Search Results - "Wu, H. R."

First Detection of sub-PeV Diffuse Gamma Rays from the Galactic Disk: Evidence for Ubiquitous Galactic Cosmic Rays beyond PeV Energies by Amenomori, M, Bao, Y W, Bi, X J, Chen, D, Chen, T L, Chen, W Y, Chen, Xu, Chen, Y, Cirennima, Cui, S W, Danzengluobu, Ding, L K, Fang, J H, Fang, K, Feng, C F, Feng, Zhaoyang, Feng, Z Y, Gao, Qi, Gou, Q B, Guo, Y Q, Guo, Y Y, He, H H, He, Z T, Hibino, K, Hotta, N, Hu, Haibing, Hu, H B, Huang, J, Jia, H Y, Jiang, L, Jin, H B, Kasahara, K, Katayose, Y, Kato, C, Kato, S, Kawata, K, Kihara, W, Ko, Y, Kozai, M, Labaciren, Le, G M, Li, A F, Li, H J, Li, W J, Lin, Y H, Liu, B, Liu, C, Liu, J S, Liu, M Y, Liu, W, Lou, Y-Q, Lu, H, Meng, X R, Munakata, K, Nakada, H, Nakamura, Y, Nanjo, H, Nishizawa, M, Ohnishi, M, Ohura, T, Ozawa, S, Qian, X L, Qu, X B, Saito, T, Sakata, M, Sako, T K, Shao, J, Shibata, M, Shiomi, A, Sugimoto, H, Takano, W, Takita, M, Tan, Y H, Tateyama, N, Torii, S, Tsuchiya, H, Udo, S, Wang, H, Wu, H R, Xue, L, Yamamoto, Y, Yang, Z, Yokoe, Y, Yuan, A F, Zhai, L M, Zhang, H M, Zhang, J L, Zhang, X, Zhang, X Y, Zhang, Y, Zhang, Yi, Zhang, Ying, Zhao, S P, Zhaxisangzhu, Zhou, X X

“…We report, for the first time, the long-awaited detection of diffuse gamma rays with energies between 100 TeV and 1 PeV in the Galactic disk. Particularly, all…”
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First Detection of Photons with Energy beyond 100 TeV from an Astrophysical Source by Amenomori, M, Bao, Y W, Bi, X J, Chen, D, Chen, T L, Chen, W Y, Chen, Xu, Chen, Y, Cirennima, Cui, S W, Danzengluobu, Ding, L K, Fang, J H, Fang, K, Feng, C F, Feng, Zhaoyang, Feng, Z Y, Gao, Qi, 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, Jin, H B, Kajino, F, Kasahara, K, Katayose, Y, Kato, C, Kato, S, Kawata, K, Kozai, M, Labaciren, Le, G M, Li, A F, Li, H J, Li, W J, Lin, Y H, Liu, B, Liu, C, Liu, J S, Liu, M Y, Lou, Y-Q, Lu, H, Meng, X R, Mitsui, H, Munakata, K, Nakamura, Y, Nanjo, H, Nishizawa, M, Ohnishi, M, Ohta, I, Ozawa, S, Qian, X L, Qu, X B, Saito, T, Sakata, M, Sako, T K, Sengoku, Y, Shao, J, Shibata, M, Shiomi, A, Sugimoto, H, Takita, M, Tan, Y H, Tateyama, N, Torii, S, Tsuchiya, H, Udo, S, Wang, H, Wu, H R, Xue, L, Yagisawa, K, Yamamoto, Y, Yang, Z, Yuan, A F, Zhai, L M, Zhang, H M, Zhang, J L, Zhang, X, Zhang, X Y, Zhang, Y, Zhang, Yi, Zhang, Ying, Zhaxisangzhu, Zhou, X X

