Research output: Contribution to journal › Conference article › peer-review
Camera of the first TAIGA-IACT : Construction and calibration. / the TAIGA Collaboration.
In: Proceedings of Science, Vol. Part F135186, 01.01.2017.Research output: Contribution to journal › Conference article › peer-review
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TY - JOUR
T1 - Camera of the first TAIGA-IACT
T2 - Construction and calibration
AU - the TAIGA Collaboration
AU - Lubsandorzhiev, N.
AU - Astapov, I.
AU - Bezyazeekov, P.
AU - Boreyko, V.
AU - Borodin, A.
AU - Brueckner, M.
AU - Budnev, N.
AU - Chiavassa, A.
AU - Dyachok, A.
AU - Fedorov, O.
AU - Gafarov, A.
AU - Garmash, A.
AU - Gorbunov, N.
AU - Grebenyuk, V.
AU - Gress, O.
AU - Gress, T.
AU - Grishin, O.
AU - Grinyuk, A.
AU - Horns, D.
AU - Igoshin, A.
AU - Ivanova, A.
AU - Kalmykov, N.
AU - Kazarina, Y.
AU - Kindin, V.
AU - Kirilenko, P.
AU - Kiryuhin, S.
AU - Kokoulin, R.
AU - Kompaniets, K.
AU - Korosteleva, E.
AU - Kozhin, V.
AU - Kravchenko, E.
AU - Kunnas, M.
AU - Kuzmichev, L.
AU - Lemeshev, Yu
AU - Lenok, V.
AU - Lubsandorzhiev, B.
AU - Mirgazov, R.
AU - Mirzoyan, R.
AU - Monkhoev, R.
AU - Nachtigall, R.
AU - Osipova, E.
AU - Pakhorukov, A.
AU - Panasyuk, M.
AU - Pankov, L.
AU - Petrukhin, A.
AU - Poleschuk, V.
AU - Popescu, E.
AU - Popova, E.
AU - Porelli, A.
AU - Sokolov, A.
N1 - Publisher Copyright: © Copyright owned by the author(s) under the terms of the Creative Commons. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-Non Commercial-No Derivatives 4.0 International License (CC BY-NC-ND 4.0).
PY - 2017/1/1
Y1 - 2017/1/1
N2 - The first imaging atmospheric Cherenkov telescope as a part of the TAIGA (Tunka Advanced Instrument for cosmic rays and Gamma Astronomy) detector was put into commission in the Tunka valley in December 2016. The reflector of the telescope follows the Davis-Cotton design. It is composed of 34 glassmirror tiles, each of 60 cm diameter, and has a diameter of 4.3 m. The focal length is 4.75 m. The imaging camera includes 560 photomultiplier-based pixels, providing a FoV of ∼10×10 degrees. The imaging camera is made by using a modular principle and includes trigger, data acquisition and processing systems based on MAROC3 chips. The slow control system monitors the count rate and the PMT anode currents as well as controls the high voltage. For monitoring performance of the camera a dedicated calibration system based on nanosecond pulsed LED light source was developed.
AB - The first imaging atmospheric Cherenkov telescope as a part of the TAIGA (Tunka Advanced Instrument for cosmic rays and Gamma Astronomy) detector was put into commission in the Tunka valley in December 2016. The reflector of the telescope follows the Davis-Cotton design. It is composed of 34 glassmirror tiles, each of 60 cm diameter, and has a diameter of 4.3 m. The focal length is 4.75 m. The imaging camera includes 560 photomultiplier-based pixels, providing a FoV of ∼10×10 degrees. The imaging camera is made by using a modular principle and includes trigger, data acquisition and processing systems based on MAROC3 chips. The slow control system monitors the count rate and the PMT anode currents as well as controls the high voltage. For monitoring performance of the camera a dedicated calibration system based on nanosecond pulsed LED light source was developed.
UR - http://www.scopus.com/inward/record.url?scp=85046058522&partnerID=8YFLogxK
M3 - Conference article
VL - Part F135186
JO - Proceedings of Science
JF - Proceedings of Science
SN - 1824-8039
ER -
ID: 12562509