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

Dournaux, J.L.; De Franco, A.; Laporte, P.; White, R.; Greenshaw, T.; Sol, H.; Abchiche, A.; Allan, D.; Amans, J.P.; Armstrong, T.P.; Balzer, A.; Berge, D.; Boisson, C.; Bousquet, J.J.; Brown, A.M.; Bryan, M.; Buchholtz, G.; Chadwick, P.M.; Costantini, H.; Cotter, G.; Daniel, M.; De Frondat, F.; Dumas, D.; Ernenwein, J.P.; Fasola, G.; Funk, S.; Gaudemard, J.; Graham, J.A.; Gironnet, J.; Hervet, O.; Hidaka, N.; Hinton, J.A.; Huet, J.M.; Jégouzo, I.; Jogler, T.; Kawashima, T.; Kraus, M.; Lapington, J.S.; Lefaucheur, J.; Markoff, S.; Melse, T.; Morhrmann, L.; Molnyeux, P.; Nolan, S.J.; Okumura, A.; Parsons, R.D.; Ross, D.; Rowell, G.; Sato, Y.; Sayède, F.; Schmoll, J.; Schoorlemmer, H.; Servillat, M.; Stamatescu, V.; Stephan, M.; Stuik, R.; Sykes, J.; Tajima, H.; Thornhill, J.; Tibaldo, L.; Trichard, C.; Vink, J.; Watson, J.; Yamane, N.; Zech, A.; Zink, A.

Authors

J.L. Dournaux

A. De Franco

P. Laporte

R. White

T. Greenshaw

H. Sol

A. Abchiche

D. Allan

J.P. Amans

T.P. Armstrong

A. Balzer

D. Berge

C. Boisson

J.J. Bousquet

A.M. Brown

M. Bryan

G. Buchholtz

H. Costantini

G. Cotter

M. Daniel

F. De Frondat

D. Dumas

J.P. Ernenwein

G. Fasola

S. Funk

J. Gaudemard

J.A. Graham

J. Gironnet

O. Hervet

N. Hidaka

J.A. Hinton

J.M. Huet

I. Jégouzo

T. Jogler

T. Kawashima

M. Kraus

J.S. Lapington

J. Lefaucheur

S. Markoff

T. Melse

L. Morhrmann

P. Molnyeux

S.J. Nolan

A. Okumura

R.D. Parsons

D. Ross

G. Rowell

Y. Sato

F. Sayède

J. Schmoll

H. Schoorlemmer

M. Servillat

V. Stamatescu

M. Stephan

R. Stuik

J. Sykes

H. Tajima

J. Thornhill

L. Tibaldo

C. Trichard

J. Vink

J. Watson

N. Yamane

A. Zech

A. Zink



Abstract

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.

Citation

Dournaux, J., De Franco, A., Laporte, P., White, R., Greenshaw, T., Sol, H., …Zink, A. (2017). Operating performance of the gamma-ray Cherenkov telescope: An end-to-end Schwarzschild–Couder telescope prototype for the Cherenkov Telescope Array. Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 845, 355-358. https://doi.org/10.1016/j.nima.2016.05.059

Journal Article Type Article
Acceptance Date May 14, 2016
Online Publication Date May 16, 2016
Publication Date 2017-02
Deposit Date Sep 28, 2017
Journal Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Print ISSN 0168-9002
Publisher Elsevier
Peer Reviewed Peer Reviewed
Volume 845
Pages 355-358
DOI https://doi.org/10.1016/j.nima.2016.05.059
Public URL https://durham-repository.worktribe.com/output/1375470