Search for gamma rays above 100 TeV from the crab nebula using the tibet air shower array and the 100 m2 muon detector

M. Amenomori, X. J. Bi, D. Chen, T. L. Chen, W. Y. Chen, S. W. Cui, Danzengluobu, L. K. Ding, C. F. Feng, Zhaoyang Feng, Z. Y. Feng, Q. B. Gou, Y. Q. Guo, H. H. He, Z. T. He, K. Hibino, N. Hotta, Haibing Hu, H. B. Hu, J. Huang & 64 others H. Y. Jia, L. Jiang, F. Kajino, K. Kasahara, Y. Katayose, C. Kato, K. Kawata, M. Kozai, Labaciren, G. M. Le, A. F. Li, H. J. Li, W. J. Li, C. Liu, J. S. Liu, M. Y. Liu, H. Lu, X. R. Meng, T. Miyazaki, K. Mizutani, K. Munakata, T. Nakajima, Y. Nakamura, H. Nanjo, M. Nishizawa, T. Niwa, M. Ohnishi, I. Ohta, Shunsuke Ozawa, X. L. Qian, X. B. Qu, T. Saito, T. Y. Saito, M. Sakata, T. K. Sako, J. Shao, M. Shibata, A. Shiomi, T. Shirai, H. Sugimoto, M. Takita, Y. H. Tan, N. Tateyama, Shoji Torii, H. Tsuchiya, S. Udo, H. Wang, H. R. Wu, L. Xue, Y. Yamamoto, K. Yamauchi, Z. Yang, S. Yasue, A. F. Yuan, T. Yuda, L. M. Zhai, H. M. Zhang, J. L. Zhang, X. Y. Zhang, Y. Zhang, Yi Zhang, Ying Zhang, Zhaxisangzhu, X. X. Zhou

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1 Citation (Scopus)

Abstract

We search for continuous gamma-ray emission from the Crab Nebula above 100 TeV, using the data collected from March 2008 to July 2009 by the Tibet air shower array and the 100 m2 muon detector. We find that our MC simulation is in good agreement with the experimental data. No significant excess is found. An upper limit, comparable to the world's best limit until now, is obtained above 140 TeV.

Original languageEnglish
Article number833
JournalUnknown Journal
Volume30-July-2015
Publication statusPublished - 2015

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Crab nebula
Tibet
cosmic ray showers
muons
gamma rays
detectors
simulation

ASJC Scopus subject areas

  • General

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Amenomori, M., Bi, X. J., Chen, D., Chen, T. L., Chen, W. Y., Cui, S. W., ... Zhou, X. X. (2015). Search for gamma rays above 100 TeV from the crab nebula using the tibet air shower array and the 100 m2 muon detector. Unknown Journal, 30-July-2015, [833].

Search for gamma rays above 100 TeV from the crab nebula using the tibet air shower array and the 100 m2 muon detector. / Amenomori, M.; Bi, X. J.; Chen, D.; Chen, T. L.; Chen, W. Y.; Cui, S. W.; Danzengluobu; Ding, L. K.; Feng, C. F.; Feng, Zhaoyang; Feng, Z. Y.; Gou, Q. B.; Guo, Y. Q.; He, H. H.; He, Z. T.; Hibino, K.; Hotta, N.; Hu, Haibing; Hu, H. B.; Huang, J.; Jia, H. Y.; Jiang, L.; Kajino, F.; Kasahara, K.; Katayose, Y.; Kato, C.; Kawata, K.; Kozai, M.; Labaciren; Le, G. M.; Li, A. F.; Li, H. J.; Li, W. J.; Liu, C.; Liu, J. S.; Liu, M. Y.; Lu, H.; Meng, X. R.; Miyazaki, T.; Mizutani, K.; Munakata, K.; Nakajima, T.; Nakamura, Y.; Nanjo, H.; Nishizawa, M.; Niwa, T.; Ohnishi, M.; Ohta, I.; Ozawa, Shunsuke; Qian, X. L.; Qu, X. B.; Saito, T.; Saito, T. Y.; Sakata, M.; Sako, T. K.; Shao, J.; Shibata, M.; Shiomi, A.; Shirai, T.; Sugimoto, H.; Takita, M.; Tan, Y. H.; Tateyama, N.; Torii, Shoji; Tsuchiya, H.; Udo, S.; Wang, H.; Wu, H. R.; Xue, L.; Yamamoto, Y.; Yamauchi, K.; Yang, Z.; Yasue, S.; Yuan, A. F.; Yuda, T.; Zhai, L. M.; Zhang, H. M.; Zhang, J. L.; Zhang, X. Y.; Zhang, Y.; Zhang, Yi; Zhang, Ying; Zhaxisangzhu; Zhou, X. X.

