The GCT camera for the Cherenkov Telescope Array
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| Publication date | 2016 |
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| Book title | Ground-based and Airborne Telescopes VI |
| Book subtitle | 26 June-1 July 2016, Edinburgh, United Kingdom |
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| ISBN (electronic) |
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| 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 |
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| 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.
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| 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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