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Dedicated SiPM array for GRD of GECAM

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arxiv 2112.04770 v1 pith:BY63AGUU submitted 2021-12-09 hep-ex astro-ph.IM

Dedicated SiPM array for GRD of GECAM

D.L. Zhang , X.L. Sun , Z.H. An , X.Q. Li , X.Y. Wen , K. Gong , C. Cai , Z. Chang
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G. Chen C. Chen Y.Y. Du M. Gao R. Gao D.Y. Guo J.J. He D.J. Hou Y.G. Li C.Y. Li G. Li L. Li X.F. Li M.S. Li X.H. Liang X.J. Liu Y.Q. Liu F.J. Lu H. Lu B. Meng W.X. Peng F. Shi H. Wang J.Z. Wang Y.S. Wang H.Z. Wang X. Wen S. Xiao S.L. Xiong Y.B. Xu Y.P. Xu S. Yang J.W. Yang Fan Zhang S.N. Zhang C.Y. Zhang C.M. Zhang Fei Zhang X.Y. Zhao X. Zhou
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classification hep-ex astro-ph.IM
keywords gravitationalall-skyburstsgamma-raygecamwavesabilityachieve
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The discovery of gravitational waves and gamma-ray bursts heralds the era of multi-messenger astronomy. With the adoption of two small satellites to achieve the all-sky monitoring of gamma-ray bursts, the gravitational wave high-energy electromagnetic counterpart all-sky monitor (GECAM) possesses a quasi-real-time early warning ability and plays an important role in positioning the sources of gravitational waves and in subsequent observations.

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