“…We report on the highest energy photons from the Crab Nebula observed by the Tibet air shower array with the underground water-Cherenkov-type muon detector…”
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Knee of the cosmic hydrogen and helium spectrum below 1 PeV measured by ARGO-YBJ and a Cherenkov telescope of LHAASO by Bartoli, B., Bernardini, P., Bi, X. J., Cao, Z., Catalanotti, S., Chen, S. Z., Chen, T. L., Cui, S. W., Dai, B. Z, D’Amone, A., Danzengluobu, De Mitri, I., D’Ettorre Piazzoli, B., Di Girolamo, T., Di Sciascio, G., Feng, C. F., Feng, Zhaoyang, Feng, Zhenyong, Guo, Q. B., Guo, Y. Q., He, H. H., Hu, Haibing, Hu, Hongbo, Iacovacci, M., Iuppa, R., Jia, H. Y., Labaciren, Li, H. J., Liu, C., Liu, J., Liu, M. Y., Lu, H., Ma, L. L., Ma, X. H., Mancarella, G., Mari, S. M., Marsella, G., Mastroianni, S., Montini, P., Ning, C. C., Perrone, L., Pistilli, P., Salvini, P., Santonico, R., Shen, P. R., Sheng, X. D., Shi, F., Surdo, A., Tan, Y. H., Vallania, P., Vernetto, S., Vigorito, C., Wang, H., Wu, C. Y., Wu, H. R., Xue, L., Yang, Q. Y., Yang, X. C., Yao, Z. G., Yuan, A. F., Zha, M., Zhang, H. M., Zhang, L., Zhang, X. Y., Zhang, Y., Zhao, J., Zhaxiciren, Zhaxisangzhu, Zhou, X. X., Zhu, F. R., Zhu, Q. Q., Bai, Y. X., Chen, M. J., Feng, S. H., Gao, B., Gu, M. H., Hou, C., Liu, J. L., Wang, X., Xiao, G., Zhang, B. K., Zhang, S. S., Zhou, B., Zuo, X.

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Gamma-Ray Observation of the Cygnus Region in the 100-TeV Energy Region by Amenomori, M., Bao, Y. W., Bi, X. J., Chen, D., Chen, T. L., Chen, W. Y., Chen, Xu, Chen, Y., Cirennima, Cui, S. W., Danzengluobu, Ding, L. K., Fang, J. H., Fang, K., Feng, C. F., Feng, Zhaoyang, Feng, Z. Y., Gao, Qi, Gomi, A., Gou, Q. B., Guo, Y. Q., Guo, Y. Y., He, H. H., He, Z. T., Hibino, K., Hotta, N., Hu, Haibing, Hu, H. B., Huang, J., Jia, H. Y., Jiang, L., Jiang, P., Jin, H. B., Kasahara, K., Katayose, Y., Kato, C., Kato, S., Kawata, K., Kozai, M., Kurashige, D., Labaciren, Le, G. M., Li, A. F., Li, H. J., Li, W. J., Li, Y., Lin, Y. H., Liu, B., Liu, C., Liu, J. S., Liu, L. Y., Liu, M. Y., Liu, W., Liu, X. L., Lou, Y.-Q., Lu, H., Meng, X. R., Munakata, K., Nakada, H., Nakamura, Y., Nakazawa, Y., Nanjo, H., Ning, C. C., Nishizawa, M., Ohnishi, M., Ohura, T., Okukawa, S., Ozawa, S., Qian, L., Qian, X., Qian, X. L., Qu, X. B., Saito, T., Sakata, M., Sako, T., Sako, T. K., Shao, J., Shibata, M., Shiomi, A., Sugimoto, H., Takano, W., Takita, M., Tan, Y. H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, H., Wang, Y. P., Wangdui, Wu, H. R., Wu, Q., Xu, J. L., Xue, L., Yamamoto, Y., Yang, Z., Yao, Y. Q., Yin, J., Yokoe, Y., Yu, N. P.

