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Dournaux--Operating performance of the gamma-ray Cherenkov telescope NIMA(2017).pdf (4.54 MB)

Operating performance of the gamma-ray Cherenkov telescope: An end-to-end Schwarzschild-Couder telescope prototype for the Cherenkov Telescope Array

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journal contribution
posted on 2019-03-20, 10:20 authored by JL Dournaux, A De Franco, P Laporte, R White, T Greenshaw, H Sol, A Abchiche, D Allan, JP Amans, TP Armstrong, A Balzer, D Berge, C Boisson, JJ Bousquet, AM Brown, M Bryan, G Buchholtz, PM Chadwick, H Costantini, G Cotter, M Daniel, F De Frondat, D Dumas, JP Ernenwein, G Fasola, S Funk, J Gaudemard, JA Graham, J Gironnet, O Hervet, N Hidaka, JA Hinton, JM Huet, I Jegouzo, T Jogler, T Kawashima, M Kraus, JS Lapington, J Lefaucheur, S Markoff, T Melse, L Morhrmann, P Molnyeux, SJ Nolan, A Okumura, RD Parsons, D Ross, G Rowell, Y Sato, F Sayede, J Schmoll, H Schoorlemmer, M Servillat, V Stamatescu, M Stephan, R Stuik, J Sykes, H Tajima, J Thornhill, L Tibaldo, C Trichard, J Vinkh, J Watson, N Yamane, A Zech, A Zink
The Cherenkov Telescope Array (CTA) consortium aims to build the next-generation ground-based very-high-energy gamma-ray observatory. The array will feature different sizes of telescopes allowing it to cover a wide gamma-ray energy band from about 20 GeV to above 100 TeV. The highest energies, above 5 TeV, will be covered by a large number of Small-Sized Telescopes (SSTs) with a field-of-view of around 9°. The Gamma-ray Cherenkov Telescope (GCT), based on Schwarzschild–Couder dual-mirror optics, is one of the three proposed SST designs. The GCT is described in this contribution and the first images of Cherenkov showers obtained using the telescope and its camera are presented. These were obtained in November 2015 in Meudon, France.

Funding

The authors gratefully acknowledge support from the agencies and organisations listed under Funding Agencies at this website: http://www.cta-observatory.org/.

History

Citation

Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2017, 845, pp. 355-358

Author affiliation

/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy

Version

  • AM (Accepted Manuscript)

Published in

Nuclear Instruments and Methods in Physics Research Section A: Accelerators

Publisher

Elsevier for North-Holland

issn

0168-9002

eissn

1872-9576

Acceptance date

2016-05-14

Copyright date

2016

Available date

2019-03-20

Publisher version

https://www.sciencedirect.com/science/article/pii/S016890021630448X?via=ihub

Language

en