New flux upper limits of diffuse TeV gamma rays from the galactic plane observed with the tibet air shower array

M. Amenomori; S. Ayabe; D. Chen; S. W. Cui; Danzengluobu; L. K. Ding; X. H. Ding; C. F. Feng; Z. Y. Feng; X. Y. Gao; Q. X. Geng; H. W. Guo; H. H. He; M. He; K. Hibino; N. Hotta; Haibing 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; J. Y. Li; 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; Shunsuke Ozawa; J. R. Ren; T. Saito; M. Sakata; T. Sasaki; M. Shibata; A. Shiomi; T. Shirai; H. Sugimoto; M. Takita; Y. H. Tan; N. Tateyama; Shoji Torii; H. Tsuchiya; S. Udo; H. Wang; X. 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

New flux upper limits of diffuse TeV gamma rays from the galactic plane observed with the tibet air shower array

M. Amenomori, S. Ayabe, D. Chen, S. W. Cui, Danzengluobu, L. K. Ding, X. H. Ding, C. F. Feng, Z. Y. Feng, X. Y. Gao, Q. X. Geng, H. W. Guo, H. H. He, M. He, K. Hibino, N. Hotta, Haibing Hu, H. B. Hu, J. Huang, Q. HuangH. Y. Jia, F. Kajino, K. Kasahara, Y. Katayose, C. Kato, K. Kawata, Labaciren, G. M. Le, J. Y. Li, 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, Shunsuke Ozawa, J. R. Ren, T. Saito, M. Sakata, T. Sasaki, M. Shibata, A. Shiomi, T. Shirai, H. Sugimoto, M. Takita, Y. H. Tan, N. Tateyama, Shoji Torii, H. Tsuchiya, S. Udo, H. Wang, X. 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

研究成果: Conference contribution

3 被引用数 (Scopus)

抄録

The flux upper limits of the diffuse gamma rays, from the inner and outer Galactic planes, are found to be decreased by factors of 4.0∼3.6 for 3∼10 TeV, respectively, by using the simulation results of effective area ratios for gamma-ray and cosmic-ray induced showers in the Tibet air shower array. In our previous work, the flux upper limits were deduced only from the flux ratio of air showers generated by gamma rays versus cosmic rays. As a result the source electron spectral index for inverse Compton should be steeper than 2.2 and 2.1 for the inner and outer Galactic planes, respectively.

本文言語	English
ホスト出版物のタイトル	29th International Cosmic Ray Conference, ICRC 2005
出版社	Tata Institute of Fundamental Research
ページ	43-46
ページ数	4
巻	4
出版ステータス	Published - 2005
イベント	29th International Cosmic Ray Conference, ICRC 2005 - Pune 継続期間: 2005 8月 3 → 2005 8月 10

Other

Other	29th International Cosmic Ray Conference, ICRC 2005
City	Pune
Period	05/8/3 → 05/8/10

ASJC Scopus subject areas

核物理学および高エネルギー物理学

他のファイルとリンク

引用スタイル

Amenomori, M., Ayabe, S., Chen, D., Cui, S. W., Danzengluobu, Ding, L. K., Ding, X. H., Feng, C. F., Feng, Z. Y., Gao, X. Y., Geng, Q. X., Guo, H. W., He, H. H., He, M., Hibino, K., Hotta, N., Hu, H., Hu, H. B., Huang, J., ... Zhou, X. X. (2005). New flux upper limits of diffuse TeV gamma rays from the galactic plane observed with the tibet air shower array. In 29th International Cosmic Ray Conference, ICRC 2005 (Vol. 4, pp. 43-46). Tata Institute of Fundamental Research.

