Zobrazeno 1 - 10
of 397
pro vyhledávání: '"Tang, ZhengHong"'
The systematic errors are inevitable in Gaia published astrometric data. Lindegren et al. (L21) proposed a global recipe to correct for the GEDR3 parallax zero point offset, which did not consider the Galactic plane. The applicability of their correc
Externí odkaz:
http://arxiv.org/abs/2409.15694
Autor:
Ge, Jian, Zhang, Hui, Zang, Weicheng, Deng, Hongping, Mao, Shude, Xie, Ji-Wei, Liu, Hui-Gen, Zhou, Ji-Lin, Willis, Kevin, Huang, Chelsea, Howell, Steve B., Feng, Fabo, Zhu, Jiapeng, Yao, Xinyu, Liu, Beibei, Aizawa, Masataka, Zhu, Wei, Li, Ya-Ping, Ma, Bo, Ye, Quanzhi, Yu, Jie, Xiang, Maosheng, Yu, Cong, Liu, Shangfei, Yang, Ming, Wang, Mu-Tian, Shi, Xian, Fang, Tong, Zong, Weikai, Liu, Jinzhong, Zhang, Yu, Zhang, Liyun, El-Badry, Kareem, Shen, Rongfeng, Tam, Pak-Hin Thomas, Hu, Zhecheng, Yang, Yanlv, Zou, Yuan-Chuan, Wu, Jia-Li, Lei, Wei-Hua, Wei, Jun-Jie, Wu, Xue-Feng, Sun, Tian-Rui, Wang, Fa-Yin, Zhang, Bin-Bin, Xu, Dong, Yang, Yuan-Pei, Li, Wen-Xiong, Xiang, Dan-Feng, Wang, Xiaofeng, Wang, Tinggui, Zhang, Bing, Jia, Peng, Yuan, Haibo, Zhang, Jinghua, Wang, Sharon Xuesong, Gan, Tianjun, Wang, Wei, Zhao, Yinan, Liu, Yujuan, Wei, Chuanxin, Kang, Yanwu, Yang, Baoyu, Qi, Chao, Liu, Xiaohua, Zhang, Quan, Zhu, Yuji, Zhou, Dan, Zhang, Congcong, Yu, Yong, Zhang, Yongshuai, Li, Yan, Tang, Zhenghong, Wang, Chaoyan, Wang, Fengtao, Li, Wei, Cheng, Pengfei, Shen, Chao, Li, Baopeng, Pan, Yue, Yang, Sen, Gao, Wei, Song, Zongxi, Wang, Jian, Zhang, Hongfei, Chen, Cheng, Wang, Hui, Zhang, Jun, Wang, Zhiyue, Zeng, Feng, Zheng, Zhenhao, Zhu, Jie, Guo, Yingfan, Zhang, Yihao, Li, Yudong, Wen, Lin, Feng, Jie, Chen, Wen, Chen, Kun, Han, Xingbo, Yang, Yingquan, Wang, Haoyu, Duan, Xuliang, Huang, Jiangjiang, Liang, Hong, Bi, Shaolan, Gai, Ning, Ge, Zhishuai, Guo, Zhao, Huang, Yang, Li, Gang, Li, Haining, Li, Tanda, Yuxi, Lu, Rix, Hans-Walter, Shi, Jianrong, Song, Fen, Tang, Yanke, Ting, Yuan-Sen, Wu, Tao, Wu, Yaqian, Yang, Taozhi, Yin, Qing-Zhu, Gould, Andrew, Lee, Chung-Uk, Dong, Subo, Yee, Jennifer C., Shvartzvald, Yossi, Yang, Hongjing, Kuang, Renkun, Zhang, Jiyuan, Liao, Shilong, Qi, Zhaoxiang, Yang, Jun, Zhang, Ruisheng, Jiang, Chen, Ou, Jian-Wen, Li, Yaguang, Beck, Paul, Bedding, Timothy R., Campante, Tiago L., Chaplin, William J., Christensen-Dalsgaard, Jørgen, García, Rafael A., Gaulme, Patrick, Gizon, Laurent, Hekker, Saskia, Huber, Daniel, Khanna, Shourya, Mathur, Savita, Miglio, Andrea, Mosser, Benoît, Ong, J. M. Joel, Santos, Ângela R. G., Stello, Dennis, Bowman, Dominic M., Lares-Martiz, Mariel, Murphy, Simon, Niu, Jia-Shu, Ma, Xiao-Yu, Molnár, László, Fu, Jian-Ning, De Cat, Peter, Su, Jie, consortium, the ET
We propose to develop a wide-field and ultra-high-precision photometric survey mission, temporarily named "Earth 2.0 (ET)". This mission is designed to measure, for the first time, the occurrence rate and the orbital distributions of Earth-sized plan
Externí odkaz:
http://arxiv.org/abs/2206.06693
Autor:
Tang, Zhenghong
The lack of early integration with the planning and decision-making process has been a major problem in environmental assessment. Traditional project-based environmental impact assessment has inadequate incentives and capacities to incorporate critic
