Zobrazeno 1 - 10
of 27
pro vyhledávání: '"Fan, YiZhong"'
Autor:
GRAND Collaboration, Batista, Rafael Alves, Benoit-Lévy, Aurélien, Bister, Teresa, Bustamante, Mauricio, Chen, Yiren, Cheng, LingMei, Chiche, Simon, Colley, Jean-Marc, Correa, Pablo, Laurenciu, Nicoleta Cucu, Dai, Zigao, de Errico, Beatriz, de Jong, Sijbrand, Neto, João R. T. de Mello, de Vries, Krijn D., Denton, Peter B., Deocoene, Valentin, Duan, Kaikai, Duan, Bohao, Engel, Ralph, Fan, Yizhong, Ferrière, Arsène, Gou, QuanBu, Gu, Junhua, Guelfand, Marion, Guo, Jianhua, Guo, Yiqing, Gupta, Vaidhai, Guépin, Claire, Gülzow, Lukas, Haungs, Andreas, He, Haoning, Hivon, Eric, Hu, Hongbo, Huang, Xiaoyuan, Huang, Yan, Huege, Tim, Jiang, Wen, Koirala, Ramesh, Kotera, Kumiko, Köhler, Jelena, Lago, Bruno L., Coz, Sandra Le, Legrand, François, Leisos, Antonios, Li, Rui, Liu, Cheng, Liu, Ruoyu, Liu, Wei, Ma, Pengxiong, Macias, Oscar, Magnard, Frédéric, Martineau-Huynh, Olivier, Mikhno, Ananstasiia, Mitra, Pragati, Mostafá, Miguel, Mottez, Fabrice, Mouette, Jean, Murase, Kohta, Niess, Valentin, Nonis, Stavros, Ogio, Shoichi, Oikonomou, Foteini, Pierog, Tanguy, Piotrowski, Lech Wiktor, Poisvert, Pierre, Prunet, Simon, Qian, Xiangli, Roth, Markus, Sako, Takashi, Schoorlemmer, Harm, Steeman, Bart, Szálas-Motesiczky, Dániel, Sławiński, Szymon, Timmermans, Anne, Timmermans, Charles, Tsirigotis, Apostolos, Tueros, Matías, Wang, Shen, Wang, Xiangyu, Wang, Xu, Wei, Daming, Wei, Feng, Wu, Xiangping, Wu, Xuefeng, Xu, Xin, Xu, Xing, Yang, Lili, Yang, Xuan, Yuan, Qiang, Zarka, Philippe, Zeng, Houdun, Zhang, Chao, Zhang, Jianli, Zhang, Kewen, Zhang, Pengfei, Zhang, Songbo, Zhou, Hao
The Giant Radio Array for Neutrino Detection (GRAND) is an envisioned observatory of ultra-high-energy particles of cosmic origin, with energies in excess of 100 PeV. GRAND uses large surface arrays of autonomous radio-detection units to look for the
Externí odkaz:
http://arxiv.org/abs/2308.00120
Autor:
WFST Collaboration, Wang, Tinggui, Liu, Guilin, Cai, Zhenyi, Geng, Jinjun, Fang, Min, He, Haoning, Jiang, Ji-an, Jiang, Ning, Kong, Xu, Li, Bin, Li, Ye, Luo, Wentao, Pan, Zhizheng, Wu, Xuefeng, Yang, Ji, Yu, Jiming, Zheng, Xianzhong, Zhu, Qingfeng, Cai, Yi-Fu, Chen, Yuanyuan, Chen, Zhiwei, Dai, Zigao, Fan, Lulu, Fan, Yizhong, Fang, Wenjuan, He, Zhicheng, Hu, Lei, Hu, Maokai, Jin, Zhiping, Jiang, Zhibo, Li, Guoliang, Li, Fan, Li, Xuzhi, Liang, Runduo, Lin, Zheyu, Liu, Qingzhong, Liu, Wenhao, Liu, Zhengyan, Liu, Wei, Liu, Yao, Lou, Zheng, Qu, Han, Sheng, Zhenfeng, Shi, Jianchun, Shu, Yiping, Su, Zhenbo, Sun, Tianrui, Wang, Hongchi, Wang, Huiyuan, Wang, Jian, Wang, Junxian, Wei, Daming, Wei, Junjie, Xue, Yongquan, Yan, Jingzhi, Yang, Chao, Yuan, Ye, Yuan, Yefei, Zhang, Hongxin, Zhang, Miaomiao, Zhao, Haibin, Zhao, Wen
Publikováno v:
SCPMA-Vol. 66 No. 10: 109512 (2023)
The Wide Field Survey Telescope (WFST) is a dedicated photometric surveying facility being built jointly by the University of Science and Technology of China and the Purple Mountain Observatory. It is equipped with a 2.5-meter diameter primary mirror
Externí odkaz:
http://arxiv.org/abs/2306.07590
Autor:
