Imaging Very High Energy Gamma-Ray Telescopes
arXiv:0812.4198 · doi:10.1007/s10686-009-9151-z
Abstract
The technique of gamma-ray astronomy at very high energies (VHE: > 100 GeV) with ground-based imaging atmospheric Cherenkov telescopes is described, the H.E.S.S. array in Namibia serving as example. Mainly a discussion of the physical principles of the atmospheric Cherenkov technique is given, emphasizing its rapid development during the last decade. The present status is illustrated by two examples: the spectral and morphological characterization in VHE gamma-rays of a shell-type supernova remnant together with its theoretical interpretation, and the results of a survey of the Galactic Plane that shows a large variety of non-thermal sources. The final part is devoted to an overview of the ongoing and future instrumental developments.
To be published in Experimental Astronomy. Also to be published in proceedings "400 Years of Astronomical Telescopes: A Review of History, Science and Technology", editors B.R. Brandl, R. Stuik, J.K. Katgert-Merkelijn, Springer 2009
References in corpus (12)
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- VERITAS: the Very Energetic Radiation Imaging Telescope Array System
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Cited by in corpus (12)
- A high performance likelihood reconstruction of gamma-rays for Imaging Atmospheric Cherenkov Telescopes
- First Experimental Characterization of Microwave Emission from Cosmic Ray Air Showers
- Sensitivity of the Cherenkov Telescope Array to the detection of a dark matter signal in comparison to direct detection and collider experiments
- Gamma rays from the Galactic Centre region: a review
- Stellar Intensity Interferometry: Prospects for sub-milliarcsecond optical imaging
- The Discovery of Cherenkov Radiation and its use in the detection of extensive air showers
- Galactic magnetic fields and the large-scale anisotropy at MILAGRO
- Volcanoes muon imaging using Cherenkov telescopes
- Constraints on very high energy gamma-ray emission from the Fermi Bubbles with future ground-based experiments
- Asymmetry of the angular distribution of Cherenkov photons of extensive air showers induced by the geomagnetic field
- Statistical Tools for Imaging Atmospheric Cherenkov Telescopes
- Analysis Methods for Gamma-ray Astronomy