EPJ Web Conf.
Volume 191, 2018XXth International Seminar on High Energy Physics (QUARKS-2018)
|Number of page(s)||8|
|Published online||31 October 2018|
TAIGA - a hybrid array for high energy gamma astronomy and cosmic ray physics
Skobeltsyn Institute of Nuclear Physics MSU, Moscow, Russia
2 Institute of Applied Physics ISU, Irkutsk, Russia
3 Dipartimento di Fisica Generale Universiteta di Torino and INFN, Torino, Italy
4 Max-Planck-Institute for Physics, Munich, Germany
5 Institut fuür Experimentalphysik, University of Hamburg, Germany
6 IZMIRAN, Moscow, Russia
7 DESY, Zeuthen, Germany
8 National Research Nuclear University MEPhI, Moscow, Russia
9 JINR, Dubna, Russia
10 Novosibirsk State University, NSU, Novosibirsk, Russia
11 Budker Institute of Nuclear Physics SB RAS, Novosibirsk, Russia
12 ISS, Bucharest, Romania
13 Dubna State University, Dubna, Russia
14 Institut für Kernphysik, Karlsruhe Institute of Technology (KIT), Karlsruhe, 76021 Germany
15 Institut für Prozessdatenverarbeitung und Elektronik, Karlsruhe Institute of Technology (KIT)
* e-mail: email@example.com
Published online: 31 October 2018
The physics motivations and advantages of the new TAIGA (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) detector are presented. TAIGA aims at gamma-ray astronomy at energies from a few TeV to several PeV, as well as cosmic ray physics from 100 TeV to several EeV. For the energy range 30 – 200 TeV the sensitivity of 10 km2 area TAIGA array for the detection of local sources is expected to be 5 × 10-14 erg cm-2 sec-1 for 300 h of observations. Reconstruction of the given EAS energy, incoming direction and its core position, based on the timing TAIGA-HiSCORE data, allows one to increase a distance between the IACTs up to 600-1000 m. The low investments together with the high sensitivity for energies ≥ 30-50 TeV make this pioneering technique very attractive for exploring the galactic PeVatrons and cosmic rays. At present the TAIGA first stage has been constructed in Tunka valley, 50 km West from the Lake Baikal. The first experimental results of the TAIGA first stage are presented.
© The Authors, published by EDP Sciences, 2018
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.