Alemanno, Francesca, An, Qi, Azzarello, Philipp, Barbato, Felicia Carla Tiziana, Bernardini, Paolo, Bi, XiaoJun, Cai, MingSheng, Casilli, Elisabetta, Catanzani, Enrico, Chang, Jin, Chen, DengYi, Chen, JunLing, Chen, ZhanFang, Cui, MingYang, Cui, TianShu, Cui, YuXing, Dai, HaoTing, De Benedittis, Antonio, De Mitri, Ivan, de Palma, Francesco, Deliyergiyev, Maksym, Di Santo, Margherita, Ding, Qi, Dong, TieKuang, Dong, ZhenXing, Donvito, Giacinto, Droz, David, Duan, JingLai, Duan, KaiKai, D'Urso, Domenico, Fan, RuiRui, Fan, YiZhong, Fang, Fang, Fang, Kun, Feng, ChangQing, Feng, Lei, Fusco, Piergiorgio, Gao, Min, Gargano, Fabio, Gong, Ke, Gong, YiZhong, Guo, DongYa, Guo, JianHua, Han, ShuangXue, Hu, YiMing, Huang, GuangShun, Huang, XiaoYuan, Huang, YongYi, Ionica, Maria, Jiang, Wei, Kong, Jie, Kotenko, Andrii, Kyratzis, Dimitrios, Li, ., Lei, ShiJun, Li, WenHao, Li, WeiLiang, Li, Xiang, Li, XianQiang, Liang, YaoMing, Liu, ChengMing, Liu, Hao, Liu, Jie, Liu, ShuBin, Liu, Yang, Loparco, Francesco, Luo, ChuanNing, Ma, Miao, Ma, PengXiong, Ma, Tao, Ma, XiaoYong, Marsella, Giovanni, Mazziotta, Mario Nicola, Mo, Dan, Niu, XiaoYang, Pan, Xu, Parenti, Andrea, Peng, WenXi, Peng, XiaoYan, Perrina, Chiara, Qiao, Rui, Rao, JiaNing, Ruina, Arshia, Salinas, MariaMunoz, Shangguan, Zhi, Shen, WeiHua, Shen, ZhaoQiang, Shen, ZhongTao, Silveri, Leandro, Song, JingXing, Stolpovskiy, Mikhail, Su, Hong, Su, Meng, Sun, HaoRan, Sun, ZhiYu, Surdo, Antonio, Teng, XueJian, Tykhonov, Andrii, Wang, JinZhou, Wang, LianGuo, Wang, Shen, Wang, ShuXin, Wang, XiaoLian, Wang, Ying, Wang, YanFang, Wang, YuanZhu, Wei, DaMing, Wei, JiaJu, Wei, YiFeng, Wu, Di, Wu, Jian, Wu, LiBo, Wu, Sha Sha, Wu, Xin, Xia, ZiQing, Xu, EnHeng, Xu, HaiTao, Xu, ZhiHui, Xu, ZunLei, Xue, GuoFeng, Xu, ZiZong, Yang, HaiBo, Yang, Peng, Yang, YaQing, Yao, Hui Jun, Yu, YuHong, Yuan, GuanWen, Yuan, Qiang, Yue, Chuan, Zang, JingJing, Zhang, ShengXia, Zhang, WenZhang, Zhang, Yan, Zhang, Yi, Zhang, YongJie, Zhang, YunLong, Zhang, YaPeng, Zhang, YongQiang, Zhang, ZhiYong, Zhang, Zhe, Zhao, Cong, Zhao, HongYun, Zhao, XunFeng, Zhou, ChangYi, Zhu, Yan, Chen, Wei, Feng, Li, Luo, Xi, Zhu, ChengRui
The Forbush Decrease (FD) represents the rapid decrease of the intensities of charged particles accompanied with the coronal mass ejections (CMEs) or high-speed streams from coronal holes. It has been mainly explored with ground-based neutron monitor
Externí odkaz:
http://arxiv.org/abs/2110.00123
Autor:
Wen, Jiaxing, Long, Xiangyun, Zheng, Xutao, An, Yu, Cai, Zhengyang, Cang, Jirong, Che, Yuepeng, Chen, Changyu, Chen, Liangjun, Chen, Qianjun, Chen, Ziyun, Cheng, Yingjie, Deng, Litao, Deng, Wei, Ding, Wenqing, Du, Hangci, Duan, Lian, Gan, Quan, Gao, Tai, Gao, Zhiying, Han, Wenbin, Han, Yiying, He, Xinbo, He, Xinhao, Hou, Long, Hu, Fan, Hu, Junling, Huang, Bo, Huang, Dongyang, Huang, Xuefeng, Jia, Shihai, Jiang, Yuchen, Jin, Yifei, Li, Ke, Li, Siyao, Li, Yurong, Liang, Jianwei, Liang, Yuanyuan, Lin, Wei, Liu, Chang, Liu, Gang, Liu, Mengyuan, Liu, Rui, Liu, Tianyu, Liu, Wanqiang, Lu, Di'an, Lu, Peiyibin, Lu, Zhiyong, Luo, Xiyu, Ma, Sizheng, Ma, Yuanhang, Mao, Xiaoqing, Mo, Yanshan, Nie, Qiyuan, Qu, Shuiyin, Shan, Xiaolong, Shi, Gengyuan, Song, Weiming, Sun, Zhigang, Tan, Xuelin, Tang, Songsong, Tao, Mingrui, Wang, Boqin, Wang, Yue, Wang, Zhiang, Wu, Qiaoya, Wu, Xuanyi, Xia, Yuehan, Xiao, Hengyuan, Xie, Wenjin, Xu, Dacheng, Xu, Rui, Xu, Weili, Yan, Longbiao, Yan, Shengyu, Yang, Dongxin, Yang, Hang, Yang, Haoguang, Yang, Yi-Si, Yang, Yifan, Yao, Lei, Yu, Huan, Yu, Yangyi, Zhang, Aiqiang, Zhang, Bingtao, Zhang, Lixuan, Zhang, Maoxing, Zhang, Shen, Zhang, Tianliang, Zhang, Yuchong, Zhao, Qianru, Zhao, Ruining, Zheng, Shiyu, Zhou, Xiaolong, Zhu, Runyu, Zou, Yu, An, Peng, Cai, Yifu, Chen, Hongbing, Dai, Zigao, Fan, Yizhong, Feng, Changqing, Feng, Hua, Gao, He, Huang, Liang, Kang, Mingming, Li, Lixin, Li, Zhuo, Liang, Enwei, Lin, Lin, Lin, Qianqian, Liu, Congzhan, Liu, Hongbang, Liu, Xuewen, Liu, Yinong, Lu, Xiang, Mao, Shude, Shen, Rongfeng, Shu, Jing, Su, Meng, Sun, Hui, Tam, Pak-Hin, Tang, Chi-Pui, Tian, Yang, Wang, Fayin, Wang, Jianjun, Wang, Wei, Wang, Zhonghai, Wu, Jianfeng, Wu, Xuefeng, Xiong, Shaolin, Xu, Can, Yu, Jiandong, Yu, Wenfei, Yu, Yunwei, Zeng, Ming, Zeng, Zhi, Zhang, Bin-Bin, Zhang, Bing, Zhao, Zongqing, Zhou, Rong, Zhu, Zonghong
Publikováno v:
Exp. Astron. 48 (2019) 77
The Gamma-Ray Integrated Detectors (GRID) is a space mission concept dedicated to monitoring the transient gamma-ray sky in the energy range from 10 keV to 2 MeV using scintillation detectors onboard CubeSats in low Earth orbits. The primary targets
Externí odkaz:
http://arxiv.org/abs/1907.06842
We report the detection of GeV $\gamma$-ray emission from the very-high-energy (VHE) $\gamma$-ray source VER J2227+608 associated with the "tail" region of SNR G106.3+2.7. The GeV $\gamma$-ray emission is extended and spatially coincident with molecu
Externí odkaz:
http://arxiv.org/abs/1907.04972
Autor:
Wu, Xin, Su, Meng, Bravar, Alessandro, Chang, Jin, Fan, Yizhong, Pohl, Martin, Walter, Roland
We describe the instrument concept of a high angular resolution telescope dedicated to the sub-GeV (from $\gtrsim$10 MeV to $\gtrsim$1 GeV) gamma-ray photon detection. This mission, named PANGU (PAir-productioN Gamma-ray Unit), has been suggested as
Externí odkaz:
http://arxiv.org/abs/1407.0710
Akademický článek
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We intend to determine the type of circumburst medium and measure directly the initial Lorentz factor $\Gamma_0$ of GRB outflows. If the early X-ray afterglow lightcurve has a peak and the whole profile across the peak is consistent with the standard
Externí odkaz:
http://arxiv.org/abs/0902.2613
Publikováno v:
Mon.Not.Roy.Astron.Soc.389:321,2008
In the neutron-rich internal shocks model for gamma-ray bursts (GRBs), the Lorentz factors (LFs) of ion shells are variable, and so are the LFs of accompanying neutron shells. For slow neutron shells with a typical LF of approximate tens, the typical
Externí odkaz:
http://arxiv.org/abs/0810.3130
The X-ray afterglow flat segment in short GRB 051221A: Energy injection from a millisecond magnetar?
Autor:
Fan, Yizhong, Xu, Dong
Publikováno v:
Mon.Not.Roy.Astron.Soc.372:L19-L22,2006
The flat segment lasting $\sim 10^4$ seconds in the X-ray afterglow of GRB051221A represents the first clear case of strong energy injection in the external shock of a short GRB afterglow. In this work, we show that a millisecond pulsar with dipole m
Externí odkaz:
http://arxiv.org/abs/astro-ph/0605445