韓旭輝

主要研究方向為天文技術與方法。在 SVOM 任務中擔任“科學運行分系統副主任設計師”，負責 SVOM GRB 警報處理系統的方案設計和研發， 負責SVOM ToO Tools的方案設計和研發；參與完成了 SVOM BA Tools 和 ToO Tools的需求分析。SVOM GRB 警報處理系統、 BA tools和ToO Tools已參加兩輪 SVOM 系統級測試，完成全部測試項目，滿足各項指標要求；還承擔SVOM 地基光學望遠鏡後隨觀測網絡構建任務。為此，開展瞭望遠鏡動態規劃技術，望遠鏡網絡中通信時序控制技術，數據中心管理機制等關鍵技術研究。基於上述技術的SVOM/GWAC-N 網絡在2019-2020 觀測季中，共自動觀測 17 個引力波事件；目前，正主導開展SVOM 關鍵子系統之一的“科學用户支持系統“ 的GP tools的研發。 ^[1] 

1. Xuhui Han; Yujie Xiao; PinPin Zhang; Damien Turpin; Liping Xin; Chao Wu; Hongbo Cai; Wenl ong Dong; Lei Huang; Zhe Kang; Nicolas Leroy; Huali Li; Zhenwei Li; Xiaomeng Lu; Yulei Qiu; Benja min E. Stahl; Jing Wang; Xianggao Wang; Yang Xu; Yuangui Yang; Yong Zhao; Ruosong Zhang; Weikang Zheng; Yatong Zheng; Jianyan Wei ; An Automated Observation Management System of GWAC Network I: System Architecture and Workflow, Publications of the Astronomical Society of the Pacific, 2021, 133(065001): 065001-065018

2. Turpin Damien; Wu Chao; Han Xuhui; Xin Liping; Antier Sarah; Leroy Nicolas; Cao Li; Cai H ongbo; Cordier Bertrand; Deng Jinsong; Dong Wenlong; Feng Qichen; Huang Lei; Jia Lei; Klotz Alain ; Lachaud Cyril; Li Huali; Liang Enwei; Liu Shunfang; Lu Xiaomeng; Meng Xianmin; Qiu Yulei; Wang Huijuan; Wang Jing; Wang Shen; Wang Xianggao; Wei Jianyan; Wu Bobing; Xiao Yujie; Xu Dawei; Xu Ya ng; Yang Yuangui; Zhang Pinpin; Zhang Ruosong; Zhang Shuangnan; Zheng Yatong; Zou Sicheng ; The m ini-GWAC optical follow-up of gravitational wave alerts- results from the O2 campaign and prospec ts for the upcoming O3 run, Research in Astronomy and Astrophysics, 2020, 20(1): 13-30

3. Xuhui Han; WeiKang Zheng; Benjamin E.Stahl; Jamison Burke; Jozsef Vinko; Thomas de Jaeger ; Iair Arcavi; Thomas G.Brink; Borbala Cseh; Daichi Hiramatsu; Griffin Hosseinzadeh; D.Andrew How ell; Bernadett Ignacz; Reka Konyves-Toth; Mate Krezinger; Curtis McCully; Andras Ordasi; Dora Pin ter; Krisztian Sarneczky; Robert Szakats; Kevin Tang; Krisztian Vida; Jing Wang; Jianyan Wei; J.C raig Wheeler; Liping Xin; Alexei V.Filippenko ; SN 2017cfd: A Normal Type Ia Supernova Discovered Very Young, The Astrophysical Journal, 2020, 892(2): 142-152 ^[1]