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The precision of the IACT mechanical mounts of the TAIGA observatory. / the TAIGA Collaboration.

2022. Paper presented at 37th International Cosmic Ray Conference, Берлин, Berlin, Germany.

Research output: Contribution to conference › Paper › peer-review

Harvard

the TAIGA Collaboration 2022, 'The precision of the IACT mechanical mounts of the TAIGA observatory', Paper presented at 37th International Cosmic Ray Conference, Берлин, Germany, 12.07.2021 - 23.07.2021. https://doi.org/10.22323/1.395.0742

APA

the TAIGA Collaboration (2022). The precision of the IACT mechanical mounts of the TAIGA observatory. Paper presented at 37th International Cosmic Ray Conference, Берлин, Berlin, Germany. https://doi.org/10.22323/1.395.0742

Vancouver

the TAIGA Collaboration. The precision of the IACT mechanical mounts of the TAIGA observatory. 2022. Paper presented at 37th International Cosmic Ray Conference, Берлин, Berlin, Germany. doi: 10.22323/1.395.0742

Author

the TAIGA Collaboration. / The precision of the IACT mechanical mounts of the TAIGA observatory. Paper presented at 37th International Cosmic Ray Conference, Берлин, Berlin, Germany.8 p.

BibTeX

@conference{8c764d80732b479493229657721b60e1,
title = "The precision of the IACT mechanical mounts of the TAIGA observatory",
abstract = "The TAIGA (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) observatory is located in the Tunka valley (∼50 km west from the southern shore of Lake Baikal) at an altitude of 675 m a.s.l. The TAIGA observatory aims to address gamma-ray astronomy at energies from a few TeV to several PeV and CR physics from 100 TeV to several EeV. Its main feature is the complementary, hybrid approach to distinguish CR events from those of gamma rays. Currently TAIGA consists of ∼80 wide-angle air Cherenkov detectors (HiSCORE stations), three ∼4 m diameter IACTs and several hundred surface and underground muon detectors, grouped in three jointly operating arrays. The exceptional feature of the TAIGA IACT array is it's topology that allows one to aim for the optimal cost/performance by scanning the optimal inter-telescope distances from 300 m up to 600 m. The IACTs have alt-azimuth type mounts and 576-pixel imaging cameras in the foci, covering 9.6° aperture in the sky. The segmented reflectors of ∼10 m2 area follow the Davis-Cotton design. The largest diameter of the hexagonal shape reflector is 4.3 m and the focal length is 4.75 m. The rigid telescope mount provides a maximum displacement of EAS image below 2 mm (i.e. ≤ 0.024°) in the photodetector plane. The main parameters of IACTs are of a crucial importance for their efficient operation and is presented.",
author = "{the TAIGA Collaboration} and A. Borodin and A. Grinyuk and A. Pan and Y. Sagan and L. Tkachev and D. Zhurov and I. Astapov and P. Bezyazeekov and M. Brueckner and N. Budnev and A. Chiavassa and A. Dyachok and O. Fedorov and A. Gafarov and A. Garmash and V. Grebenyuk and O. Gress and T. Gress and O. Grishin and D. Horns and A. Ivanova and N. Kalmykov and Y. Kazarina and V. Kindin and P. Kirilenko and S. Kiryushin and R. Kokoulin and K. Kompaniets and E. Korosteleva and V. Kozhin and E. Kravchenko and M. Kunnas and L. Kuzmichev and Yu Lemeshev and V. Lenok and N. Lubsandorzhiev and B. Lubsandorzhiev and R. Mirgazov and R. Mirzoyan and R. Monkhoev and R. Nachtigall and E. Osipova and A. Pakhorukov and M. Panasyuk and L. Pankov and A. Petrukhin and V. Poleschuk and E. Popescu and E. Popova and A. Sokolov",
year = "2022",
month = mar,
day = "18",
doi = "10.22323/1.395.0742",
language = "English",
note = "37th International Cosmic Ray Conference : The astroparticle physics conference, ICRC2021 ; Conference date: 12-07-2021 Through 23-07-2021",
url = "https://icrc2021.desy.de/",

}

RIS

TY - CONF

T1 - The precision of the IACT mechanical mounts of the TAIGA observatory

AU - the TAIGA Collaboration

AU - Borodin, A.

