Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/44351
Title: Final characterisation and design of the Gamma-ray Cherenkov Telescope (GCT) for the Cherenkov Telescope Array
Authors: Le Blanc, O
Fasola, G
Huet, JM
White, R
Dmytriiev, A
Sol, H
Zech, A
Abchiche, A
Amans, JP
Armstrong, TP
Barcelo, M
Berge, D
Brown, AM
Buchholtz, G
Chadwick, PM
Clark, P
Cotter, G
Dangeon, L
De Frondat, F
Deiml, P
Dournaux, JL
Duffy, C
Einecke, S
Flis, S
Funk, S
Giavitto, G
Gironnet, J
Graham, JA
Greenshaw, T
Hinton, JA
Jégouzo, I
Kraus, M
Lapington, JS
Laporte, P
Leach, SA
Lloyd, S
Minaya, IA
Morier, R
Okumura, A
Prokoph, H
Ross, D
Rowell, G
Rulten, CB
Schoorlemmer, H
Schmoll, J
Spencer, ST
Stephan, M
Stuik, R
Tajima, H
Thornhill, J
Tibaldo, L
Vink, J
Watson, JJ
Williams, J
Zink, A
Zorn, J
First Published: 6-Jul-2018
Presented at: SPIE Astronomical Telescopes + Instrumentation, 2018, Austin, Texas, United States
Publisher: Society of Photo-optical Instrumentation Engineers (SPIE)
Citation: Proceedings of SPIE - The International Society for Optical Engineering, 2018, 10700, Ground-based and Airborne Telescopes VII; 1070010
Abstract: The Gamma-ray Cherenkov Telescope (GCT) is one of the telescopes proposed for the Small Sized Telescope (SST) section of CTA. Based on a dual-mirror Schwarzschild-Couder design, which allows for more compact telescopes and cameras than the usual single-mirror designs, it will be equipped with a Compact High-Energy Camera (CHEC) based on silicon photomultipliers (SiPM). In 2015, the GCT prototype was the first dual-mirror telescope constructed in the prospect of CTA to record Cherenkov light on the night sky. Further tests and observations have been performed since then. This report describes the current status of the GCT, the results of tests performed to demonstrate its compliance with CTA requirements, and the optimisation of the design for mass production. The GCT collaboration, including teams from Australia, France, Germany, Japan, the Netherlands and the United Kingdom, plans to install the first telescopes on site in Chile for 2019-2020 as part of the CTA pre-production phase.
DOI Link: 10.1117/12.2313158
ISSN: 0277-786X
ISBN: 9781510619531
eISSN: 1996-756X
Links: https://www.spiedigitallibrary.org/conference-proceedings-of-spie/10700/1070010/Final-characterisation-and-design-of-the-Gamma-ray-Cherenkov-Telescope/10.1117/12.2313158.short?SSO=1
http://hdl.handle.net/2381/44351
Version: Post-print
Status: Peer-reviewed
Type: Conference Paper
Rights: Copyright © 2018, Society of Photo-optical Instrumentation Engineers (SPIE). Deposited with reference to the publisher’s open access archiving policy. (http://www.rioxx.net/licenses/all-rights-reserved)
Appears in Collections:Conference Papers & Presentations, Dept. of Physics and Astronomy

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