“…We report observations of gamma-ray emissions with energies in the 100-TeV energy region from the Cygnus region in our Galaxy. Two sources are significantly…”
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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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Observation of Gamma Rays up to 320 TeV from the Middle-aged TeV Pulsar Wind Nebula HESS J1849−000 by Amenomori, M., Asano, S., Bao, Y. W., Bi, X. J., Chen, T. L., Chen, W. Y., Chen, Xu, Chen, Y., Cirennima, Cui, S. W., Danzengluobu, Ding, L. K., Fang, K., Feng, C. F., Feng, Zhaoyang, Feng, Z. Y., Gao, Qi, Gomi, A., Gou, Q. B., Guo, Y. Q., Hayashi, Y., He, Z. T., Hibino, K., Hotta, N., Hu, Haibing, Hu, H. B., Hu, K. Y., Huang, J., Jia, H. Y., Jiang, L., Jiang, P., Kasahara, K., Katayose, Y., Kato, C., Kato, S., Kawahara, I., Kawashima, T., Kawata, K., Kozai, M., Le, G. M., Li, H. J., Li, W. J., Li, Y., Lin, Y. H., Liu, B., Liu, C., Liu, J. S., Liu, L. Y., Liu, M. Y., Liu, W., Lu, H., Meng, X. R., Meng, Y., Nagaya, K., Nakamura, Y., Nakazawa, Y., Ning, C. C., Nishizawa, M., Noguchi, R., Ohnishi, M., Okukawa, S., Ozawa, S., Qian, X., Qian, X. L., Qu, X. B., Sakata, M., Sako, T., Sako, T. K., Sasaki, T., Shao, J., Shibata, M., Sugimoto, H., Tan, Y. H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, H., Wang, S. F., Wang, Y. P., Wangdui, Wu, H. R., Wu, Q., Xu, J. L., Xue, L., Yang, Z., Yao, Y. Q., Yin, J., Yokoe, Y., Yu, Y. L., Yuan, A. F., Zhai, L. M., Zhang, H. M., Zhang, J. L., Zhang, X., Zhang, X. Y., Zhang, Yi, Zhang, Ying, Zhaxisangzhu, Zou, Y. H.

“…Abstract Gamma rays from HESS J1849−000, a middle-aged TeV pulsar wind nebula (PWN), are observed by the Tibet air shower array and the muon detector array…”
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Measurement of the Gamma-Ray Energy Spectrum beyond 100 TeV from the HESS J1843–033 Region by Amenomori, M., Asano, S., Bao, Y. W., Bi, X. J., Chen, D., Chen, T. L., Chen, W. Y., Chen, Y., Cirennima, Cui, S. W., Danzengluobu, Fang, K., Feng, C. F., Feng, Zhaoyang, Gao, Qi, Gomi, A., Gou, Q. B., Guo, Y. Q., Guo, Y. Y., He, H. H., Hibino, K., Hotta, N., Hu, Haibing, Hu, H. B., Hu, K. Y., Huang, J., Jia, H. Y., Jiang, L., Jiang, P., Jin, H. B., Kasahara, K., Katayose, Y., Kato, S., Kawashima, T., Kawata, K., Kozai, M., Kurashige, D., Labaciren, Li, A. F., Li, H. J., Li, W. J., Li, Y., Lin, Y. H., Liu, B., Liu, C., Liu, L. Y., Liu, M. Y., Liu, W., Liu, X. L., Lou, Y.-Q., Lu, H., Meng, X. R., Meng, Y., Nagaya, K., Nakamura, Y., Nakazawa, Y., Ning, C. C., Nishizawa, M., Ohnishi, M., Okukawa, S., Ozawa, S., Qian, X., Qian, X. L., Qu, X. B., Sakakibara, Y., Sakata, M., Sako, T., Sako, T. K., Shao, J., Shiomi, A., Sugimoto, H., Takano, W., Takita, M., Tan, Y. H., Tateyama, N., Torii, S., Udo, S., Wang, H., Wang, Y. P., Wangdui, Wu, H. R., Wu, Q., Xu, J. L., Xue, L., Yang, Z., Yao, Y. Q., Yin, J., Yokoe, Y., Yu, N. P., Yuan, A. F., Zhai, L. M., Zhang, C. P., Zhang, H. M., Zhang, J. L., Zhang, X. Y., Zhang, Y., Zhang, Yi, Zhang, Ying, Zhaxisangzhu, Zhou, X. X.

