Kongjian kexue xuebao (Aug 2024)

Progress of GECAM Observation Research

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

DOI
https://doi.org/10.11728/cjss2024.04.2024-yg13
Journal volume & issue
Vol. 44
pp. 668 – 673

Abstract

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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 high-energy transients, demonstrating the unique role of GECAM in the “multi-wavelength, multi-messenger” era.

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