Progress of GECAM Observation Research  

作　　者：WANG Chenwei ZHANG Yanqiu XIONG Shaolin LIU Jiacong TAN Wenjun XIAO Shuo XIE Shenglun XUE Wangchen ZHAO Haisheng ZHAO Yi ZHENG Chao 

机构地区：[1]Key Laboratory of Particle Astrophysics,Institute of High Energy Physics,Chinese Academy of Sciences,Beijing 100049 [2]University of Chinese Academy of Sciences,Beijing 100049 [3]Guizhou Normal University,Guizhou 550025 [4]Central China Normal University,Wuhan 4300795 [5]Dezhou University,Dezhou 253023

出　　处：《空间科学学报》2024年第4期668-673,共6页Chinese Journal of Space Science

摘　　要：Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor(GECAM)is a constellation with four instruments(launch date):GECAM-A/B(10 December 2020),GECAM-C(27 July 2022)and GECAM-D(13 March 2024),which are dedicated to monitoring gamma-ray transients in all-sky.The primary science objectives of GECAM include Gamma-Ray Bursts(GRBs),Soft Gamma-ray Repeaters(SGRs),high energy counterparts of Gravitation Wave(GW)and Fast Radio Burst(FRB),Solar Flares(SFLs),as well as Terrestrial Gamma-ray Flashes(TGFs)and Terrestrial Electron Beams(TEBs).A series of observations and research have been made since the launch of GECAM-A/B.GECAM observations provide new insights into these highenergy transients,demonstrating the unique role of GECAM in the“multi-wavelength,multi-messenger”era.

关 键 词：GECAM Gravitational wave electromagnetic counterpart High energy transients 

分 类 号：V474[航空宇航科学与技术—飞行器设计]