24-28 February 2020
Budker Institute of Nuclear Physics
Asia/Novosibirsk timezone

Development of a compact-size, novel wide Field of View VHE Gamma-Ray Imaging Air Cherenkov Telescope with a SiPM-based camera for energies above 10 TeV for operation in the TAIGA installation.

Not scheduled
15m
Budker Institute of Nuclear Physics

Budker Institute of Nuclear Physics

11, akademika Lavrentieva prospect, Novosibirsk, Russia
Board: 55
Poster Instrumentation for Astroparticle and Neutrino physics

Speaker

Dr Dmitry Chernov (Skobeltsyn Institute of Lomonosov Moscow State University)

Description

D. Chernov for the TAIGA collaboration. The TAIGA complex-detector is designed to study gamma and cosmic rays in the energy range above 30TeV. We are developing a novel wide-angle telescope with a SiPM-based imaging camera of a FoV of 15-20° and of an aperture of not more than 1 m2 . In this report we intend to present the design of such a camera (optical system and DAQ), based on 1000-1200 SiPMs. The prototype of such a camera, based on 49 SiPMs, is operating at the TAIGA’s site in Tunka valley since September 2019. The design of the prototype and the preliminary results of data analysis will be presented.

Primary author

Dr Dmitry Chernov (Skobeltsyn Institute of Lomonosov Moscow State University)

Presentation Materials