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1. The wide-aperture gamma-ray telescope TAIGA-HiSCORE in the Tunka Valley: Design, composition and commissioning

Author

Gress, O., Astapov, I., Budnev, N., Bezyazeekov, P., Bogdanov, A., Boreyko, V., Brückner, M., Chiavassa, A., Chvalaev, O., Dyachok, A., Gress, T., Epimakhov, S., Fedoseev, E., Gafarov, A., Gorbunov, N., Grebenyuk, V., Grinuk, A., Grishin, O., Horns, D., Ivanova, A., Kalinin, A., Karpov, N., Kalmykov, N., Kazarina, Yu., Kirichkov, N., Kiryuhin, S., Kokoulin, R., Komponiest, K., Korosteleva, E., Kozhin, V., Kunnas, M., Kuzmichev, L., Lenok, V., Lubsandorzhiev, B., Lubsandorzhiev, N., Mirgazov, R., Mirzoyan, R., Monkhoev, R., Nachtigall, R., Pakhorukov, A., Panasyuk, M., Pankov, L., Petrukhin, A., Platonov, V., Poleschuk, V., Popova, E., Porelli, A., Prosin, V., Rubtsov, G., Pushnin, A., Samoliga, V., Saunkin, A., Semeney, Yu., Shaibonov(ju), B., Silaev, A., Silaev(ju), A., Skurikhin, A., Slucka, V., Spiering, C., Sveshnikova, L., Tabolenko, V., Tarashchansky, B., Tkachenko, A., Tkachev, L., Tluczykont, M., Voronin, D., Wischnewski, R., Zagorodnikov, A., Zurbanov, V., and Yashin, I.

Published
2017
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3. The TAIGA timing array HiSCORE - first results

Author

Tluczykont M., Budnev N., Astapov I., Barbashina N., Bogdanov A., Boreyko V., Brückner M., Chiavassa A., Chvalaev O., Gress O., Gress T., Grishin O., Dyachok A., Epimakhov S., Fedorov O., Gafarov A., Gorbunov N., Grebenyuk V., Grinuk A., Horns D., Kalinin A., Karpov N., Kalmykov N., Kazarina Y., Kiryuhin S., Kokoulin R., Kompaniets K., Konstantinov A., Korosteleva E., Kozhin V., Kravchenko E., Kunnas M., Kuzmichev L., Lemeshev Yu., Lubsandorzhiev B., Lubsandorzhiev N., Mirgazov R., Mirzoyan R., Monkhoev R., Nachtigall R., Osipova E., Pakhorukov A., Panasyuk M., Pankov L., Petrukhin A., Poleschuk V., Popova E., Porelli A., Postnikov E., Prosin V., Ptuskin V., Rubtsov G., Pushnin A., Samoliga V., Satunin P., Semeney Yu., Silaev A., Skurikhin A., Slunecka M., Sokolov A., Spiering C., Sveshnikova L., Tabolenko V., Tarashansky B., Tkachenko A., Tkachev L., Voronin D., Wischnewski R., Zagorodnikov A., Zurbanov V., Zhurov D., and Yashin I.

Subjects
Physics, QC1-999
Abstract

Observations of gamma rays up to several 100 TeV are particularly important to spectrally resolve the cutoff regime of the long-sought Pevatrons, the cosmic-ray PeV accelerators. One component of the TAIGA hybrid detector is the TAIGA-HiSCORE timing array, which currently consists of 28 wide angle (0.6 sr) air Cherenkov timing stations distributed on an area of 0.25 km2. The HiSCORE concept is based on (non-imaging) air shower front sampling with Cherenkov light. First results are presented.

Published
2017
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6. Calculation and Determination of Energy Parameters of the Mini-CHP on the Basis of the Heat Pump

Author

A. A. Shimanov, R.A. Panshin, U.I. Grinuk, D.A. Uglanov, and O.V. Tereshchenko

Subjects
Materials science, Basis (linear algebra), law, Nuclear engineering, Energy (signal processing), Heat pump, law.invention
Abstract

In this paper, the calculation and determination of the parameters of a mini-CHP on the basis of a heat pump is carried out, using four different plant diagrams as the power supply for the heat pump. Thermodynamic calculation of the heat pump. Calculation of the efficiency of the heat pump. Analysis of structural schemes for generating electricity using micro-thermal power plants and based on heat pumps A comparative analysis of the effectiveness of various schemes with mini-CHP. An assessment of the capital costs of installation, operation and determination of the payback period of the mini-CHP on the basis of a heat pump with various plant diagrams is carried out and the most economically advantageous scheme is selected. The practical application of the studied structural schemes is evaluated.