“…Abstract HESS J1843–033 is a very high energy gamma-ray source whose origin remains unidentified. This work presents, for the first time, the energy spectrum…”
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Evaluation of the Interplanetary Magnetic Field Strength Using the Cosmic-Ray Shadow of the Sun by 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, S, 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, S, Tsuchiya, H, Udo, S, Wang, H, Wu, H R, Xue, L, Yamamoto, Y, Yamauchi, K, Yang, Z, 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

“…We analyze the Sun's shadow observed with the Tibet-III air shower array and find that the shadow's center deviates northward (southward) from the optical…”
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Probe of the solar magnetic field using the "cosmic-ray shadow" of the sun by 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, Hakamada, K, 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, 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, Mizutani, K, Munakata, K, Nanjo, H, Nishizawa, M, Ohnishi, M, Ohta, I, Onuma, H, Ozawa, S, 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, S, Tsuchiya, H, Udo, S, Wang, H, Wu, H R, Xue, L, Yamamoto, Y, 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

“…We report on a clear solar-cycle variation of the Sun’s shadow in the 10 TeV cosmic-ray flux observed by the Tibet air shower array during a full solar cycle…”
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Influence of Earth-directed Coronal Mass Ejections on the Sun's Shadow Observed by the Tibet-III Air Shower Array by 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., Munakata, K., Nakajima, T., Nakamura, Y., Nanjo, H., Nishizawa, M., Niwa, T., Ohnishi, M., Ohta, I., Ozawa, S., 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, S., Tsuchiya, H., Udo, S., Wang, H., Wu, H. R., Xue, L., Yamamoto, Y., Yamauchi, K., Yang, Z., Yuan, A. F., Zhai, L. M., Zhang, H. M., Zhang, J. L., Zhang, X. Y., Zhang, Y., Zhang, Yi, Zhang, Ying, Zhaxisangzhu, Zhou, X. X.

“…We examine the possible influence of Earth-directed coronal mass ejections (ECMEs) on the Sun's shadow in the 3 TeV cosmic-ray intensity observed by the…”
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Serum miR-133 as a novel biomarker for predicting treatment response and survival in acute myeloid leukemia by Zheng, Z-Z, Ma, Y-P, Wu, R-H, Rong, G, Li, C, Li, G-X, Ren, F-G, Xu, L-J

“…MiRNA-133 (miR-133) has been identified as a tumor suppressor in many types of human cancers. However, its clinical significance in acute myeloid leukemia…”
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Multi-TeV Gamma-Ray Observation from the Crab Nebula Using the Tibet-III Air Shower Array Finely Tuned by the Cosmic Ray Moon's Shadow by Amenomori, M, Bi, X. J, Chen, D, Cui, S. W, Danzengluobu, Ding, L. K, Ding, X. H, Fan, C, 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, 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, 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-III air shower array, consisting of 533 scintillation detectors, has been operating successfully at Yangbajing in Tibet, China since 1999. Using the…”
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Computed tomography has low sensitivity for the diagnosis of early colon cancer by Lao, I-H., Chao, H., Wang, Y.-J., Mak, C.-W., Tzeng, W.-S., Wu, R.-H., Chang, S.-T., Fang, J.-L.

“…Aim The accuracy of computed tomography (CT) in detecting local invasion (T status) and nodal metastasis (N status) of colon cancer was determined. Method Data…”
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Large-Scale Sidereal Anisotropy of Galactic Cosmic-Ray Intensity Observed by 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, 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, Zhang, Yi, Zhaxisangzhu, Zhou, X. X

“…We present the large-scale sidereal anisotropy of Galactic cosmic-ray intensity in the multi-TeV region observed with the Tibet-III air shower array during the…”
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Tissue Distribution of the 27.8 kDa Receptor and its Dynamic Expression in Response to Lymphocystis Disease Virus Infection in Flounder (Paralichthys olivaceus) by Wu, R.-H., Tang, X.-Q., Sheng, X.-Z., Zhan, W.-B.

