Technological Novelties of Ground-Based Very High Energy Gamma-Ray Astrophysics with the Imaging Atmospheric Cherenkov Telescopes

Fuente: arXiv
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Main Author: Mirzoyan, Razmik
Format: Preprint
Published: 2024
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author Mirzoyan, Razmik
author_facet Mirzoyan, Razmik
contents Over the last three decades, the ground-based technique of imaging atmospheric Cherenkov telescopes has established itself as a powerful scientific discipline. About 250 very high gamma-ray sources of both galactic and extragalactic origin have been discovered, largely thanks to this technique. The study of these sources provides clues to many fundamental questions in astrophysics, astroparticle physics, cosmic ray physics and cosmology. The current generation of telescopes in operation offers solid performance. Further improvements in this technique led to the next generation large-scale instrument known as the Cherenkov Telescope Array (CTA). In its final configuration, the sensitivity of CTA will be several times higher than that of the current best instruments VERITAS, H.E.S.S. and MAGIC. This article is devoted to presenting the technological developments that have shaped this technique and led to its current success.
format Preprint
id arxiv_https___arxiv_org_abs_2411_09815
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Technological Novelties of Ground-Based Very High Energy Gamma-Ray Astrophysics with the Imaging Atmospheric Cherenkov Telescopes
Mirzoyan, Razmik
Instrumentation and Methods for Astrophysics
Over the last three decades, the ground-based technique of imaging atmospheric Cherenkov telescopes has established itself as a powerful scientific discipline. About 250 very high gamma-ray sources of both galactic and extragalactic origin have been discovered, largely thanks to this technique. The study of these sources provides clues to many fundamental questions in astrophysics, astroparticle physics, cosmic ray physics and cosmology. The current generation of telescopes in operation offers solid performance. Further improvements in this technique led to the next generation large-scale instrument known as the Cherenkov Telescope Array (CTA). In its final configuration, the sensitivity of CTA will be several times higher than that of the current best instruments VERITAS, H.E.S.S. and MAGIC. This article is devoted to presenting the technological developments that have shaped this technique and led to its current success.
title Technological Novelties of Ground-Based Very High Energy Gamma-Ray Astrophysics with the Imaging Atmospheric Cherenkov Telescopes
topic Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2411.09815