Published
2019
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7. The TAIGA timing array HiSCORE - first results

Author

M. Tluczykont, N. Budnev, I. Astapov, N. Barbashina, A. Bogdanov, V. Boreyko, M. Brückner, A. Chiavassa, O. Chvalaev, O. Gress, T. Gress, O. Grishin, A. Dyachok, S. Epimakhov, O. Fedorov, A. Gafarov, N. Gorbunov, V. Grebenyuk, A. Grinuk, D. Horns, A. Kalinin, N. Karpov, N. Kalmykov, Y. Kazarina, S. Kiryuhin, R. Kokoulin, K. Kompaniets, A. Konstantinov, E. Korosteleva, V. Kozhin, E. Kravchenko, M. Kunnas, L. Kuzmichev, Yu. Lemeshev, B. Lubsandorzhiev, N. Lubsandorzhiev, R. Mirgazov, R. Mirzoyan, R. Monkhoev, R. Nachtigall, E. Osipova, A. Pakhorukov, M. Panasyuk, L. Pankov, A. Petrukhin, V. Poleschuk, E. Popova, A. Porelli, E. Postnikov, V. Prosin, V. Ptuskin, G. Rubtsov, A. Pushnin, V. Samoliga, P. Satunin, Yu. Semeney, A. Silaev, A. Skurikhin, M. Slunecka, A. Sokolov, C. Spiering, L. Sveshnikova, V. Tabolenko, B. Tarashansky, A. Tkachenko, L. Tkachev, D. Voronin, R. Wischnewski, A. Zagorodnikov, V. Zurbanov, D. Zhurov, and I. Yashin

Subjects
Physics, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, QC1-999, Detector, Taiga, Gamma ray, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Astrophysics, 01 natural sciences, Air shower, Sampling (signal processing), 0103 physical sciences, 010303 astronomy & astrophysics, Cherenkov radiation, Remote sensing
Abstract

Observations of gamma rays up to several 100 TeV are particularly important to spectrally resolve the cutoff regime of the long-sought Pevatrons, the cosmic-ray PeV accelerators. One component of the TAIGA hybrid detector is the TAIGA-HiSCORE timing array, which currently consists of 28 wide angle (0.6 sr) air Cherenkov timing stations distributed on an area of 0.25 km2 . The HiSCORE concept is based on (non-imaging) air shower front sampling with Cherenkov light. First results are presented.

Published
2017

8. The wide-aperture gamma-ray telescope TAIGA-HiSCORE in the Tunka Valley: Design, composition and commissioning

Author

O. Gress, I. Astapov, N. Budnev, P. Bezyazeekov, A. Bogdanov, V. Boreyko, M. Brückner, A. Chiavassa, O. Chvalaev, A. Dyachok, T. Gress, S. Epimakhov, E. Fedoseev, A. Gafarov, N. Gorbunov, V. Grebenyuk, A. Grinuk, O. Grishin, D. Horns, A. Ivanova, A. Kalinin, N. Karpov, N. Kalmykov, Yu. Kazarina, N. Kirichkov, S. Kiryuhin, R. Kokoulin, K. Komponiest, E. Korosteleva, V. Kozhin, M. Kunnas, L. Kuzmichev, V. Lenok, B. Lubsandorzhiev, N. Lubsandorzhiev, R. Mirgazov, R. Mirzoyan, R. Monkhoev, R. Nachtigall, A. Pakhorukov, M. Panasyuk, L. Pankov, A. Petrukhin, V. Platonov, V. Poleschuk, E. Popova, A. Porelli, V. Prosin, G. Rubtsov, A. Pushnin, V. Samoliga, A. Saunkin, Yu. Semeney, B. Shaibonov(ju), A. Silaev, A. Silaev(ju), A. Skurikhin, V. Slucka, C. Spiering, L. Sveshnikova, V. Tabolenko, B. Tarashchansky, A. Tkachenko, L. Tkachev, M. Tluczykont, D. Voronin, R. Wischnewski, A. Zagorodnikov, V. Zurbanov, I. Yashin, Shaibonov, B., and Silaev, A.