In: Unknown Journal, Vol. 30-July-2015, 833, 2015.

Research output: Contribution to journalArticle

Amenomori, M, Bi, XJ, Chen, D, Chen, TL, Chen, WY, Cui, SW, Danzengluobu, Ding, LK, Feng, CF, Feng, Z, Feng, ZY, Gou, QB, Guo, YQ, He, HH, He, ZT, Hibino, K, Hotta, N, Hu, H, Hu, HB, Huang, J, Jia, HY, Jiang, L, Kajino, F, Kasahara, K, Katayose, Y, Kato, C, Kawata, K, Kozai, M, Labaciren, Le, GM, Li, AF, Li, HJ, Li, WJ, Liu, C, Liu, JS, Liu, MY, Lu, H, Meng, XR, Miyazaki, T, Mizutani, K, Munakata, K, Nakajima, T, Nakamura, Y, Nanjo, H, Nishizawa, M, Niwa, T, Ohnishi, M, Ohta, I, Ozawa, S, Qian, XL, Qu, XB, Saito, T, Saito, TY, Sakata, M, Sako, TK, Shao, J, Shibata, M, Shiomi, A, Shirai, T, Sugimoto, H, Takita, M, Tan, YH, Tateyama, N, Torii, S, Tsuchiya, H, Udo, S, Wang, H, Wu, HR, Xue, L, Yamamoto, Y, Yamauchi, K, Yang, Z, Yasue, S, Yuan, AF, Yuda, T, Zhai, LM, Zhang, HM, Zhang, JL, Zhang, XY, Zhang, Y, Zhang, Y, Zhang, Y, Zhaxisangzhu & Zhou, XX 2015, 'Search for gamma rays above 100 TeV from the crab nebula using the tibet air shower array and the 100 m2 muon detector', Unknown Journal, vol. 30-July-2015, 833.
Amenomori, M. ; Bi, X. J. ; Chen, D. ; Chen, T. L. ; Chen, W. Y. ; Cui, S. W. ; Danzengluobu ; Ding, L. K. ; Feng, C. F. ; Feng, Zhaoyang ; Feng, Z. Y. ; Gou, Q. B. ; Guo, Y. Q. ; He, H. H. ; He, Z. T. ; Hibino, K. ; Hotta, N. ; Hu, Haibing ; Hu, H. B. ; Huang, J. ; Jia, H. Y. ; Jiang, L. ; Kajino, F. ; Kasahara, K. ; Katayose, Y. ; Kato, C. ; Kawata, K. ; Kozai, M. ; Labaciren ; Le, G. M. ; Li, A. F. ; Li, H. J. ; Li, W. J. ; Liu, C. ; Liu, J. S. ; Liu, M. Y. ; Lu, H. ; Meng, X. R. ; Miyazaki, T. ; Mizutani, K. ; Munakata, K. ; Nakajima, T. ; Nakamura, Y. ; Nanjo, H. ; Nishizawa, M. ; Niwa, T. ; Ohnishi, M. ; Ohta, I. ; Ozawa, Shunsuke ; Qian, X. L. ; Qu, X. B. ; Saito, T. ; Saito, T. Y. ; Sakata, M. ; Sako, T. K. ; Shao, J. ; Shibata, M. ; Shiomi, A. ; Shirai, T. ; Sugimoto, H. ; Takita, M. ; Tan, Y. H. ; Tateyama, N. ; Torii, Shoji ; Tsuchiya, H. ; Udo, S. ; Wang, H. ; Wu, H. R. ; Xue, L. ; Yamamoto, Y. ; Yamauchi, K. ; Yang, Z. ; Yasue, S. ; Yuan, A. F. ; Yuda, T. ; Zhai, L. M. ; Zhang, H. M. ; Zhang, J. L. ; Zhang, X. Y. ; Zhang, Y. ; Zhang, Yi ; Zhang, Ying ; Zhaxisangzhu ; Zhou, X. X. / Search for gamma rays above 100 TeV from the crab nebula using the tibet air shower array and the 100 m2 muon detector. In: Unknown Journal. 2015 ; Vol. 30-July-2015.
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abstract = "We search for continuous gamma-ray emission from the Crab Nebula above 100 TeV, using the data collected from March 2008 to July 2009 by the Tibet air shower array and the 100 m2 muon detector. We find that our MC simulation is in good agreement with the experimental data. No significant excess is found. An upper limit, comparable to the world's best limit until now, is obtained above 140 TeV.",
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TY - JOUR

