Collaborations are very welcome and are foreseen to join the core science team of Insight-HXMT in the following three ways:
1) Partner institutions that had provided contributions to HXMT;
2) Coordinate multi-wavelength observations of both in space and on ground;
3) Fill the application form and send it to the leader of a specific core science group of Insight-HXMT and cc the email to the PI of Insight-HXMT.
(1)Form for application to join the core science team
(This form is applicable to any researcher (regardless of nationality) who has an official position in China, but not to students, postdocs and visitors)
(2)Form for application of Insight-HXMT core science data within the proprietary period
(Applicable only to core science team member)
(3)Form for application of Insight-HXMT core science data within the proprietary period
(Applicable to association team member)
The core science groups of HXMT:
Group 1: accretion X-ray binaries (leaders: Qu Jin Lu ( qujl@ihep.ac.cn), Zhang Shu ( szhang@ihep.ac.cn), vice leaders: Cui Wei, Tao Lian, Chen YuPeng)
Group 2: Galactic survey and diffuse emission research (leader: Liu Yuan ( liuyuan@ihep.ac.cn), vice leader: Li ChengKui)
Group 3: Multi-wavelength observations (leader: Liu JiFeng ( jfliu@nao.cas.cn), vice leader: Xiong Shao Lin)
Group 4: Calibration and background model (leader: Song LiMing ( songlm@ihep.ac.cn), vice leader: Liao Jin Yuan)
Group 5: pulsar navigation (leader: Zheng Shi Jie ( zhengsj@ihep.ac.cn), vice leader: Zheng Wei)
Group 6: Extragalactic sources (leader: Yuan Wei Min ( wmy@nao.cas.cn), vice leader: Jia Shu Mei)
Group 7: Gamma-ray bursts and gravitational wave EM counterparts (leader: Xiong Shao Lin ( xiongsl@ihep.ac.cn), vice leader: Liu Cong Zhan)
Group 8: non-accreting pulsars (leader: Zhang Shuang Nan ( zhangsn@ihep.ac.cn), vice leader: Ge Ming Yu)