AU - Grinyuk, A.

AU - Pan, A.

AU - Sagan, Y.

AU - Tkachev, L.

AU - Zhurov, D.

AU - Astapov, I.

AU - Bezyazeekov, P.

AU - Brueckner, M.

AU - Budnev, N.

AU - Chiavassa, A.

AU - Dyachok, A.

AU - Fedorov, O.

AU - Gafarov, A.

AU - Garmash, A.

AU - Grebenyuk, V.

AU - Gress, O.

AU - Gress, T.

AU - Grishin, O.

AU - Horns, D.

AU - Ivanova, A.

AU - Kalmykov, N.

AU - Kazarina, Y.

AU - Kindin, V.

AU - Kirilenko, P.

AU - Kiryushin, 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, N.

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 - Sokolov, A.

N1 - Conference code: 37

PY - 2022/3/18

Y1 - 2022/3/18

N2 - The TAIGA (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) observatory is located in the Tunka valley (∼50 km west from the southern shore of Lake Baikal) at an altitude of 675 m a.s.l. The TAIGA observatory aims to address gamma-ray astronomy at energies from a few TeV to several PeV and CR physics from 100 TeV to several EeV. Its main feature is the complementary, hybrid approach to distinguish CR events from those of gamma rays. Currently TAIGA consists of ∼80 wide-angle air Cherenkov detectors (HiSCORE stations), three ∼4 m diameter IACTs and several hundred surface and underground muon detectors, grouped in three jointly operating arrays. The exceptional feature of the TAIGA IACT array is it's topology that allows one to aim for the optimal cost/performance by scanning the optimal inter-telescope distances from 300 m up to 600 m. The IACTs have alt-azimuth type mounts and 576-pixel imaging cameras in the foci, covering 9.6° aperture in the sky. The segmented reflectors of ∼10 m2 area follow the Davis-Cotton design. The largest diameter of the hexagonal shape reflector is 4.3 m and the focal length is 4.75 m. The rigid telescope mount provides a maximum displacement of EAS image below 2 mm (i.e. ≤ 0.024°) in the photodetector plane. The main parameters of IACTs are of a crucial importance for their efficient operation and is presented.

AB - The TAIGA (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) observatory is located in the Tunka valley (∼50 km west from the southern shore of Lake Baikal) at an altitude of 675 m a.s.l. The TAIGA observatory aims to address gamma-ray astronomy at energies from a few TeV to several PeV and CR physics from 100 TeV to several EeV. Its main feature is the complementary, hybrid approach to distinguish CR events from those of gamma rays. Currently TAIGA consists of ∼80 wide-angle air Cherenkov detectors (HiSCORE stations), three ∼4 m diameter IACTs and several hundred surface and underground muon detectors, grouped in three jointly operating arrays. The exceptional feature of the TAIGA IACT array is it's topology that allows one to aim for the optimal cost/performance by scanning the optimal inter-telescope distances from 300 m up to 600 m. The IACTs have alt-azimuth type mounts and 576-pixel imaging cameras in the foci, covering 9.6° aperture in the sky. The segmented reflectors of ∼10 m2 area follow the Davis-Cotton design. The largest diameter of the hexagonal shape reflector is 4.3 m and the focal length is 4.75 m. The rigid telescope mount provides a maximum displacement of EAS image below 2 mm (i.e. ≤ 0.024°) in the photodetector plane. The main parameters of IACTs are of a crucial importance for their efficient operation and is presented.

UR - https://www.scopus.com/inward/record.url?eid=2-s2.0-85145020502&partnerID=40&md5=37c618f28f12c63069888a8dc8e24cfc

UR - https://www.mendeley.com/catalogue/59b0ec52-6c2f-3fec-a967-266dfd686cad/

U2 - 10.22323/1.395.0742

DO - 10.22323/1.395.0742

M3 - Paper

T2 - 37th International Cosmic Ray Conference

Y2 - 12 July 2021 through 23 July 2021

ER -

ID: 46023529