Capabilities of the GAMMA-400 gamma-ray telescope for lateral aperture
Autor: | Yu. T. Yurkin, V. V. Mikhailov, S. I. Suchkov, P. Yu. Minaev, A. M. Galper, A. Leonov, Irina V. Chernysheva, A. G. Mayorov, M. D. Kheymits, A. V. Mikhailova, A. V. Bakaldin, Nikolay Topchiev |
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Rok vydání: | 2020 |
Předmět: |
Physics
History Scintillation Range (particle radiation) Calorimeter (particle physics) Physics::Instrumentation and Detectors business.industry Astrophysics::High Energy Astrophysical Phenomena Antenna aperture Detector Computer Science Applications Education law.invention Telescope Optics law Lateral aperture business Fermi Gamma-ray Space Telescope |
Zdroj: | Journal of Physics: Conference Series. 1690:012026 |
ISSN: | 1742-6596 1742-6588 |
Popis: | The future GAMMA-400 γ-ray telescope will provide fundamentally new data on discrete sources and spectra of γ-ray emissions and electrons + positrons due to its unique angular and energy resolutions in the wide energy range from 20 MeV up to several TeV. The γ-ray telescope consists of the anticoincidence system (AC), the converter-tracker (C), the time-of-flight system (S1 and S2), the position-sensitive and electromagnetic calorimeters (CC1 and CC2), the scintillation detectors of the calorimeter (S3 and S4) and lateral anticoincidence detectors of the calorimeter (LD). To extend the GAMMA-400 capabilities to measure γ-ray bursts, Monte-Carlo simulations were performed for lateral aperture of the one of the versions of GAMMA-400. Second-level trigger based on signals from CC2, LD, S3, and S4 allows us to detect γ-ray bursts in the energy range of ~10-300 MeV with high effective area about 1 m2. |
Databáze: | OpenAIRE |
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