Development of the camera for the Large Size Telescopes of the Cherenkov Telescope Array

被引：5

作者：

Inome, Y. ^{[1
]}

Ambrosi, G. ^{[2
]}

Awane, Y. ^{[3
]}

Baba, H. ^{[4
]}

Bamba, A. ^{[5
]}

Barcelo, M. ^{[6
]}

Barres de Almeida, U. ^{[7
]}

Barrio, J. A. ^{[8
]}

Blanch Bigas, O. ^{[6
]}

Boix, J. ^{[6
]}

Brunetti, L. ^{[9
]}

Carmona, E. ^{[10
]}

Chabanne, E. ^{[9
]}

Chikawa, M. ^{[11
]}

Cho, N. ^{[4
]}

Colin, P. ^{[12
]}

Conteras, J. L. ^{[8
]}

Cortina, J. ^{[6
]}

Dazzi, F. ^{[13
]}

Deangelis, A. ^{[14
,15
]}

Deleglise, G. ^{[9
]}

Delgado, C. ^{[10
]}

Diaz, C. ^{[10
]}

Dubois, F. ^{[8
]}

Fiasson, A. ^{[9
]}

Fink, D. ^{[12
]}

Fouque, N. ^{[9
]}

Freixas, L. ^{[10
]}

Fruck, C. ^{[12
]}

Gadola, A. ^{[16
]}

Garcia, R. ^{[17
]}

Gascon, D. ^{[18
]}

Geffroy, N. ^{[9
]}

Giglietto, N. ^{[19
]}

Giordano, F. ^{[19
]}

Granena, F. ^{[6
]}

Gunji, S. ^{[20
]}

Hagiwara, R. ^{[20
]}

Hamer, N. ^{[10
]}

Hanabata, Y. ^{[21
]}

Hassan, T. ^{[8
]}

Hatanaka, K. ^{[3
]}

Haubold, T. ^{[12
]}

Hayashida, M. ^{[21
]}

Hermel, R. ^{[9
]}

Herranz, D. ^{[8
]}

Hirotani, K. ^{[21
]}

Hose, J. ^{[12
]}

Hugh, D. ^{[12
]}

Inoue, S. ^{[21
]}

机构：

[1] Konan Univ, Dept Phys, Kobe, Hyogo 6588501, Japan

[2] Ist Nazl Fis Nucl, Sez Perugia, I-06100 Perugia, Italy

[3] Kyoto Univ, Sakyo Ku, Kyoto 6068502, Japan

[4] Ibaraki Univ, Fac Sci, Mito, Ibaraki 3108512, Japan

[5] Aoyama Gakuin Univ, Dept Math & Phys, Sagamihara, Kanagawa 2298558, Japan

[6] Inst Fsica Altes Energies, Bellaterra 08193, Spain

[7] Ctr Brasileiro Pesquisas Fis CBPF MCTI, BR-22290180 Rio De Janeiro, Brazil

[8] Univ Complutense Madrid, Grp Altas Energas, E-28040 Madrid, Spain

[9] Univ Savoie, LAPP, CNRS, IN2P3, F-74941 Annecy Le Vieux, France

[10] CIEMAT, E-28040 Madrid, Spain

[11] Kinki Univ, Dept Phys, Higashiosaka, Osaka 5778502, Japan

[12] Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany

[13] Univ Padua, Dipartimento Fis, I-35131 Padua, Italy

[14] Univ Udine, I-33100 Udine, Italy

[15] Ist Nazl Fis Nucl, Sez Trieste, I-33100 Udine, Italy

[16] Univ Zurich, Inst Phys, CH-8057 Zurich, Switzerland

[17] Inst Astrofis Canarias, Tenerife 38205, Spain

[18] Univ Barcelona, Dept Astron & Meteorol ICC UB, E-08028 Barcelona, Spain

[19] Ist Nazl Fis Nucl, Sez Bari, I-70126 Bari, Italy

[20] Yamagata Univ, Dept Phys, Yamagata, Yamagata 9908560, Japan

[21] Univ Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba 2778582, Japan

[22] High Energy Accelerator Org, Inst Particle & Nucl Studies, KEK, Tsukuba, Ibaraki 3050801, Japan

[23] Waseda Univ, Fac Sci & Engn, Shinjuku Ku, Tokyo 1698555, Japan

[24] Tokai Univ, Dept Phys, Hiratsuka, Kanagawa 2591292, Japan

[25] Saitama Univ, Sakura Ku, Saitama 3388570, Japan

[26] Saha Inst Nucl Phys, Kolkata, India

[27] RIKEN, Adv Sci Inst, Wako, Saitama 3510198, Japan

[28] Univ Complutense Madrid, Grp Elect, E-28040 Madrid, Spain

[29] Nagoya Univ, Chikusa Ku, Nagoya, Aichi 4648602, Japan

[30] Univ Tokushima, Inst Socio Arts & Sci, Tokushima 7708502, Japan

[31] Univ Siena, I-53100 Siena, Italy

[32] Ist Nazl Fis Nucl, Sez Pisa, I-53100 Siena, Italy

[33] Univ Tokyo, Dept Phys, Grad Sch Sci, Bunkyo Ku, Tokyo 1130033, Japan

来源：

ADVANCES IN OPTICAL AND MECHANICAL TECHNOLOGIES FOR TELESCOPES AND INSTRUMENTATION | 2014年 / 9151卷

关键词：

Imaging Atmospheric Cherenkov Telescope; CTA; gamma-rays;

D O I：

10.1117/12.2054619

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Large Size Telescopes, LSTs, located at the center of the Cherenkov Telescope Array, CTA, will be sensitive for low energy gamma-rays. The camera on the LST focal plane is optimized to detect low energy events based on a high photon detection efficiency and high speed electronics. Also the trigger system is designed to detect low energy showers as much as possible. In addition, the camera is required to work stably without maintenance in a few tens of years. In this contribution we present the design of the camera for the first LST and the status of its development and production.

引用

页数：8

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