Synchrotron DESY, Irkutsk State University, Institute of Applied Physics, Institute of Terrestrial Magnetism Ionosphere and Radio Wave Propagation, Institute for Nuclear Research, University of Turin

#Array Construction #Elaborate Method + Show 8 more

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Abstract

The deployment of the new Extensive air shower Cherenkov installation Tunka-133 with about 1 km 2 geometric acceptance area was completed in October 2009. The array will permit a detailed long-term study of the cosmic ray energy spectrum and mass composition in the energy range 10 15–10 18 eV with a unique and more elaborate method. The array construction and data acquisition system, preliminary results and plans for future development are presented.

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