Multiwavelength searches of the Shell-like SNR G40.5-0.5

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. I. Zhang, Zhaxisangzhu, X. X. Zhou

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

    2 Citations (Scopus)

    Abstract

    Using observation data of the extended Tibet air shower array from October 2000 to September 2001, a region around the shell-like SNR G40.5-0.5 direction with the highest excess of 4.4 sigma was found using two dimension analysis method. In this article we presented some work done to understanding the nature of the G40.5-0.5 using a multiwavelength approach. In order to look for a site of the CR accelerators, a survey of the CO(J=1-0) line to G40.5-0.5 region will be conducting with the 13.7m radio telescope at Delingha, the millimeter-wave radio observatory of Purple Mountain Observatory this year.

    Original languageEnglish
    Title of host publication29th International Cosmic Ray Conference, ICRC 2005
    PublisherTata Institute of Fundamental Research
    Pages93-96
    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

    observatories
    Tibet
    radio telescopes
    cosmic ray showers
    mountains
    millimeter waves
    accelerators
    conduction

    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). Multiwavelength searches of the Shell-like SNR G40.5-0.5. In 29th International Cosmic Ray Conference, ICRC 2005 (Vol. 4, pp. 93-96). Tata Institute of Fundamental Research.

    Multiwavelength searches of the Shell-like SNR G40.5-0.5. / 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. I.; Zhaxisangzhu; Zhou, X. X.

    29th International Cosmic Ray Conference, ICRC 2005. Vol. 4 Tata Institute of Fundamental Research, 2005. p. 93-96.

    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, YI, Zhaxisangzhu & Zhou, XX 2005, Multiwavelength searches of the Shell-like SNR G40.5-0.5. in 29th International Cosmic Ray Conference, ICRC 2005. vol. 4, Tata Institute of Fundamental Research, pp. 93-96, 29th International Cosmic Ray Conference, ICRC 2005, Pune, 05/8/3.
    Amenomori M, Ayabe S, Chen D, Cui SW, Danzengluobu, Ding LK et al. Multiwavelength searches of the Shell-like SNR G40.5-0.5. In 29th International Cosmic Ray Conference, ICRC 2005. Vol. 4. Tata Institute of Fundamental Research. 2005. p. 93-96
    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. I. ; Zhaxisangzhu ; Zhou, X. X. / Multiwavelength searches of the Shell-like SNR G40.5-0.5. 29th International Cosmic Ray Conference, ICRC 2005. Vol. 4 Tata Institute of Fundamental Research, 2005. pp. 93-96
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    title = "Multiwavelength searches of the Shell-like SNR G40.5-0.5",
    abstract = "Using observation data of the extended Tibet air shower array from October 2000 to September 2001, a region around the shell-like SNR G40.5-0.5 direction with the highest excess of 4.4 sigma was found using two dimension analysis method. In this article we presented some work done to understanding the nature of the G40.5-0.5 using a multiwavelength approach. In order to look for a site of the CR accelerators, a survey of the CO(J=1-0) line to G40.5-0.5 region will be conducting with the 13.7m radio telescope at Delingha, the millimeter-wave radio observatory of Purple Mountain Observatory this year.",
    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 Zhang, {Y. I.} and Zhaxisangzhu and Zhou, {X. X.}",
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    TY - GEN

    T1 - Multiwavelength searches of the Shell-like SNR G40.5-0.5

    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. I.

    AU - Zhaxisangzhu,

    AU - Zhou, X. X.

    PY - 2005

    Y1 - 2005

    N2 - Using observation data of the extended Tibet air shower array from October 2000 to September 2001, a region around the shell-like SNR G40.5-0.5 direction with the highest excess of 4.4 sigma was found using two dimension analysis method. In this article we presented some work done to understanding the nature of the G40.5-0.5 using a multiwavelength approach. In order to look for a site of the CR accelerators, a survey of the CO(J=1-0) line to G40.5-0.5 region will be conducting with the 13.7m radio telescope at Delingha, the millimeter-wave radio observatory of Purple Mountain Observatory this year.

    AB - Using observation data of the extended Tibet air shower array from October 2000 to September 2001, a region around the shell-like SNR G40.5-0.5 direction with the highest excess of 4.4 sigma was found using two dimension analysis method. In this article we presented some work done to understanding the nature of the G40.5-0.5 using a multiwavelength approach. In order to look for a site of the CR accelerators, a survey of the CO(J=1-0) line to G40.5-0.5 region will be conducting with the 13.7m radio telescope at Delingha, the millimeter-wave radio observatory of Purple Mountain Observatory this year.

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    UR - http://www.scopus.com/inward/citedby.url?scp=84899026470&partnerID=8YFLogxK

    M3 - Conference contribution

    VL - 4

    SP - 93

    EP - 96

    BT - 29th International Cosmic Ray Conference, ICRC 2005

    PB - Tata Institute of Fundamental Research

    ER -