New flux upper limits of diffuse TeV gamma rays from the galactic plane observed with the tibet air shower array. / Amenomori, M.; Ayabe, S.; Chen, D.; Cui, S. W.; Danzengluobu; Ding, L. K.; Ding, X. H.; Feng, C. F.; Feng, Z. Y.; Gao, X. Y.; Geng, Q. X.; Guo, H. W.; He, H. H.; He, M.; Hibino, K.; Hotta, N.; Hu, Haibing; Hu, H. B.; Huang, J.; Huang, Q.; Jia, H. Y.; Kajino, F.; Kasahara, K.; Katayose, Y.; Kato, C.; Kawata, K.; Labaciren; Le, G. M.; Li, J. Y.; Lu, H.; Lu, S. L.; Meng, X. R.; Mizutani, K.; Mu, J.; Munakata, K.; Nagai, A.; Nanjo, H.; Nishizawa, M.; Ohnishi, M.; Ohta, I.; Onuma, H.; Ouchi, T.; Ozawa, Shunsuke; Ren, J. R.; Saito, T.; Sakata, M.; Sasaki, T.; Shibata, M.; Shiomi, A.; Shirai, T.; Sugimoto, H.; Takita, M.; Tan, Y. H.; Tateyama, N.; Torii, Shoji; Tsuchiya, H.; Udo, S.; Wang, H.; Wang, X.; Wang, Y. G.; Wu, H. R.; Xue, L.; Yamamoto, Y.; Yan, C. T.; Yang, X. C.; Yasue, S.; Ye, Z. H.; Yu, G. C.; Yuan, A. F.; Yuda, T.; Zhang, H. M.; Zhang, J. L.; Zhang, N. J.; Zhang, X. Y.; Zhang, Y.; Zhang, Y.; Zhaxisangzhu; Zhou, X. X.

29th International Cosmic Ray Conference, ICRC 2005. Vol. 4 Tata Institute of Fundamental Research, 2005. p. 43-46.

研究成果: Conference contribution

Amenomori, M, Ayabe, S, Chen, D, Cui, SW, Danzengluobu, Ding, LK, Ding, XH, Feng, CF, Feng, ZY, Gao, XY, Geng, QX, Guo, HW, He, HH, He, M, Hibino, K, Hotta, N, Hu, H, Hu, HB, Huang, J, Huang, Q, Jia, HY, Kajino, F, Kasahara, K, Katayose, Y, Kato, C, Kawata, K, Labaciren, Le, GM, Li, JY, Lu, H, Lu, SL, Meng, XR, Mizutani, K, Mu, J, Munakata, K, Nagai, A, Nanjo, H, Nishizawa, M, Ohnishi, M, Ohta, I, Onuma, H, Ouchi, T, Ozawa, S, Ren, JR, Saito, T, Sakata, M, Sasaki, T, Shibata, M, Shiomi, A, Shirai, T, Sugimoto, H, Takita, M, Tan, YH, Tateyama, N, Torii, S, Tsuchiya, H, Udo, S, Wang, H, Wang, X, Wang, YG, Wu, HR, Xue, L, Yamamoto, Y, Yan, CT, Yang, XC, Yasue, S, Ye, ZH, Yu, GC, Yuan, AF, Yuda, T, Zhang, HM, Zhang, JL, Zhang, NJ, Zhang, XY, Zhang, Y, Zhang, Y, Zhaxisangzhu & Zhou, XX 2005, New flux upper limits of diffuse TeV gamma rays from the galactic plane observed with the tibet air shower array. in 29th International Cosmic Ray Conference, ICRC 2005. vol. 4, Tata Institute of Fundamental Research, pp. 43-46, 29th International Cosmic Ray Conference, ICRC 2005, Pune, 05/8/3.

