The 3rd PANDA Symposium on Time Domain Astronomy and first results from Insight-HXMT
Chengdu(成都), China
*** SYMPOSIUM BACKGROUND***
The PANDA Symposia series are aiming at establishing and fostering collaborations among young postdoctoral fellows (0-6 years from graduation) from the Pacific/Asiatic scientific community with their peers across the globe. Besides enabling scientific mobility and networking, we are also aiming in providing young researchers with a forum to exchange ideas on current and future projects. The Symposia should take place every 2-3 years and have been held successfully two times.
*** SCIENTIFIC RATIONALE ***
The Hard X-ray Modulation Telescope (HXMT), also known as Insight, is China’s first space X-ray astronomy satellite, designed to observe X-ray emission from galactic and extragalactic transients, and compact objects, such as black holes, neutron stars and gamma-ray bursts (GRBs). This satellite was launched on June 15, 2017; it has completed the commissioning phase and it is now in full operational mode. The mission also participated in a global joint observation in search of the electromagnetic counterparts of GW170817, providing stringent constraints for the properties of the binary neutron star merger. We plan to unveil the first scientific results from the Insight-HXMT a year after its launch, and discuss some hot topics in high-energy astrophysics. Hence, we organize the third PANDA Symposium, aiming at introducing the Insight-HXMT results to an international astrophysics community.
***SCIENTIFIC AGENDA***
The 3rd PANDA Symposium aims to include experts in many high-energy astrophysics areas, in particular multi-wavelength Time Domain Astrophysics. It is organized in 5 days focused presenting the satellite’s instrument operation status and performance as well as scientific contributions interspersed in several scientific areas encompassing extreme astrophysical environments and the physical processes in the transient Universe: gravitational waves and their electromagnetic counterparts, Gamma-Ray Bursts, accretion on black holes and neutron stars, pulsars, magnetars, as well as Galactic Plane monitoring and surveying for high energy transients. A good part of the meeting will be dedicated in lively discussions fostering international multi-wavelength collaborations on new ideas and multi- mission projects.
Afamuefuna Valentine Eze
Alessandro Patruno
Alexander van der Horst
Baiyang Wu
Bei You
Beibei Dai
Binbin Zhang
Bing Li
Bingqiu Chen
Can Gungor
Changsheng Shi
CHENGCHENG(程程) GUO(郭)
Chengkui 李承奎
Chryssa Kouveliotou
Dahai(大海) Yan(闫)
Di Li
Di Xiao
Donghua ZHAO
Enwei Liang
Fangkun Peng
Feng Yuan
Guobao Zhang
Guoqiang (国强) Ding (丁)
Hai Yu
Haibo Yuan
haisheng ZHAO Haisheng
Hancheng(汉成) LI(李)
Hao(昊) Liu(刘)
Hirofumi Noda
Houdun Zeng
Hsiang-Kuang Chang
Hui Yang
Jianfeng Zhou
Jianping Yuan
Jie Lin
Jieru Song
Jingwei Hu
Jinke He
Jinyuan 廖进元
John Ruan
Jonathan Granot
Ju Guan
Juan ZHANG
kang chen
Kenta Hotokezaka
Kun XU
Kunihito Ioka
Lang Shao
Lara Nava
Lei Sun
Lei Sun
Leo Singer
Lian Tao
Liang Sun Liang
liang zhang
Liming Song
Linli(林丽) YAN（闫）
Liping Xin
Longbiao Li
luo 雒涛
Martin Ward
Menquan Liu
Ming Lyu
Na(娜) Sai(赛)
Nang Yi(曩毅)
Nozomu Tominaga
Pak Hin Tam
Partha Sarathi Pal
pawan kumar
Paz Beniamini
Pei Wang
Q. Daniel Wang
Qian-Qing Yin
Qiang Yuan
Qingcui Bu
Quan Cheng
REETANJALI MOHARANA
Rong-Feng Shen
Rui Huang
Shangyu Sun
Shaolin Xiong
Shaoshao Wang
Shu Zhang
Shuang-Nan Zhang
Shumei 贾淑梅
Tianxiang Chen
tsvi piran
Wenbin Lu
WenFei Yu
Wenjie Zhang
wenzhao zhang
Xian LI Xian
Xiang Ma
Xiang-Gao Wang
xiao zhang
Xiaobo 李小波
Xiaochuan Chang
xiaohua liang
Yanji Yang
Yanli Qiu
Yashpal Bhulla
yi xing
Yi ZHAO
Yi-Jung Yang
Yong CHEN
Yong-Feng Huang
Yu Peng 陈玉鹏
Yuanming Wang
Yuanyuan Du
Yudong CUI
Yue HUANG
Yue ZHANG
Yue Zhao
Yun-Wei YU
Zhen Cheng
Zhengheng (正恒) Li (李)
Zhigang Wen
Zhiping Jin
Zhongxiang Wang
Zigao Dai
世界 郑
东铭 毛
伟 张
伟长风 郭
伯冰 Bobing Wu
元月 潘
兆升 李
宇 王
富国 谢
广成 肖
建胤 聂建胤
德华 王
惠 孙
惠惠 王
承民 张
攸隶 庹
新文 舒
明玉 葛
星星 胡
晓为 刘
晓杰 徐
晨 王
李 玉丰
正华 安
海武 潘
海涛 李
灵俊 王
逸炜 包
鹏程 杨
