Dedicated SiPM array for GRD of GECAM

Authors :: Zhang, D. L.
Sun, X. L.
An, Z. H.
Li, X. Q.
Wen, X. Y.
Gong, K.
Cai, C.
Chang, Z.
Chen, G.
Chen, C.
Du, Y. Y.
Gao, M.
Gao, R.
Guo, D. Y.
He, J. J.
Hou, D. J.
Li, Y. G.
Li, C. Y.
Li, G.
Li, L.
Li, X. F.
Li, M. S.
Liang, X. H.
Liu, X. J.
Liu, Y. Q.
Lu, F. J.
Lu, H.
Meng, B.
Peng, W. X.
Shi, F.
Wang, H.
Wang, J. Z.
Wang, Y. S.
Wang, H. Z.
Wen, X.
Xiao, S.
Xiong, S. L.
Xu, Y. B.
Xu, Y. P.
Yang, S.
Yang, J. W.
Zhang, Fan
Zhang, S. N.
Zhang, C. Y.
Zhang, C. M.
Zhang, Fei
Zhao, X. Y.
Zhou, X.
Publication Year :: 2021
Abstract: 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.

Subjects :: High Energy Physics - Experiment
Astrophysics - Instrumentation and Methods for Astrophysics

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