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 & 58 others 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

    Research output: Chapter in Book/Report/Conference proceedingConference contribution

    2 Citations (Scopus)

    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.

    Original languageEnglish
    Title of host publication29th International Cosmic Ray Conference, ICRC 2005
    PublisherTata Institute of Fundamental Research
    Pages43-46
    Number of pages4
    Volume4
    Publication statusPublished - 2005
    Event29th International Cosmic Ray Conference, ICRC 2005 - Pune
    Duration: 2005 Aug 32005 Aug 10

    Other

    Other29th International Cosmic Ray Conference, ICRC 2005
    CityPune
    Period05/8/305/8/10

    Fingerprint

    Tibet
    cosmic ray showers
    gamma rays
    cosmic rays
    electron sources
    showers
    simulation

    ASJC Scopus subject areas

    • Nuclear and High Energy Physics

    Cite this

    Amenomori, M., Ayabe, S., Chen, D., Cui, S. W., Danzengluobu, Ding, L. K., ... 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.

    Research output: Chapter in Book/Report/Conference proceedingConference 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 SW, Danzengluobu, Ding LK et al. 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. 2005. p. 43-46
    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",

    }

    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 - 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

    VL - 4

    SP - 43

    EP - 46

    BT - 29th International Cosmic Ray Conference, ICRC 2005

    PB - Tata Institute of Fundamental Research

    ER -