Abstract
Gravitational wave burst high-energy Electromagnetic Counterpart All-sky Monitor (GECAM) is specially designed for detecting high-energy electromagnetic counterpart that generates by the gravitational wave source. GECAM consists of two micro-satellites which make a straight line with the Earth to enlarge the field of view to all-sky. The electromagnetic radiation may distribute in a wide range from radio-wave to high-energy γ-Rays. A novel gamma-ray detector which is made up of the 3 in. LaBr3 crystal and the large area SiPM to detect rays from 6 keV to 2000 keV. The detector performances, include dynamic range, linear response, energy-resolution and uniformity, will be discussed in this paper.
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Acknowledgement
Thanks for supporting by the Key Research Program of Frontier Sciences, CAS, and Grant NO. Y6292690K1.
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Lv, P., Xiong, SL., Sun, XL., Lv, JG. (2018). A Novel Gamma-Ray Detector for GECAM. In: Liu, ZA. (eds) Proceedings of International Conference on Technology and Instrumentation in Particle Physics 2017. TIPP 2017. Springer Proceedings in Physics, vol 212. Springer, Singapore. https://doi.org/10.1007/978-981-13-1313-4_1
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DOI: https://doi.org/10.1007/978-981-13-1313-4_1
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