Search Results - "Qu, X. B."

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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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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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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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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Northern Sky Galactic Cosmic Ray Anisotropy between 10 and 1000 TeV with the Tibet 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., 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 report on the analysis of the 10-1000 TeV large-scale sidereal anisotropy of Galactic cosmic rays (GCRs) with the data collected by the Tibet Air Shower…”
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Potential PeVatron supernova remnant G106.3+2.7 seen in the highest-energy gamma rays 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.

“…Cosmic rays (protons and other atomic nuclei) are believed to gain energies of petaelectronvolts (PeV) and beyond at astrophysical particle accelerators called…”
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Review and Prospect: Deep Learning in Nuclear Magnetic Resonance Spectroscopy by Chen, Dicheng, Wang, Zi, Guo, Di, Orekhov, Vladislav, Qu, Xiaobo

“…Since the concept of deep learning (DL) was formally proposed in 2006, it has had a major impact on academic research and industry. Nowadays, DL provides an…”
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Accelerated NMR Spectroscopy with Low-Rank Reconstruction by Qu, Xiaobo, Mayzel, Maxim, Cai, Jian-Feng, Chen, Zhong, Orekhov, Vladislav

“…Accelerated multi‐dimensional NMR spectroscopy is a prerequisite for high‐throughput applications, studying short‐lived molecular systems and monitoring…”
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A novel hypothesis: specific oncogenes and tumor suppression genes are involved in the expression of the proopiomelanocortin gene by small cell lung cancer by Amsler, U J, Pasi, A, Qu, B X

“…The endogenous opioid beta-endorphin, a derivative of proopiomelanocortin, stimulates the growth of cloned human small cell lung carcinoma. The present…”
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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, Bi, X. J, Chen, D, Chen, T. L, Chen, W. Y, Chen, Xu, Cirennima, Cui, S. W, Danzengluobu, Ding, L. K, Fang, J. H, Fang, K, Feng, C. F, Feng, Zhaoyang, Feng, Z. Y, Gomi, A, Gou, Q. B, Guo, Y. Q, Guo, Y. Y, Hayashi, Y, He, H. H, He, Z. T, Hibino, K, Hotta, N, Hu, Haibing, Hu, H. B, Hu, K. Y, Huang, J, Jiang, L, Jiang, P, Jin, H. B, Kasahara, K, Katayose, Y, Kato, C, Kato, S, Kawahara, I, Kawashima, T, Labaciren, Le, G. M, Li, A. F, Li, H. J, Li, W. J, Li, Y, Liu, B, Liu, C, Liu, J. S, Liu, L. Y, Liu, M. Y, Liu, W, Lu, H, Meng, X. R, Meng, Y, Munakata, K, Nagaya, K, Nakamura, Y, Nakazawa, Y, Nanjo, H, Ning, C. C, Nishizawa, M, Noguchi, R, Okukawa, S, Qian, X, Qu, X. B, Saito, T, 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, Tsuchiya, H, Wang, H, Wang, S. F, Wang, Y. P, 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, J. L, Zhang, X, Zhang, X. Y, Zhang, Y, Zhang, Yi, Zhang, Ying, Zhao, S. P, Zhaxisangzhu, Zou, Y. H

“…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. The…”
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A Sparse Model-Inspired Deep Thresholding Network for Exponential Signal Reconstruction-Application in Fast Biological Spectroscopy by Wang, Zi, Guo, Di, Tu, Zhangren, Huang, Yihui, Zhou, Yirong, Wang, Jian, Feng, Liubin, Lin, Donghai, You, Yongfu, Agback, Tatiana, Orekhov, Vladislav, Qu, Xiaobo

“…The nonuniform sampling (NUS) is a powerful approach to enable fast acquisition but requires sophisticated reconstruction algorithms. Faithful reconstruction…”
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Potential PeVatron supernova remnant G106.3+2.7 seen in the highest-energy gamma rays 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

“…Nature Astronomy, 5, 460-464 (2021) Cosmic rays (protons and other atomic nuclei) are believed to gain energies of petaelectronvolts (PeV) and beyond at…”
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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, 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, 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, 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, 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, Sakata, M, Sako, T, Shao, J, Shibata, M, Shiomi, A, Sugimoto, H, Takano, W, Tan, Y. H, Tateyama, N, Torii, S, Tsuchiya, H, Udo, S, Wang, H, Wang, Y. P, Wu, H. R, Wu, Q, Xu, J. L, Yamamoto, Y, 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, Zhang, X. Y, Zhang, Y, Zhang, Yi, Zhang, Ying, Zhaxisangzhu, Zhou, X. X

“…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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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

“…Phys. Rev. Lett. 126, 141101 (2021) We report, for the first time, the long-awaited detection of diffuse gamma rays with energies between 100 TeV and 1 PeV in…”
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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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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

“…Phys. Rev. Lett. 123, 051101 (2019) We report on the highest energy photons from the Crab Nebula observed by the Tibet air shower array with the underground…”
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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, S. A. F, Zhai, L. M, Zhang, H. M, Zhang, J. L, Zhang, X. Y, Zhang, Y, Zhang, Yi, Zhang, Ying, Zhaxisangzhu, Zho, X. X

“…ApJ 860 (2018) We examine the possible influence of Earth-directed coronal mass ejections (ECMEs) on the Sun's shadow in the 3~TeV cosmic-ray intensity…”
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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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