“…Lymphocystis disease virus (LCDV) enters and infects the gill cells of flounder (Paralichthys olivaceus) via a 27.8 kDa membrane protein receptor. In the…”
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Involvement of cannabinoid‐1 and cannabinoid‐2 receptors in septic ileus by Li, Y.‐y., Li, Y.‐n., Ni, J.‐b., Chen, C.‐j., Lv, S., Chai, S.‐y., Wu, R.‐h., Yüce, B., Storr, M.

“…Background  Cannabinoid (CB) receptors are involved in the regulation of gastrointestinal (GI) motility under physiological and pathophysiological conditions…”
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On Temporal Variations of the Multi-TeV Cosmic Ray Anisotropy Using the Tibet III Air Shower Array by Amenomori, M, Bi, X. J, Chen, D, Cui, S. W, Danzengluobu, Ding, L. K, Ding, X. H, Fan, C, Feng, C. F, Feng, Zhaoyang, Feng, Z. Y, Gao, X. Y, Geng, Q. X, Gou, Q. B, Guo, H. W, He, H. H, He, M, Hibino, K, Hotta, N, Hu, Haibing, Hu, H. B, Huang, J, Huang, Q, Jia, H. Y, Jiang, L, Kajino, F, Kasahara, K, Katayose, Y, Kato, C, Kawata, K, Labaciren, Le, G. M, Li, A. F, Li, H. C, Li, J. Y, Liu, C, Lou, Y.-Q, Lu, H, Meng, X. R, Mizutani, K, Mu, J, Munakata, K, Nagai, A, Nanjo, H, Nishizawa, M, Ohnishi, M, Ohta, I, Ozawa, S, Saito, T, Saito, T. Y, Sakata, M, Sako, T. K, 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, Y, 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, Zhang, Ying, Zhaxisangzhu, Zhou, X. X

“…We analyze the large-scale two-dimensional sidereal anisotropy of multi-TeV cosmic rays (CRs) by the Tibet Air Shower Array, with the data taken from 1999…”
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PB2325: APPLICATION AND COMPARISON OF TWO PHARMACOKINETIC DETECTION METHODS IN CHILDREN WITH HEMOPHILIA A—AN INSPECTION REPORT FROM SINGLE CENTER by Li, C.‐G., Wang, Y., Mai, H.‐R., Fang, X.‐M., Long, Q.‐L., Zhou, G.‐C., Wang, C.‐Y., Liu, S.‐X., Fu, X.‐Y., Shu, Q.‐R., Cai, L.‐S., Chen, Z.‐P., Wu, R.‐H.

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EIF5A2 predicts outcome in localised invasive bladder cancer and promotes bladder cancer cell aggressiveness in vitro and in vivo by Wei, J-H, Cao, J-Z, Zhang, D, Liao, B, Zhong, W-M, Lu, J, Zhao, H-W, Zhang, J-X, Tong, Z-T, Fan, S, Liang, C-Z, Liao, Y-B, Pang, J, Wu, R-H, Fang, Y, Chen, Z-H, Li, B, Xie, D, Chen, W, Luo, J-H

“…Background: EIF5A2, eukaryotic translation initiation factor 5A2, is associated with several human cancers. In this study, we investigated the role of EIF5A2…”
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A Northern Sky Survey for Steady Tera-Electron Volt Gamma-Ray Point Sources Using the Tibet Air Shower Array 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, Takashima, M, Takita, M, Tan, Y. H, Tateyama, N, Torii, S, Tsuchiya, H, Udo, S, Utsugi, T, 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, Yi, Zhang, Y, Zhaxisangzhu, Zhou, X. X

“…Results of a steady TeV g-ray point-source search using data taken from the Tibet HD (1997 February -1999 September) and Tibet III (1999 November-2001 October)…”
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