Subjects
Data acquisition system, Nuclear and High Energy Physics, Cherenkov light, Cherenkov detector, Cosmic ray, 01 natural sciences, Particle detector, law.invention, Optics, law, 0103 physical sciences, ddc:530, 010306 general physics, Instrumentation, Cherenkov radiation, Physics, Gamma-ray sources, 010308 nuclear & particles physics, business.industry, Detector, Gamma ray, Cherenkov Telescope Array, business, Fermi Gamma-ray Space Telescope
Abstract

Nuclear instruments & methods in physics research / A 845, 367 - 372 (2017). doi:10.1016/j.nima.2016.08.031, The new TAIGA-HiSCORE non-imaging Cherenkov array aims to detect air showers induced by gamma rays above 30 TeV and to study cosmic rays above 100 TeV. TAIGA-HiSCORE is made of integrating air Cherenkov detector stations with a wide field of view (0.6 sr), placed at a distance of about 100 m. They cover an area of initially ∼0.25 km$^2$ (prototype array), and of ∼5 km$^2$ at the final phase of the experiment. Each station includes 4 PMTs with 20 or 25 cm diameter, equipped with light guides shaped as Winstone cones. We describe the design, specifications of the read-out, DAQ and control and monitoring systems of the array. The present 28 detector stations of the TAIGA-HiSCORE engineering setup are in operation since September 2015., Published by North-Holland Publ. Co., Amsterdam

Published
2017
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9. Connecting neutrino Astrophysics to Multi-TeV to PeV gamma-ray astronomy with TAIGA

Author

Tluczykont, Martin, Budnev, N., Astapov, I., Bezyazeekov, P., Bogdanov, A., Boreyko, V., Brueckner, Martin, Chiavassa, A., Chvalaev, O., Gress, O., Gress, T., Grishin, O., Dyachok, A., Epimakhov, Sergey, Fedorov, O., Gafarov, A., Gorbunov, N., Grebenyuk, V., Grinuk, A., Horns, Dieter, Ivanova, Anna, Kalinin, Anton, Karpov, N., Kalmykov, N., Kazarina, Y., Kirichkov, N., Kiryuhin, S., Kokoulin, R., Komponiest, K., Konstantinov, A., Korosteleva, E., Kozhin, V., Kunnas, Maike Helena, Kuzmichev, L., Lenok, V., Lubsandorzhiev, B., Lubsandorzhiev, N., Mirgazov, R., Mirzoyan, R., Monkhoev, R., Nachtigall, Rayk, Osipova, E., Pakhorukov, A., Panasyuk, M., Pankov, L., Petrukhin, A., Platonov, V., Poleschuk, V., Popova, Elena, Porelli, Andrea, Postnikov, E., Prosin, V., Ptuskin, V., Rubtsov, G., Pushnin, A., Samoliga, V., Satunin, Peter, Semeney, Yu., Silaev, A., Skurikhin, A., Slucka, V., Spiering, Christian, Sveshnikova, L., Tabolenko, V., Tarashansky, B., Tkachenko, A., Tkachev, L., Voronin, D., Wischnewski, Ralf, Zagorodnikov, A., Zurbanov, V., and Yashin, I.

Subjects
Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Physics::Accelerator Physics
Abstract

Tluczykont, M. "Connecting neutrino Astrophysics to Multi-TeV to PeV gamma-ray astronomy with TAIGA" in Proceedings, Magellan Workshop: Connecting Neutrino Physics and Astronomy / Dahmke, Stefan K.G., Meyer, Mikko, Vanhoefer, Laura (eds.), Deutsches Elektronen-Synchrotron, DESY : 2016 ; Magellan Workshop, 2016-03-17 - 2016-03-18, Hamburg Magellan Workshop, Hamburg, Germany, 17 Mar 2016 - 18 Mar 2016 ; DESY-PROC 135-142(2016). doi:10.3204/DESY-PROC-2016-05/27, Recent evidence for neutrinos in the PeV energy range from IceCube provides additional motivation for the search for the most energetic Galactic accelerators. Gamma-ray astronomy is a sound strategy to reach this goal, providing the energy range beyond 10\,TeV can be covered at a sufficient sensitivity level. The energy spectra of most known gamma-ray emitters only reach up to few 10s of TeV. The HEGRA IACT installation reported evidence for gamma-ray energies from the Crab Nebula as high as 80\,TeV. Uncovering their spectral shape up to few 100s of TeV could answer the question whether some of these objects are cosmic ray Pevatrons, i.e. Galactic PeV accelerators. Extending observations beyond this energy range requires very large effective detector areas, as planned by the TAIGA collaboration., Published by Verlag Deutsches Elektronen-Synchrotron, Hamburg

