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Cerenkov light images of EAS produced by primary gamma

TLDR
In this paper, it was shown that it is possible to distinguish very effectively between background hadronic showers and TeV gamma ray showers from a point source on the basis of the width, length and orientation of the Cerenkov light images of the shower, seen in the focal plane of a focusing mirror.
Abstract
It is shown that it should be possible to distinguish very effectively between background hadronic showers and TeV gamma ray showers from a point source on the basis of the width, length and orientation of the Cerenkov light images of the shower, seen in the focal plane of a focusing mirror, even with a relatively coarse pixel size such as employed in the Mt Hopkins detector Predictions of the response of this system to air showers are presented

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Design concepts for the Cherenkov Telescope Array CTA: An advanced facility for ground-based high-energy gamma-ray astronomy

Marcos Daniel Actis, +685 more
TL;DR: The ground-based gamma-ray astronomy has had a major breakthrough with the impressive results obtained using systems of imaging atmospheric Cherenkov telescopes as mentioned in this paper, which is an international initiative to build the next generation instrument, with a factor of 5-10 improvement in sensitivity in the 100 GeV-10 TeV range and the extension to energies well below 100GeV and above 100 TeV.
Journal ArticleDOI

The major upgrade of the MAGIC telescopes, Part I: The hardware improvements and the commissioning of the system

Jelena Aleksić, +169 more
TL;DR: The MAGIC telescopes as mentioned in this paper are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma, Spain, which are designed to measure Cherennikov light from air showers initiated by gamma rays in the energy regime from around 50GeV to more than 50TeV.
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A Monte Carlo template based analysis for air-Cherenkov arrays

TL;DR: In this paper, an image pixel-wise fit for Atmospheric Cherenkov Telescopes (ImPACT) is proposed to estimate camera pixel amplitudes to an expected image template.
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