Amenomori, M. ; Ayabe, S. ; Chen, D. ; Cui, S. W. ; Danzengluobu ; Ding, L. K. ; Ding, X. H. ; Feng, C. F. ; Feng, Z. Y. ; Gao, X. Y. ; Geng, Q. X. ; Guo, H. W. ; He, H. H. ; He, M. ; Hibino, K. ; Hotta, N. ; Hu, Haibing ; Hu, H. B. ; Huang, J. ; Huang, Q. ; Jia, H. Y. ; Kajino, F. ; Kasahara, K. ; Katayose, Y. ; Kato, C. ; Kawata, K. ; Labaciren ; Le, G. M. ; Li, J. Y. ; Lu, H. ; Lu, S. L. ; Meng, X. R. ; Mizutani, K. ; Mu, J. ; Munakata, K. ; Nagai, A. ; Nanjo, H. ; Nishizawa, M. ; Ohnishi, M. ; Ohta, I. ; Onuma, H. ; Ouchi, T. ; Ozawa, Shunsuke ; Ren, J. R. ; Saito, T. ; Sakata, M. ; Sasaki, T. ; Shibata, M. ; Shiomi, A. ; Shirai, T. ; Sugimoto, H. ; Takita, M. ; Tan, Y. H. ; Tateyama, N. ; Torii, Shoji ; Tsuchiya, H. ; Udo, S. ; Wang, H. ; Wang, X. ; Wang, Y. G. ; Wu, H. R. ; Xue, L. ; Yamamoto, Y. ; Yan, C. T. ; Yang, X. C. ; Yasue, S. ; Ye, Z. H. ; Yu, G. C. ; Yuan, A. F. ; Yuda, T. ; Zhang, H. M. ; Zhang, J. L. ; Zhang, N. J. ; Zhang, X. Y. ; Zhang, Y. ; Zhang, Y. ; Zhaxisangzhu ; Zhou, X. X. / New flux upper limits of diffuse TeV gamma rays from the galactic plane observed with the tibet air shower array. 29th International Cosmic Ray Conference, ICRC 2005. Vol. 4 Tata Institute of Fundamental Research, 2005. pp. 43-46

@inproceedings{6da8c10981524dea983334e43ddc9b33,

title = "New flux upper limits of diffuse TeV gamma rays from the galactic plane observed with the tibet air shower array",

abstract = "The flux upper limits of the diffuse gamma rays, from the inner and outer Galactic planes, are found to be decreased by factors of 4.0∼3.6 for 3∼10 TeV, respectively, by using the simulation results of effective area ratios for gamma-ray and cosmic-ray induced showers in the Tibet air shower array. In our previous work, the flux upper limits were deduced only from the flux ratio of air showers generated by gamma rays versus cosmic rays. As a result the source electron spectral index for inverse Compton should be steeper than 2.2 and 2.1 for the inner and outer Galactic planes, respectively.",

author = "M. Amenomori and S. Ayabe and D. Chen and Cui, {S. W.} and Danzengluobu and Ding, {L. K.} and Ding, {X. H.} and Feng, {C. F.} and Feng, {Z. Y.} and Gao, {X. Y.} and Geng, {Q. X.} and Guo, {H. W.} and He, {H. H.} and M. He and K. Hibino and N. Hotta and Haibing Hu and Hu, {H. B.} and J. Huang and Q. Huang and Jia, {H. Y.} and F. Kajino and K. Kasahara and Y. Katayose and C. Kato and K. Kawata and Labaciren and Le, {G. M.} and Li, {J. Y.} and H. Lu and Lu, {S. L.} and Meng, {X. R.} and K. Mizutani and J. Mu and K. Munakata and A. Nagai and H. Nanjo and M. Nishizawa and M. Ohnishi and I. Ohta and H. Onuma and T. Ouchi and Shunsuke Ozawa and Ren, {J. R.} and T. Saito and M. Sakata and T. Sasaki and M. Shibata and A. Shiomi and T. Shirai and H. Sugimoto and M. Takita and Tan, {Y. H.} and N. Tateyama and Shoji Torii and H. Tsuchiya and S. Udo and H. Wang and X. Wang and Wang, {Y. G.} and Wu, {H. R.} and L. Xue and Y. Yamamoto and Yan, {C. T.} and Yang, {X. C.} and S. Yasue and Ye, {Z. H.} and Yu, {G. C.} and Yuan, {A. F.} and T. Yuda and Zhang, {H. M.} and Zhang, {J. L.} and Zhang, {N. J.} and Zhang, {X. Y.} and Y. Zhang and Y. Zhang and Zhaxisangzhu and Zhou, {X. X.}",

year = "2005",

language = "English",

volume = "4",

pages = "43--46",

booktitle = "29th International Cosmic Ray Conference, ICRC 2005",

publisher = "Tata Institute of Fundamental Research",

note = "29th International Cosmic Ray Conference, ICRC 2005 ; Conference date: 03-08-2005 Through 10-08-2005",

}

TY - GEN

T1 - New flux upper limits of diffuse TeV gamma rays from the galactic plane observed with the tibet air shower array

AU - Amenomori, M.