Published
2016
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10. Simulation of imaging air shower Cherenkov telescopes as part of the TAIGA Project

Author

Kunnas, Maike Helena, Astapov, I., Gress, T., Grishin, O., Dyachok, A., Epimakhov, Sergey, Fedorov, O., Gafarov, A., Gorbunov, N., Grebenyuk, V., Grinuk, A., Horns, Dieter, Bezyazeekov, P., Ivanova, A., Kalinin, A., Karpov, N., Kalmykov, N., Kazarina, Y., Kirichkov, N., Kiryuhin, S., Kokoulin, R., Komponiest, K., Konstantinov, A., Bogdanov, A., Korosteleva, E., Kozhin, V., Kuzmichev, L., Lenok, V., Lubsandorzhiev, B., Lubsandorzhiev, N., Mirgazov, R., Mirzoyan, R., Monkhoev, R., Nachtigall, Rayk, Boreyko, V., Osipova, E., Pakhorukov, A., Panasyuk, M., Pankov, L., Petrukhin, A., Platonov, V., Poleschuk, V., Popova, E., Porelli, Andrea, Postnikov, E., Brückner, M., Prosin, V., Ptuskin, V., Rubtsov, G., Pushnin, A., Samoliga, V., Satunin, P., Semeney, Yu., Silaev, A., Skurikhin, A., Budnev, N., Slucka, V., Spiering, Christian, Sveshnikova, L., Tabolenko, V., Tarashansky, B., Tkachenko, A., Tkachev, L., Tluczykont, Martin, Voronin, D., Wischnewski, Ralf, Chiavassa, A., Zagorodnikov, A., Zurbanov, V., Yashin, I., Chvalaev, O., and Gress, O.

Subjects
Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics
Abstract

Magellan Workshop, Hamburg, Germany, 17 Mar 2016 - 18 Mar 2016 ; DESY-PROC 143-150(2016). doi:10.3204/DESY-PROC-2016-05/33, The Tunka Advanced International Gamma-ray and Cosmic ray Astrophysics (TAIGA) project aims at observation of cosmic rays beyond 100 TeV and gamma rays above 1 TeV via observation of the extensive air showers (EAS) caused in the atmosphere. Two common detection techniques are timing arrays and imaging air shower cherenkov telescopes (IACT). Timing arrays yield good directional and energy reconstruction, but provide only mediocre gamma-hadron-separation at their energy threshold. IACTs are good at separation, but since a stereoscopic view of a shower is needed for high reconstruction accuracy, it is difficult to achieve the large effective areas needed for ultra high energy observations. In this work we present the simulations performed to explore and optimize our IACT design and the first steps towards hybrid reconstruction., Published by Verlag Deutsches Elektronen-Synchrotron, Hamburg

Published
2016
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11. The Tunka detector complex: from cosmic-ray to gamma-ray astronomy

Author

N Budnev, I Astapov, N Barbashina, A Bogdanov, D Bogorodskii, V Boreyko, M Büker, M Brückner, A Chiavassa, O Chvalaev, O Gress, T Gress, A Dyachok, S Epimakhov, A Gafatov, N Gorbunov, V Grebenyuk, A Grinuk, A Haungs, R Hiller, D Horns, T Huege, A Ivanova, A Kalinin, N Karpov, N Kalmykov, Y Kazarina, V Kindin, N Kirichkov, S Kiryuhin, M Kleifges, R Kokoulin, K Komponiest, A Konstantinov, E Konstantinov, A Korobchenko, E Korosteleva, D Kostunin, V Kozhin, O Krömer, M Kunnas, L Kuzmichev, V Lenok, B Lubsandorzhiev, N Lubsandorzhiev, R Mirgazov, R Mirzoyan, R Monkhoev, R Nachtigall, A Pakhorukov, M Panasyuk, L Pankov, A Petrukhin, V Platonov, V Poleschuk, E Popova, A Porelli, V Prosin, V Ptuskin, G Rubtsov, C Rühle, V Samoliga, P Satunin, V Savinov, A Saunkin, F Schröder, Yu Semeney, B Shaibonov, A Silaev, A Skurikhin, V Slucka, C Spiering, L Sveshnikova, V Tabolenko, A Tkachenko, L Tkachev, M Tluczykont, D Voronin, R Wischnewski, A Zagorodnikov, V Zurbanov, and I Yashin

