학술논문
Dedicated SiPM array for GRD of GECAM
Document Type
Working Paper
Author
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.
Source
Subject
Language
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.