AU - Ayabe, S.

AU - Chen, D.

AU - Cui, S. W.

AU - Danzengluobu,

AU - Ding, L. K.

AU - Ding, X. H.

AU - Feng, C. F.

AU - Feng, Z. Y.

AU - Gao, X. Y.

AU - Geng, Q. X.

AU - Guo, H. W.

AU - He, H. H.

AU - He, M.

AU - Hibino, K.

AU - Hotta, N.

AU - Hu, Haibing

AU - Hu, H. B.

AU - Huang, J.

AU - Huang, Q.

AU - Jia, H. Y.

AU - Kajino, F.

AU - Kasahara, K.

AU - Katayose, Y.

AU - Kato, C.

AU - Kawata, K.

AU - Labaciren,

AU - Le, G. M.

AU - Li, J. Y.

AU - Lu, H.

AU - Lu, S. L.

AU - Meng, X. R.

AU - Mizutani, K.

AU - Mu, J.

AU - Munakata, K.

AU - Nagai, A.

AU - Nanjo, H.

AU - Nishizawa, M.

AU - Ohnishi, M.

AU - Ohta, I.

AU - Onuma, H.

AU - Ouchi, T.

AU - Ozawa, Shunsuke

AU - Ren, J. R.

AU - Saito, T.

AU - Sakata, M.

AU - Sasaki, T.

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 - Wang, X.

AU - Wang, Y. G.

AU - Wu, H. R.

AU - Xue, L.

AU - Yamamoto, Y.

AU - Yan, C. T.

AU - Yang, X. C.

AU - Yasue, S.

AU - Ye, Z. H.

AU - Yu, G. C.

AU - Yuan, A. F.

AU - Yuda, T.

AU - Zhang, H. M.

AU - Zhang, J. L.

AU - Zhang, N. J.

AU - Zhang, X. Y.

AU - Zhang, Y.

AU - Zhaxisangzhu,

AU - Zhou, X. X.

PY - 2005

Y1 - 2005

N2 - The flux upper limits of the diffuse gamma rays, from the inner and outer Galactic planes, are found to be decreased by factors of 4.0∼3.6 for 3∼10 TeV, respectively, by using the simulation results of effective area ratios for gamma-ray and cosmic-ray induced showers in the Tibet air shower array. In our previous work, the flux upper limits were deduced only from the flux ratio of air showers generated by gamma rays versus cosmic rays. As a result the source electron spectral index for inverse Compton should be steeper than 2.2 and 2.1 for the inner and outer Galactic planes, respectively.

AB - The flux upper limits of the diffuse gamma rays, from the inner and outer Galactic planes, are found to be decreased by factors of 4.0∼3.6 for 3∼10 TeV, respectively, by using the simulation results of effective area ratios for gamma-ray and cosmic-ray induced showers in the Tibet air shower array. In our previous work, the flux upper limits were deduced only from the flux ratio of air showers generated by gamma rays versus cosmic rays. As a result the source electron spectral index for inverse Compton should be steeper than 2.2 and 2.1 for the inner and outer Galactic planes, respectively.

UR - http://www.scopus.com/inward/record.url?scp=84898990618&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84898990618&partnerID=8YFLogxK

M3 - Conference contribution

AN - SCOPUS:84898990618

VL - 4

SP - 43

EP - 46

BT - 29th International Cosmic Ray Conference, ICRC 2005

PB - Tata Institute of Fundamental Research

T2 - 29th International Cosmic Ray Conference, ICRC 2005

Y2 - 3 August 2005 through 10 August 2005

ER -

New flux upper limits of diffuse TeV gamma rays from the galactic plane observed with the tibet air shower array

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ASJC Scopus subject areas

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