/ Astrophysics


Tunka Advanced Instrument for cosmic rays and Gamma Astronomy (TAIGA): Status, results and perspectives


Kuzmichev, L. (Irkutsk State U.) ; Astapov, I. (Moscow Phys. Eng. Inst.) ; Bezyazeekov, P. (Irkutsk State U.) ; Boreyko, V. (Dubna, JINR) ; Borodin, A. (Dubna, JINR) ; Brückner, M. (DESY, Zeuthen) ; Budnev, N. (Irkutsk State U.) ; Chiavassa, A. (Turin U.) ; Gress, O. (Irkutsk State U.) ; Gress, T. (Irkutsk State U.) ; Grishin, O. (Irkutsk State U.) ; Dyachok, A. (Irkutsk State U.) ; Epimakhov, S. (SINP, Moscow) ; Fedorov, O. (Irkutsk State U.) ; Gafarov, A. (Irkutsk State U.) ; Grebenyuk, V. (Dubna, JINR) ; Grinyuk, A. (Dubna, JINR) ; Haungs, A. (KIT, Karlsruhe, IKP) ; Horns, D. (Hamburg U.) ; Huege, T. (KIT, Karlsruhe, IKP) ; Ivanova, A. (Irkutsk State U.) ; Jurov, D. (Irkutsk State U.) ; Kalmykov, N. (SINP, Moscow) ; Kazarina, Y. (Irkutsk State U.) ; Kindin, V. (Moscow Phys. Eng. Inst.) ; Kiryuhin, V. (Irkutsk State U.) ; Kokoulin, R. (Moscow Phys. Eng. Inst.) ; Kompaniets, K. (Moscow Phys. Eng. Inst.) ; Korosteleva, E. (SINP, Moscow) ; Kostunin, D. (KIT, Karlsruhe, IKP) ; Kozhin, V. (SINP, Moscow) ; Kravchenko, E. (Novosibirsk, IYF) ; Kunnas, M. (Hamburg U.) ; Lenok, V. (Irkutsk State U.) ; Lubsandorzhiev, B. (Moscow, INR) ; Lubsandorzhiev, N. (SINP, Moscow) ; Mirgazov, R. (Irkutsk State U.) ; Mirzoyan, R. (Munich, Max Planck Inst.) ; Monkhoev, R. (Irkutsk State U.) ; Nachtigal, R. (Hamburg U.) ; Osipova, E. (SINP, Moscow) ; Pakharukov, A. (Irkutsk State U.) ; Panasyuk, M. (SINP, Moscow) ; Pankov, L. (Irkutsk State U.) ; Petrukhin, A. (Moscow Phys. Eng. Inst.) ; Poleschuk, V. (Irkutsk State U.) ; Popesku, M. (Bucharest, Inst. Space Science) ; Popova, E. (SINP, Moscow) ; Porelli, A. (DESY, Zeuthen) ; Postnikov, E. (SINP, Moscow) ; Prosin, V. (SINP, Moscow) ; Ptuskin, V. (Troitsk, IZMIRAN) ; Pushnin, A. (Irkutsk State U.) ; Rubtsov, G. (Moscow, INR) ; Ryabov, E. (Irkutsk State U.) ; Sagan, Y. (Dubna, JINR) ; Samoliga, V. (Irkutsk State U.) ; Schröder, F.G. (KIT, Karlsruhe, IKP) ; Semeney, Yu. (Irkutsk State U.) ; Silaev, A. (SINP, Moscow) ; Sidorenko, A. (Moscow, INR) ; Skurikhin, A. (SINP, Moscow) ; Slunecka, V. (Dubna, JINR) ; Sokolov, A. (Novosibirsk, IYF) ; Spiering, C. (DESY, Zeuthen) ; Sveshnikova, L. (SINP, Moscow) ; Sulakov, V. (SINP, Moscow) ; Tabolenko, V. (Irkutsk State U.) ; Tarashansky, B. (Irkutsk State U.) ; Tkachenko, A. (Dubna, JINR) ; Tkachev, L. (Dubna, JINR) ; Tluczykont, M. (Hamburg U.) ; Wischnewski, R. (DESY, Zeuthen) ; Zagorodnikov, A. (Irkutsk State U.) ; Zurbanov, V. (Irkutsk State U.) ; Yashin, I. (Moscow Phys. Eng. Inst.)

Published in: EPJ Web Conf.
Year: 2017
Vol.: 145
Page No: 01001
Pages: 8
Year: 2017 published

Abstract: We present the current status of high-energy cosmic-ray physics and gamma-ray astronomy at the Tunka Astrophysical Center (AC). This complex is located in the Tunka Valley, about 50 km from Lake Baikal. Present efforts are focused on the construction of the first stage of the gamma-ray observatory TAIGA - the TAIGA prototype. TAIGA (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) is designed for the study of gamma rays and charged cosmic rays in the energy range 1013 eV–1018 eV. The array includes a network of wide angle timing Cherenkov stations (TAIGA-HiSCORE), each with a FOV = 0.6 sr, plus up to 16 IACTs (FOV - 10∘× 10∘). This part covers an area of 5 km2. Additional muon detectors (TAIGA-Muon), with a total coverage of 2000 m2, are distributed over an area of 1 km2.

Web-Page: http://inspirehep.net/record/1607657/files/epjconf-isvhecri2016_01001.pdf

Total numbers of views: 227
Numbers of unique views: 117
DOI: 10.1051/epjconf/201614501001
 Record created 2017-07-04, last modified 2017-07-04


External link:
Download fulltext
Fulltext
Rate this document:

Rate this document:
1
2
3
 
(Not yet reviewed)