Subjects
Physics, History, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Cosmic ray, Knee region, Astrophysics, Gamma-ray astronomy, Cherenkov Telescope Array, Computer Science Applications, Education, ddc:530, Cherenkov radiation
Abstract

TAIGA stands for "Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy" and is a project to build a complex, hybrid detector system for ground-based gamma- ray astronomy from a few TeV to several PeV, and for cosmic-ray studies from 100 TeV to 1 EeV. TAIGA will search for "PeVatrons" (ultra-high energy gamma-ray sources) and measure the composition and spectrum of cosmic rays in the knee region (100 TeV - 10 PeV) with good energy resolution and high statistics. TAIGA will include Tunka-HiSCORE (an array of wide-angle air Cherenkov stations), an array of Imaging Atmospheric Cherenkov Telescopes, an array of particle detectors, both on the surface and underground, and the TUNKA-133 air Cherenkov array.

Published
2015
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12. The TAIGA experiment: from cosmic ray to gamma-ray astronomy in the Tunka valley

Author

Budnev, N, Astapov, I, Bezyazeekov, P, Bogdanov, A, Boreyko, V, Büker, M, Brückner, M, Chiavassa, A, Chvalaev, O, Gress, O, Gress, T, Grishin, O, Dyachok, A, Epimakhov, S, Fedorov, O, Gafarov, A, Gorbunov, N, Grebenyuk, V, Grinuk, A, Haungs, A, Hiller, R, Horns, D, Huege, T, Ivanova, A, Kalinin, A, Karpov, N, Kalmykov, N, Kazarina, Y, Kirichkov, N, Kiryuhin, S, Kleifges, M, Kokoulin, R, Komponiest, K, Konstantinov, A, Korosteleva, E, Kostunin, D, Kozhin, V, Krömer, O, Kunnas, M, Kuzmichev, L, Lenok, V, Lubsandorzhiev, B, Lubsandorzhiev, N, Mirgazov, R, Mirzoyan, R, Monkhoev, R, Nachtigall, R, Pakhorukov, A, Panasyuk, M, Pankov, L, Perevalov, A, Petrukhin, A, Platonov, V, Poleschuk, V, Popova, E, Porelli, A, Prosin, V, Ptuskin, V, Rubtsov, G, Pushnin, A, Samoliga, V, Satunin, P, Schröder, F, Semeney, Yu, Silaev, A, Skurikhin, A, Slucka, V, Spiering, C, Sveshnikova, L, Tabolenko, V, Tarashansky, B, Tkachenko, A, Tkachev, L, Tluczykont, M, Voronin, D, Wischnewski, R, Zagorodnikov, A, Zurbanov, V, Yashin, I, Budnev, N, Astapov, I, Bezyazeekov, P, Bogdanov, A, Boreyko, V, Büker, M, Brückner, M, Chiavassa, A, Chvalaev, O, Gress, O, Gress, T, Grishin, O, Dyachok, A, Epimakhov, S, Fedorov, O, Gafarov, A, Gorbunov, N, Grebenyuk, V, Grinuk, A, Haungs, A, Hiller, R, Horns, D, Huege, T, Ivanova, A, Kalinin, A, Karpov, N, Kalmykov, N, Kazarina, Y, Kirichkov, N, Kiryuhin, S, Kleifges, M, Kokoulin, R, Komponiest, K, Konstantinov, A, Korosteleva, E, Kostunin, D, Kozhin, V, Krömer, O, Kunnas, M, Kuzmichev, L, Lenok, V, Lubsandorzhiev, B, Lubsandorzhiev, N, Mirgazov, R, Mirzoyan, R, Monkhoev, R, Nachtigall, R, Pakhorukov, A, Panasyuk, M, Pankov, L, Perevalov, A, Petrukhin, A, Platonov, V, Poleschuk, V, Popova, E, Porelli, A, Prosin, V, Ptuskin, V, Rubtsov, G, Pushnin, A, Samoliga, V, Satunin, P, Schröder, F, Semeney, Yu, Silaev, A, Skurikhin, A, Slucka, V, Spiering, C, Sveshnikova, L, Tabolenko, V, Tarashansky, B, Tkachenko, A, Tkachev, L, Tluczykont, M, Voronin, D, Wischnewski, R, Zagorodnikov, A, Zurbanov, V, and Yashin, I

