Tibet air shower array: results and future plan

M Amenomori; X J Bi; D Chen; S W Cui; Danzengluobu; L K Ding; X H Ding; C Fan; C F Feng; Z Feng; Z Y Feng; X Y Gao; Q X Geng; H W Guo; H H He; M He; K Hibino; N Hotta; H Hu; H B Hu; J Huang; Q Huang; H Y Jia; F Kajino; K Kasahara; Y Katayose; C Kato; K Kawata; Labaciren; G M Le; A F Li; J Y Li; Y -Q Lou; H Lu; S L Lu; X R Meng; K Mizutani; J Mu; K Munakata; A Nagai; H Nanjo; M Nishizawa; M Ohnishi; I Ohta; H Onuma; T Ouchi; S Ozawa; J R Ren; T Saito; T Y Saito; M Sakata; T K Sako; M Shibata; A Shiomi; T Shirai; H Sugimoto; M Takita; Y H Tan; N Tateyama; S Torii; H Tsuchiya; S Udo; B Wang; H Wang; X Wang; Y Wang; Y G Wang; H R Wu; L Xue; Y Yamamoto; C T Yan; X C Yang; S Yasue; Z H Ye; G C Yu; A F Yuan; T Yuda; H M Zhang; J L Zhang; N J Zhang; X Y Zhang; Y Zhang; Y Zhang; Zhaxisangzhu; X X Zhou; (The Tibet ASγ Collaboration)

doi:10.1088/1742-6596/120/6/062024

Journal of Physics: Conference Series

The following article is Open access

Tibet air shower array: results and future plan

M Amenomori¹, X J Bi², D Chen³, S W Cui⁴, Danzengluobu⁵, L K Ding², X H Ding⁵, C Fan⁶, C F Feng⁶, Z Feng², Z Y Feng⁷, X Y Gao⁸, Q X Geng⁸, H W Guo⁵, H H He², M He⁶, K Hibino⁹, N Hotta¹⁰, H Hu⁵, H B Hu², J Huang¹¹, Q Huang⁷, H Y Jia⁷, F Kajino¹², K Kasahara¹³, Y Katayose³, C Kato¹⁴, K Kawata, Labaciren⁵, G M Le¹⁵, A F Li⁶, J Y Li⁶, Y -Q Lou¹⁶, H Lu², S L Lu², X R Meng⁵, K Mizutani, J Mu⁸, K Munakata¹⁴, A Nagai¹⁸, H Nanjo¹, M Nishizawa¹⁹, M Ohnishi¹¹, I Ohta²⁰, H Onuma¹⁷, T Ouchi⁹, S Ozawa¹¹, J R Ren², T Saito²¹, T Y Saito²², M Sakata¹², T K Sako¹¹, M Shibata³, A Shiomi, T Shirai⁹, H Sugimoto²³, M Takita¹¹, Y H Tan², N Tateyama⁹, S Torii¹³, H Tsuchiya²⁴, S Udo¹¹, B Wang⁸, H Wang², X Wang¹¹, Y Wang², Y G Wang⁶, H R Wu², L Xue⁶, Y Yamamoto¹², C T Yan¹¹, X C Yang⁸, S Yasue²⁵, Z H Ye¹⁵, G C Yu⁷, A F Yuan⁵, T Yuda⁹, H M Zhang², J L Zhang², N J Zhang⁶, X Y Zhang⁶, Y Zhang², Y Zhang², Zhaxisangzhu⁵, X X Zhou⁷ and (The Tibet ASγ Collaboration)¹

Published under licence by IOP Publishing Ltd
Journal of Physics: Conference Series, Volume 120, COSMIC RAYS AND NEUTRINOS, GAMMA RAYS Citation M Amenomori et al 2008 J. Phys.: Conf. Ser. 120 062024 DOI 10.1088/1742-6596/120/6/062024

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¹ Department of Physics, Hirosaki University, Hirosaki 036-8561, Japan

² Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China

³ Faculty of Engineering, Yokohama National University, Yokohama 240-8501, Japan

⁴ Department of Physics, Hebei Normal University, Shijiazhuang 050016, China

⁵ Department of Mathematics and Physics, Tibet University, Lhasa 850000, China

⁶ Department of Physics, Shandong University, Jinan 250100, China

⁷ Institute of Modern Physics, SouthWest Jiaotong University, Chengdu 610031, China

⁸ Department of Physics, Yunnan University, Kunming 650091, China

⁹ Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan

¹⁰ Faculty of Education, Utsunomiya University, Utsunomiya 321-8505, Japan

¹¹ Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan

¹² Department of Physics, Konan University, Kobe 658-8501, Japan

¹³ Research Institute for Science and Engineering, Waseda University, Tokyo 169-8555, Japan

¹⁴ Department of Physics, Shinshu University, Matsumoto 390-8621, Japan

¹⁵ Center of Space Science and Application Research, Chinese Academy of Sciences, Beijing 100080, China

¹⁶ Physics Department and Tsinghua Center for Astrophysics, Tsinghua University, Beijing 100084, China

¹⁷ Department of Physics, Saitama University, Saitama 338-8570, Japan

¹⁸ Advanced Media Network Center, Utsunomiya University, Utsunomiya 321-8585, Japan

¹⁹ National Institute of Informatics, Tokyo 101-8430, Japan

²⁰ Tochigi Study Center, University of the Air, Utsunomiya 321-0943, Japan

²¹ Tokyo Metropolitan College of Industrial Technology, Tokyo 116-8523, Japan

²² Max-Planck-Institut für Physik, München D-80805, Deutschland

²³ Shonan Institute of Technology, Fujisawa 251-8511, Japan

²⁴ RIKEN, Wako 351-0198, Japan

²⁵ School of General Education, Shinshu University, Matsumoto 390-8621, Japan

²⁶ Paper presented at the conference by K. Kawata

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Abstract

The Tibet air shower array, which has an effective area of 36,900 m², has been in operation at Yangbajing in Tibet, China at an altitude of 4,300 m above sea level. In this paper, we will briefly introduce the recent gamma-ray observation with the present Tibet air shower array and our future plan which is called the Tibet muon detector (MD) project.

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