Externí odkaz:
http://hdl.handle.net/1969.1/ETD-TAMU-1382
Quasars are very important in materializing the reference frame. The excess emission of AGNs (active galactic nuclei) in the mid infrared band can be used to identify quasar candidates. As extremely distant and point like objects, quasars also could
Externí odkaz:
http://arxiv.org/abs/2111.02131
Autor:
Huang, Yingze, Qiu, Bingwen, Yang, Peng, Wu, Wenbin, Chen, Xuehong, Zhu, Xiaolin, Xu, Shuai, Wang, Laigang, Dong, Zhanjie, Zhang, Jianyang, Berry, Joe, Tang, Zhenghong, Tan, Jieyang, Duan, Dingding, Peng, Yufeng, Lin, Duoduo, Cheng, Feifei, Liang, Juanzhu, Huang, Hongyu, Chen, Chongcheng
Publikováno v:
In Computers and Electronics in Agriculture June 2024 221
Autor:
Qiu, Bingwen, Jian, Zeyu, Yang, Peng, Tang, Zhenghong, Zhu, Xiaolin, Duan, Mingjie, Yu, Qiangyi, Chen, Xuehong, Zhang, Miao, Tu, Ping, Xu, Weiming, Zhao, Zhiyuan
Publikováno v:
In Agricultural Systems April 2024 216
Autor:
Peng, Yufeng, Qiu, Bingwen, Tang, Zhenghong, Xu, Weiming, Yang, Peng, Wu, Wenbin, Chen, Xuehong, Zhu, Xiaolin, Zhu, Peng, Zhang, Xin, Wang, Xinshuang, Zhang, Chengming, Wang, Laigang, Li, Mengmeng, Liang, Juanzhu, Huang, Yingze, Cheng, Feifei, Chen, Jianfeng, Wu, Fangzheng, Jian, Zeyu, Li, Zhengrong
Publikováno v:
In Remote Sensing of Environment 15 March 2024 303
Autor:
Gai, Mario, Vecchiato, Alberto, Riva, Alberto, Lattanzi, Mario Gilberto, Landini, Federico, Bucciarelli, Beatrice, Busonero, Deborah, Crosta, Mariateresa, Liao, Shilong, Luo, Hao, Mana, Giovanni, Pisani, Marco, Qi, Zhaoxiang, Sasso, Carlo Paolo, Tang, Zhenghong, Yong, Yu
Publikováno v:
Proc. SPIE 11443, 114430N (2020)
The Astrometric Gravitation Probe mission is a modern version of the 1919 Dyson-Eddington-Davidson experiment, based on a space-borne telescope with a permanent built-in eclipse, provided by a coronagraphic system. The expected improvement on experim
Externí odkaz:
http://arxiv.org/abs/2104.03756
Autor:
Gai, Mario, Qi, Zhaoxiang, Lattanzi, Mario G., Bucciarelli, Beatrice, Busonero, Deborah, Crosta, Mariateresa, Landini, Federico, Liao, Shilong, Luo, Hao, Mana, Giovanni, Méndez, Rene A., Pisani, Marco, Riva, Alberto, Luque, Claudia San Martin, Sasso, Carlo P., Tang, Zhenghong, Vecchiato, Alberto, Yong, Yu
Publikováno v:
Proc. SPIE 11451, 114514I (2020)
Astrometric Science and Technology Roadmap for Astrophysics (ASTRA) is a bilateral cooperation between China and Italy with the goal of consolidating astrometric measurement concepts and technologies. In particular, the objectives include critical an
Externí odkaz:
http://arxiv.org/abs/2104.03146
Autor:
Riva, Alberto, Gai, Mario, Vecchiato, Alberto, Busonero, Deborah, Lattanzi, Mario G., Landini, Federico, Qi, Zhaoxiang, Tang, Zhenghong
Publikováno v:
Proc. SPIE 11443, 114430P (13 December 2020)
High precision astrometry aims at source position determination to a very small fraction of the diffraction image size, in high SNR regime. One of the key limitations to such goal is the optical response variation of the telescope over a sizeable FOV
Externí odkaz:
http://arxiv.org/abs/2104.03003