Abstract

The physical motivations and advantages of the new gamma-observatory TAIGA (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) is presented. The TAIGA array is a complex, hybrid detector for ground-based gamma-ray astronomy for energies from a few TeV to several PeV as well as for cosmic ray studies from 100 TeV to several EeV. The TAIGA will include the wide angle Cherenkov array TAIGA-HiSCORE with ~5 km2 area, a net of 16 I ACT telescopes (with FOV of about 10x10 degree), muon detectors with a total area of up to 2000-3000 m2 and the radio array Tunka-Rex., Peer Reviewed

Published
2016

13. The TAIGA experiment: from cosmic ray to gamma-ray astronomy in the Tunka valley

Author

Budnev, N, primary, Astapov, I, additional, Bezyazeekov, P, additional, Bogdanov, A, additional, Boreyko, V, additional, Büker, M, additional, Brückner, M, additional, Chiavassa, A, additional, Chvalaev, O, additional, Gress, O, additional, Gress, T, additional, Grishin, O, additional, Dyachok, A, additional, Epimakhov, S, additional, Fedorov, O, additional, Gafarov, A, additional, Gorbunov, N, additional, Grebenyuk, V, additional, Grinuk, A, additional, Haungs, A, additional, Hiller, R, additional, Horns, D, additional, Huege, T, additional, Ivanova, A, additional, Kalinin, A, additional, Karpov, N, additional, Kalmykov, N, additional, Kazarina, Y, additional, Kirichkov, N, additional, Kiryuhin, S, additional, Kleifges, M, additional, Kokoulin, R, additional, Komponiest, K, additional, Konstantinov, A, additional, Korosteleva, E, additional, Kostunin, D, additional, Kozhin, V, additional, Krömer, O, additional, Kunnas, M, additional, Kuzmichev, L, additional, Lenok, V, additional, Lubsandorzhiev, B, additional, Lubsandorzhiev, N, additional, Mirgazov, R, additional, Mirzoyan, R, additional, Monkhoev, R, additional, Nachtigall, R, additional, Pakhorukov, A, additional, Panasyuk, M, additional, Pankov, L, additional, Perevalov, A, additional, Petrukhin, A, additional, Platonov, V, additional, Poleschuk, V, additional, Popova, E, additional, Porelli, A, additional, Prosin, V, additional, Ptuskin, V, additional, Rubtsov, G, additional, Pushnin, A, additional, Samoliga, V, additional, Satunin, P, additional, Schröder, F, additional, Semeney, Yu, additional, Silaev, A, additional, Skurikhin, A, additional, Slucka, V, additional, Spiering, C, additional, Sveshnikova, L, additional, Tabolenko, V, additional, Tarashansky, B, additional, Tkachenko, A, additional, Tkachev, L, additional, Tluczykont, M, additional, Voronin, D, additional, Wischnewski, R, additional, Zagorodnikov, A, additional, Zurbanov, V, additional, and Yashin, I, additional

Published
2016
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14. The TAIGA experiment: from cosmic ray to gamma-ray astronomy in the Tunka valley

