arxiv: 1307.4565 · v1 · ★pith:G6BEZWYAnew · submitted 2013-07-17 · 🌌 astro-ph.IM
The Cherenkov Telescope Array Large Size Telescope
G. Ambrosi
,
Y. Awane
,
H. Baba
,
A. Bamba
,
M. Barcel\'o
,
U. Barres de Almeida
,
J.A. Barrio
,
O. Blanch Bigas
This is my paper
show 124 more authors
J. Boix
L. Brunetti
E. Carmona
E. Chabanne
M. Chikawa
P. Colin
J.L. Conteras
J. Cortina
F. Dazzi
A. Deangelis
G. Deleglise
C. Delgado
C. D\'iaz
F. Dubois
A. Fiasson
D. Fink
N. Fouque
L. Freixas
C. Fruck
A. Gadola
R. Garc\'ia
D. Gascon
N. Geffroy
N. Giglietto
F. Giordano
F. Gra\~nena
S. Gunji
R. Hagiwara
N. Hamer
Y. Hanabata
T. Hassan
K. Hatanaka
T. Haubold
M. Hayashida
R. Hermel
D. Herranz
K. Hirotani
S. Inoue
Y. Inoue
K. Ioka
C. Jablonski
M. Kagaya
H. Katagiri
T. Kishimoto
K. Kodani
K. Kohri
Y. Konno
S. Koyama
H. Kubo
J. Kushida
G. Lamanna
T. Le Flour
M. L\'opez-Moya
R. L\'opez
E. Lorenz
P. Majumdar
A. Manalaysay
M. Mariotti
G. Mart\'inez
M. Mart\'inez
D. Mazin
J.M. Miranda
R. Mirzoyan
I. Monteiro
A. Moralejo
K. Murase
S. Nagataki
D. Nakajima
T. Nakamori
K. Nishijima
K. Noda
A. Nozato
Y. Ohira
M. Ohishi
H. Ohoka
A. Okumura
R. Orito
J.L. Panazol
D. Paneque
R. Paoletti
J.M. Paredes
G. Pauletta
S. Podkladkin
J. Prast
R. Rando
O. Reimann
M. Rib\'o
S. Rosier-Lees
K. Saito
T. Saito
Y. Saito
N. Sakaki
R. Sakonaka
A. Sanuy
H. Sasaki
M. Sawada
V. Scalzotto
S. Schultz
T. Schweizer
T. Shibata
S. Shu
J. Sieiro
V. Stamatescu
S. Steiner
U. Straumann
R. Sugawara
H. Tajima
H. Takami
S. Tanaka
M. Tanaka
L.A. Tejedor
Y. Terada
M. Teshima
T. Totani
H. Ueno
K. Umehara
A. Vollhardt
R. Wagner
H. Wetteskind
T. Yamamoto
R. Yamazaki
A. Yoshida
T. Yoshida
T. Yoshikoshi (for the CTA Consortium)
classification
🌌 astro-ph.IM
keywords
telescopearraycherenkovlargesizetelescopeswillachieve
read the original abstract
The two arrays of the Very High Energy gamma-ray observatory Cherenkov Telescope Array (CTA) will include four Large Size Telescopes (LSTs) each with a 23 m diameter dish and 28 m focal distance. These telescopes will enable CTA to achieve a low-energy threshold of 20 GeV, which is critical for important studies in astrophysics, astroparticle physics and cosmology. This work presents the key specifications and performance of the current LST design in the light of the CTA scientific objectives.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.