Volume 44 Issue 4
Sep.  2024
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Article Navigation >  Chinese Journal of Space Science  > 2024  >  44(4): 668-673 Open Access
WANG Chenwei, ZHANG Yanqiu, XIONG Shaolin, LIU Jiacong, TAN Wenjun, XIAO Shuo, XIE Shenglun, XUE Wangchen, ZHAO Haisheng, ZHAO Yi, ZHENG Chao. Progress of GECAM Observation Research. Chinese Journal of Space Science, 2024, 44(4): 668-673 doi: 10.11728/cjss2024.04.2024-yg13
Citation: WANG Chenwei, ZHANG Yanqiu, XIONG Shaolin, LIU Jiacong, TAN Wenjun, XIAO Shuo, XIE Shenglun, XUE Wangchen, ZHAO Haisheng, ZHAO Yi, ZHENG Chao. Progress of GECAM Observation Research. Chinese Journal of Space Science, 2024, 44(4): 668-673 doi: 10.11728/cjss2024.04.2024-yg13
shu

Progress of GECAM Observation Research

doi: 10.11728/cjss2024.04.2024-yg13 cstr: 32142.14.cjss2024.04.2024-yg13
  • 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 430079

  • 5.

    Dezhou University, Dezhou 253023

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  • Author Bio:

    Male. Born in July 1999 in Shijiazhuang, Hebei Province, China. Currently enrolled as a Ph.D. student at the Institute of High Energy Physics, Chinese Academy of Sciences, majoring in High Energy Astrophysics (Particle Physics and Nuclear Physics), supervised by Prof. XIONG Shaolin. Research interests include the design and development of X/γ-ray astrophysical instru- ments, the observation and analysis of high- energy astrophysical transients, as well as high-energy atmospheric phenomena. E-mail: cwwang@ihep.ac.cn

    Female. Born in January 1999 in Zhumadian, Henan Province, China. Currently enrolled as a Ph.D. student at the Institute of High Energy Physics, Chinese Academy of Sciences, majoring in High Energy Astrophysics (Particle Physics and Nuclear Physics), supervised by Prof. XIONG Shaolin. The main research work is cross-calibration of GECAM satellites and data analysis of peculiar GRBs, including GRB 221009A and GRB 211211A. Research interests include instrumentation, data analysis and theory interpretation of high-energy transients (e.g. GRB, GW, SGR). E-mail: zhangyanqiu@ihep.ac.cn

    Male, born in Feb. 1983 in Fengcheng city of Jiangxi Province, China. Currently working in the Institute of High Energy Physics, Chinese Academy of Sciences as researcher (professor). Proposed the GECAM mission as the Principal Investigator. Participated in other high-energy space telescopes including Insight-HXMT, POLAR, SVOM, POLAR2, etc. Research interests include high energy astrophysics (e.g. GRB, GW, SGR, FRB) and high energy phenomena from the Sun to the Earth (e.g. SFL, TGF, TEB), in terms of instrumentation, observation, data analysis and theory interpretation.E-mail: xiongsl@ihep.ac.cn

  • Received Date: 2024-06-20
    Available Online: 2024-08-05
    Abstract
  • 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.

     

    • 1 https://gcn.nasa.gov/circulars/21520
    2http://gecam.ihep.ac.cn/ grbDataAnalysisSoftware.jhtml
    3https://gcn.nasa.gov/circulars/32751
    4https://www.astronomerstelegram.org/?read=15682
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    • References(14)
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