Author

N Budnev, I Astapov, P Bezyazeekov, A Bogdanov, V Boreyko, M Büker, M Brückner, A Chiavassa, O Chvalaev, O Gress, T Gress, O Grishin, A Dyachok, S Epimakhov, O Fedorov, A Gafarov, N Gorbunov, V Grebenyuk, A Grinuk, A Haungs, R Hiller, D Horns, T Huege, A Ivanova, A Kalinin, N Karpov, N Kalmykov, Y Kazarina, N Kirichkov, S Kiryuhin, M Kleifges, R Kokoulin, K Komponiest, A Konstantinov, E Korosteleva, D Kostunin, V Kozhin, O Krömer, M Kunnas, L Kuzmichev, V Lenok, B Lubsandorzhiev, N Lubsandorzhiev, R Mirgazov, R Mirzoyan, R Monkhoev, R Nachtigall, A Pakhorukov, M Panasyuk, L Pankov, A Perevalov, A Petrukhin, V Platonov, V Poleschuk, E Popova, A Porelli, V Prosin, V Ptuskin, G Rubtsov, A Pushnin, V Samoliga, P Satunin, F Schröder, Yu Semeney, A Silaev, A Skurikhin, V Slucka, C Spiering, L Sveshnikova, V Tabolenko, B Tarashansky, A Tkachenko, L Tkachev, M Tluczykont, D Voronin, R Wischnewski, A Zagorodnikov, V Zurbanov, and I Yashin

Subjects
Physics, History, Muon, Physics::Instrumentation and Detectors, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Taiga, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Cosmic ray, Astrophysics, Gamma-ray astronomy, 01 natural sciences, Computer Science Applications, Education, 0103 physical sciences, High Energy Physics::Experiment, ddc:620, 010306 general physics, Engineering & allied operations, Cherenkov radiation, Muon detector, Lepton
Abstract

The physical motivations and advantages of the new gamma-observatory TAIGA (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) is presented. The TAIGA array is a complex, hybrid detector for ground-based gamma-ray astronomy for energies from a few TeV to several PeV as well as for cosmic ray studies from 100 TeV to several EeV. The TAIGA will include the wide angle Cherenkov array TAIGA-HiSCORE with ~5 km$^{2}$ area, a net of 16 IACT telescopes (with FOV of about 10x10 degree), muon detectors with a total area of up to 2000-3000 m$^{2}$ and the radio array Tunka-Rex.

Published
2016
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15. The Tunka detector complex: from cosmic-ray to gamma-ray astronomy

Author

Budnev, N, Astapov, I, Barbashina, N, Bogdanov, A, Bogorodskii, D, Boreyko, V, Büker, M, Brückner, M, Chiavassa, A, Chvalaev, O, Gress, O, Gress, T, Dyachok, A, Epimakhov, S, Gafatov, A, Gorbunov, N, Grebenyuk, V, Grinuk, A, Haungs, A, Hiller, R, Horns, D, Huege, T, Ivanova, A, Kalinin, A, Karpov, N, Kalmykov, N, Kazarina, Y, Kindin, V, Kirichkov, N, Kiryuhin, S, Kleifges, M, Kokoulin, R, Komponiest, K, Konstantinov, A, Konstantinov, E, Korobchenko, A, Korosteleva, E, Kostunin, D, Kozhin, V, Krömer, O, Kunnas, M, Kuzmichev, L, Lenok, V, Lubsandorzhiev, B, Lubsandorzhiev, N, Mirgazov, R, Mirzoyan, R, Monkhoev, R, Nachtigall, R, Pakhorukov, A, Panasyuk, M, Pankov, L, Petrukhin, A, Platonov, V, Poleschuk, V, Popova, E, Porelli, A, Prosin, V, Ptuskin, V, Rubtsov, G, Rühle, C, Samoliga, V, Satunin, P, Savinov, V, Saunkin, A, Schröder, F, Semeney, Yu, Shaibonov, B, Silaev, A, Skurikhin, A, Slucka, V, Spiering, C, Sveshnikova, L, Tabolenko, V, Tkachenko, A, Tkachev, L, Tluczykont, M, Voronin, D, Wischnewski, R, Zagorodnikov, A, Zurbanov, V, Yashin, I, Budnev, N, Astapov, I, Barbashina, N, Bogdanov, A, Bogorodskii, D, Boreyko, V, Büker, M, Brückner, M, Chiavassa, A, Chvalaev, O, Gress, O, Gress, T, Dyachok, A, Epimakhov, S, Gafatov, A, Gorbunov, N, Grebenyuk, V, Grinuk, A, Haungs, A, Hiller, R, Horns, D, Huege, T, Ivanova, A, Kalinin, A, Karpov, N, Kalmykov, N, Kazarina, Y, Kindin, V, Kirichkov, N, Kiryuhin, S, Kleifges, M, Kokoulin, R, Komponiest, K, Konstantinov, A, Konstantinov, E, Korobchenko, A, Korosteleva, E, Kostunin, D, Kozhin, V, Krömer, O, Kunnas, M, Kuzmichev, L, Lenok, V, Lubsandorzhiev, B, Lubsandorzhiev, N, Mirgazov, R, Mirzoyan, R, Monkhoev, R, Nachtigall, R, Pakhorukov, A, Panasyuk, M, Pankov, L, Petrukhin, A, Platonov, V, Poleschuk, V, Popova, E, Porelli, A, Prosin, V, Ptuskin, V, Rubtsov, G, Rühle, C, Samoliga, V, Satunin, P, Savinov, V, Saunkin, A, Schröder, F, Semeney, Yu, Shaibonov, B, Silaev, A, Skurikhin, A, Slucka, V, Spiering, C, Sveshnikova, L, Tabolenko, V, Tkachenko, A, Tkachev, L, Tluczykont, M, Voronin, D, Wischnewski, R, Zagorodnikov, A, Zurbanov, V, and Yashin, I

