Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/44351
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dc.contributor.authorLe Blanc, O-
dc.contributor.authorFasola, G-
dc.contributor.authorHuet, JM-
dc.contributor.authorWhite, R-
dc.contributor.authorDmytriiev, A-
dc.contributor.authorSol, H-
dc.contributor.authorZech, A-
dc.contributor.authorAbchiche, A-
dc.contributor.authorAmans, JP-
dc.contributor.authorArmstrong, TP-
dc.contributor.authorBarcelo, M-
dc.contributor.authorBerge, D-
dc.contributor.authorBrown, AM-
dc.contributor.authorBuchholtz, G-
dc.contributor.authorChadwick, PM-
dc.contributor.authorClark, P-
dc.contributor.authorCotter, G-
dc.contributor.authorDangeon, L-
dc.contributor.authorDe Frondat, F-
dc.contributor.authorDeiml, P-
dc.contributor.authorDournaux, JL-
dc.contributor.authorDuffy, C-
dc.contributor.authorEinecke, S-
dc.contributor.authorFlis, S-
dc.contributor.authorFunk, S-
dc.contributor.authorGiavitto, G-
dc.contributor.authorGironnet, J-
dc.contributor.authorGraham, JA-
dc.contributor.authorGreenshaw, T-
dc.contributor.authorHinton, JA-
dc.contributor.authorJégouzo, I-
dc.contributor.authorKraus, M-
dc.contributor.authorLapington, JS-
dc.contributor.authorLaporte, P-
dc.contributor.authorLeach, SA-
dc.contributor.authorLloyd, S-
dc.contributor.authorMinaya, IA-
dc.contributor.authorMorier, R-
dc.contributor.authorOkumura, A-
dc.contributor.authorProkoph, H-
dc.contributor.authorRoss, D-
dc.contributor.authorRowell, G-
dc.contributor.authorRulten, CB-
dc.contributor.authorSchoorlemmer, H-
dc.contributor.authorSchmoll, J-
dc.contributor.authorSpencer, ST-
dc.contributor.authorStephan, M-
dc.contributor.authorStuik, R-
dc.contributor.authorTajima, H-
dc.contributor.authorThornhill, J-
dc.contributor.authorTibaldo, L-
dc.contributor.authorVink, J-
dc.contributor.authorWatson, JJ-
dc.contributor.authorWilliams, J-
dc.contributor.authorZink, A-
dc.contributor.authorZorn, J-
dc.date.accessioned2019-06-11T11:33:57Z-
dc.date.available2019-06-11T11:33:57Z-
dc.date.issued2018-07-06-
dc.identifier.citationProceedings of SPIE - The International Society for Optical Engineering, 2018, 10700, Ground-based and Airborne Telescopes VII; 1070010en
dc.identifier.isbn9781510619531-
dc.identifier.issn0277-786X-
dc.identifier.urihttps://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=1en
dc.identifier.urihttp://hdl.handle.net/2381/44351-
dc.description.abstractThe 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.en
dc.description.sponsorshipThis work was conducted in the context of the CTA Consortium. We gratefully acknowledge support from the agencies and organizations listed under Funding Agencies at this website: http://www.cta-observatory.org/consortium_acknowledgmentsen
dc.language.isoenen
dc.publisherSociety of Photo-optical Instrumentation Engineers (SPIE)en
dc.rightsCopyright © 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)en
dc.subjectAtmospheric Cherenkov telescopesen
dc.subjectTelescopesen
dc.subjectCamerasen
dc.subjectMirrorsen
dc.subjectPrototypingen
dc.subjectOptical instrument designen
dc.subjectComputer aided designen
dc.titleFinal characterisation and design of the Gamma-ray Cherenkov Telescope (GCT) for the Cherenkov Telescope Arrayen
dc.typeConference Paperen
dc.identifier.doi10.1117/12.2313158-
dc.identifier.eissn1996-756X-
dc.description.statusPeer-revieweden
dc.description.versionPost-printen
dc.description.presentedSPIE Astronomical Telescopes + Instrumentation, 2018, Austin, Texas, United Statesen
pubs.organisational-group/Organisationen
pubs.organisational-group/Organisation/COLLEGE OF SCIENCE AND ENGINEERINGen
pubs.organisational-group/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomyen
Appears in Collections:Conference Papers & Presentations, Dept. of Physics and Astronomy

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