The GCT camera for the Cherenkov Telescope Array

Authors
  • A.M. Brown
  • A. Abchiche
  • D. Allan
  • J.-P. Amans
Publication date 2016
Host editors
  • H.J. Hall
  • R. Gilmozzi
  • H.K. Marshall
Book title Ground-based and Airborne Telescopes VI
Book subtitle 26 June-1 July 2016, Edinburgh, United Kingdom
ISBN
  • 9781510601918
ISBN (electronic)
  • 9781510601925
Series Proceedings of SPIE
Event Ground-based and Airborne Telescopes VI <br/>
Article number 99065K
Volume | Issue number 3
Number of pages 8
Publisher Bellingham, WA: SPIE
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract
The Gamma-ray Cherenkov Telescope (GCT) is proposed for the Small-Sized Telescope component of the Cherenkov Telescope Array (CTA). GCT's dual-mirror Schwarzschild-Couder (SC) optical system allows the use of a compact camera with small form-factor photosensors. The GCT camera is ~ 0:4 m in diameter and has 2048 pixels; each pixel has a ~ 0:2° angular size, resulting in a wide field-of-view. The design of the GCT camera is high performance at low cost, with the camera housing 32 front-end electronics modules providing full waveform information for all of the camera's 2048 pixels. The first GCT camera prototype, CHEC-M, was commissioned during 2015, culminating in the first Cherenkov images recorded by a SC telescope and the first light of a CTA prototype. In this contribution we give a detailed description of the GCT camera and present preliminary results from CHEC-M's commissioning.
Document type Conference contribution
Language English
Published at https://doi.org/10.1117/12.2231685
Other links https://ui.adsabs.harvard.edu/abs/2016SPIE.9906E..5KB/abstract
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