Abstract

TAIGA stands for "Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy" and is a project to build a complex, hybrid detector system for ground-based gamma- ray astronomy from a few TeV to several PeV, and for cosmic-ray studies from 100 TeV to 1 EeV. TAIGA will search for "PeVatrons" (ultra-high energy gamma-ray sources) and measure the composition and spectrum of cosmic rays in the knee region (100 TeV - 10 PeV) with good energy resolution and high statistics. TAIGA will include Tunka-HiSCORE (an array of wide-angle air Cherenkov stations), an array of Imaging Atmospheric Cherenkov Telescopes, an array of particle detectors, both on the surface and underground, and the TUNKA-133 air Cherenkov array., Peer Reviewed

Published
2015

16. The Tunka detector complex: from cosmic-ray to gamma-ray astronomy

Author

Budnev, N, primary, Astapov, I, additional, Barbashina, N, additional, Bogdanov, A, additional, Bogorodskii, D, additional, Boreyko, V, additional, Büker, M, additional, Brückner, M, additional, Chiavassa, A, additional, Chvalaev, O, additional, Gress, O, additional, Gress, T, additional, Dyachok, A, additional, Epimakhov, S, additional, Gafatov, A, additional, Gorbunov, N, additional, Grebenyuk, V, additional, Grinuk, A, additional, Haungs, A, additional, Hiller, R, additional, Horns, D, additional, Huege, T, additional, Ivanova, A, additional, Kalinin, A, additional, Karpov, N, additional, Kalmykov, N, additional, Kazarina, Y, additional, Kindin, V, additional, Kirichkov, N, additional, Kiryuhin, S, additional, Kleifges, M, additional, Kokoulin, R, additional, Komponiest, K, additional, Konstantinov, A, additional, Konstantinov, E, additional, Korobchenko, A, additional, Korosteleva, E, additional, Kostunin, D, additional, Kozhin, V, additional, Krömer, O, additional, Kunnas, M, additional, Kuzmichev, L, additional, Lenok, V, additional, Lubsandorzhiev, B, additional, Lubsandorzhiev, N, additional, Mirgazov, R, additional, Mirzoyan, R, additional, Monkhoev, R, additional, Nachtigall, R, additional, Pakhorukov, A, additional, Panasyuk, M, additional, Pankov, L, additional, Petrukhin, A, additional, Platonov, V, additional, Poleschuk, V, additional, Popova, E, additional, Porelli, A, additional, Prosin, V, additional, Ptuskin, V, additional, Rubtsov, G, additional, Rühle, C, additional, Samoliga, V, additional, Satunin, P, additional, Savinov, V, additional, Saunkin, A, additional, Schröder, F, additional, Semeney, Yu, additional, Shaibonov, B, additional, Silaev, A, additional, Skurikhin, A, additional, Slucka, V, additional, Spiering, C, additional, Sveshnikova, L, additional, Tabolenko, V, additional, Tkachenko, A, additional, Tkachev, L, additional, Tluczykont, M, additional, Voronin, D, additional, Wischnewski, R, additional, Zagorodnikov, A, additional, Zurbanov, V, additional, and Yashin, I, additional

Published
2015
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