Search Results - "Yan, C.T"

IgH class switching and translocations use a robust non-classical end-joining pathway by Yan, C.T

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Anisotropy and Corotation of Galactic Cosmic Rays by Amenomori, M, Ayabe, S, Bi, X.J, Chen, D, Cui, S.W, Danzengluobu, Ding, L.K, Ding, X.H, Feng, C.F, Feng, Zhaoyang, 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, A.F, Li, J.Y, Lou, Y.-Q, 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, S, Ren, J.R, Saito, T, Saito, T.Y, Sakata, M, Sako, T.K, Sasaki, T, Shibata, M, Shiomi, A, Shirai, T, Sugimoto, H, Takita, M, Tan, Y.H, Tateyama, N, Torii, S, Tsuchiya, H, Udo, S, Wang, B, 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, Yi, Zhaxisangzhu, Zhou, X.X

“…The intensity of Galactic cosmic rays is nearly isotropic because of the influence of magnetic fields in the Milky Way. Here, we present two-dimensional…”
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Are protons still dominant at the knee of the cosmic-ray energy spectrum? by 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, S., 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, S., 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, Yi, Zhaxisangzhu, Zhou, X.X.

“…A hybrid experiment consisting of emulsion chambers, burst detectors and the Tibet-II air-shower array was carried out at Yangbajing (4300 m a.s.l., 606 g/cm2)…”
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Moon shadow by cosmic rays under the influence of geomagnetic field and search for antiprotons at multi-TeV energies by Amenomori, M., Ayabe, S., Bi, X.J., Chen, D., Cui, S.W., Danzengluobu, Ding, L.K., Ding, X.H., Feng, C.F., Feng, Zhaoyang, 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, A.F., Li, J.Y., Lou, Y.-Q., 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, S., Ren, J.R., Saito, T., Saito, T.Y., Sakata, M., Sako, T.K., Sasaki, T., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y.H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, B.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, Yi, Zhaxisangzhu, Zhou, X.X.

“…We have observed the shadowing of galactic cosmic ray flux in the direction of the moon, the so-called moon shadow, using the Tibet-III air shower array…”
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Flux upper limits of diffuse TeV gamma rays from the Galactic plane using the effective area of the Tibet-II and -III arrays by Amenomori, M., Ayabe, S., 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., Izumi, M., 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, S., 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, S., Tsuchiya, H., Udo, S., Utsugi, T., Wang, B.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., Zhaxisangzhu, Zhou, X.X.

“…We obtained new upper limits on the diffuse gamma rays from the inner Galactic (IG) and outer Galactic (OG) planes in 3–10 TeV region, using the Tibet air…”
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Variation of Sun shadow in the Solar Cycle 23 observed with the Tibet air shower array by Amenomori, M., Ayabe, S., 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., Izumi, M., 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, S., 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, S., Tsuchiya, H., Udo, S., Utsugi, T., Wang, B.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., Zhaxisangzhu, Zhou, X.X.

“…According to many solar observations, the solar activity, during the Solar Cycle 23, is gradually declining to the quiet phase from the high state in…”
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The cosmic-ray energy spectrum around the knee measured by the Tibet-III air-shower array by Amenomori, M., Ayabe, S., Bi, X.J., Chen, D., Cui, S.W., Danzengluobu, Ding, L.K., Ding, X.H., Feng, C.F., Feng, Zhaoyang, 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, A.F., Li, J.Y., Lou, Y.-Q., 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, S., Ren, J.R., Saito, T., Saito, T.Y., Sakata, M., Sako, T.K., Sasaki, T., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y.H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, B., 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, Yi, Zhaxisangzhu, Zhou, X.X.

“…We present an updated all-particle energy spectrum using data collected in the period from 2000 November through 2004 October by Tibet III air-shower array…”
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Northern Sky Survey for Gamma-ray Point Sources in 100 TeV Region with the Tibet Air Shower Array by Amenomori, M., Ayabe, S., Bi, X.J., Chen, D., Cui, S.W., Danzengluobu, Ding, L.K., Ding, X.H., Feng, C.F., Feng, Zhaoyang, 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, A.F., Li, J.Y., Lou, Y.-Q., 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, S., Ren, J.R., Saito, T., Saito, T.Y., Sakata, M., Sasaki, T., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y.H., Tateyama, N., Sako, T.K., Torii, S., Tsuchiya, H., Udo, S., Wang, B., 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, Yi, Zhaxisangzhu, Zhou, X.X.

“…We searched for steady 100 TeV gamma-ray point sources from −10° to +70° in declination based on six year data obtained from Nov. 1999 to Nov. 2005 by the…”
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Spectral index of high-energy cosmic rays by the Compton-Getting effect at solar time frame with the Tibet air shower array by Amenomori, M., Ayabe, S., Bi, X.J., Chen, D., Cui, S.W., Danzengluobu, Ding, L.K., Ding, X.H., Feng, C.F., Feng, Zhaoyang, 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, A.F., Li, J.Y., Lou, Y.-Q., 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, S., Ren, J.R., Saito, T., Saito, T.Y., Sakata, M., Sasaki, T., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y.H., Tateyama, N., Sako, T.K., Torii, S., Tsuchiya, H., Udo, S., Wang, B., 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, Yi, Zhaxisangzhu, Zhou, X.X.

“…We report on the spectral index of cosmic rays around 10 TeV energy region obtained by observation of the Compton-Getting anisotropy due to the terrestrial…”
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A large underground water Cherenkov muon detector array with the Tibet air shower array for the Gamma-ray astronomy in the 100 TeV region: Overview and physics goal by Amenomori, M., Ayabe, S., Bi, X.J., Chen, D., Cui, S.W., Danzengluobu, Ding, L.K., Ding, X.H., Feng, C.F., Feng, Zhaoyang, 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, A.F., Li, J.Y., Lou, Y.-Q., 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, S., Ren, J.R., Saito, T., Saito, T.Y., Sakata, M., Sasaki, T., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y.H., Tateyama, N., Sako, T.K., Torii, S., Tsuchiya, H., Udo, S., Wang, B., 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, Yi, Zhaxisangzhu, Zhou, X.X.

“…The Tibet air shower array with effective area 37,000 m 2 located at 4300m in altitude, in Tibet, China, is sensitive to celestial gamma rays with energies…”
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A large underground water Cherenkov muon detector array with the Tibet air shower array for Gamma-ray astronomy in the 100 TeV region: detector design and simulation by Amenomori, M., Ayabe, S., Bi, X.J., Chen, D., Cui, S.W., Danzengluobu, Ding, L.K., Ding, X.H., Feng, C.F., Feng, Zhaoyang, 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, A.F., Li, J.Y., Lou, Y.-Q., 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, S., Ren, J.R., Saito, T., Saito, T.Y., Sakata, M., Sasaki, T., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y.H., Tateyama, N., Sako, T.K., Torii, S., Tsuchiya, H., Udo, S., Wang, B., 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, Yi, Zhaxisangzhu, Zhou, X.X.

“…We are planning to build a large water-Cherenkov-type muon detector array around the Tibet air shower array for Gamma-ray astronomy in the 100 TeV Region. In…”
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