T1 - Search for gamma rays above 100 TeV from the crab nebula using the tibet air shower array and the 100 m2 muon detector

AU - Amenomori, M.

AU - Bi, X. J.

AU - Chen, D.

AU - Chen, T. L.

AU - Chen, W. Y.

AU - Cui, S. W.

AU - Danzengluobu,

AU - Ding, L. K.

AU - Feng, C. F.

AU - Feng, Zhaoyang

AU - Feng, Z. Y.

AU - Gou, Q. B.

AU - Guo, Y. Q.

AU - He, H. H.

AU - He, Z. T.

AU - Hibino, K.

AU - Hotta, N.

AU - Hu, Haibing

AU - Hu, H. B.

AU - Huang, J.

AU - Jia, H. Y.

AU - Jiang, L.

AU - Kajino, F.

AU - Kasahara, K.

AU - Katayose, Y.

AU - Kato, C.

AU - Kawata, K.

AU - Kozai, M.

AU - Labaciren,

AU - Le, G. M.

AU - Li, A. F.

AU - Li, H. J.

AU - Li, W. J.

AU - Liu, C.

AU - Liu, J. S.

AU - Liu, M. Y.

AU - Lu, H.

AU - Meng, X. R.

AU - Miyazaki, T.

AU - Mizutani, K.

AU - Munakata, K.

AU - Nakajima, T.

AU - Nakamura, Y.

AU - Nanjo, H.

AU - Nishizawa, M.

AU - Niwa, T.

AU - Ohnishi, M.

AU - Ohta, I.

AU - Ozawa, Shunsuke

AU - Qian, X. L.

AU - Qu, X. B.

AU - Saito, T.

AU - Saito, T. Y.

AU - Sakata, M.

AU - Sako, T. K.

AU - Shao, J.

AU - Shibata, M.

AU - Shiomi, A.

AU - Shirai, T.

AU - Sugimoto, H.

AU - Takita, M.

AU - Tan, Y. H.

AU - Tateyama, N.

AU - Torii, Shoji

AU - Tsuchiya, H.

AU - Udo, S.

AU - Wang, H.

AU - Wu, H. R.

AU - Xue, L.

AU - Yamamoto, Y.

AU - Yamauchi, K.

AU - Yang, Z.

AU - Yasue, S.

AU - Yuan, A. F.

AU - Yuda, T.

AU - Zhai, L. M.

AU - Zhang, H. M.

AU - Zhang, J. L.

AU - Zhang, X. Y.

AU - Zhang, Y.

AU - Zhang, Yi

AU - Zhang, Ying

AU - Zhaxisangzhu,

AU - Zhou, X. X.

PY - 2015

Y1 - 2015

N2 - We search for continuous gamma-ray emission from the Crab Nebula above 100 TeV, using the data collected from March 2008 to July 2009 by the Tibet air shower array and the 100 m2 muon detector. We find that our MC simulation is in good agreement with the experimental data. No significant excess is found. An upper limit, comparable to the world's best limit until now, is obtained above 140 TeV.

AB - We search for continuous gamma-ray emission from the Crab Nebula above 100 TeV, using the data collected from March 2008 to July 2009 by the Tibet air shower array and the 100 m2 muon detector. We find that our MC simulation is in good agreement with the experimental data. No significant excess is found. An upper limit, comparable to the world's best limit until now, is obtained above 140 TeV.

UR - http://www.scopus.com/inward/record.url?scp=84988728355&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84988728355&partnerID=8YFLogxK

M3 - Article

VL - 30-July-2015

JO - Nuclear Physics A

JF - Nuclear Physics A

SN - 0375-9474

M1 - 833

ER -