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pro vyhledávání: '"Jia, Mingzhen"'
In the future, the third generation (3G) gravitational wave (GW) detectors, exemplified by the Einstein Telescope (ET), will be operational. The detection rate of GW from binary neutron star (BNS) is expected to reach approximately $10^4$ per year. T
Externí odkaz:
http://arxiv.org/abs/2406.15813
In recent years, much work have studied the use of convolutional neural networks for gravitational-wave detection. However little work pay attention to whether the transient noise can trigger the CNN model or not. In this paper, we study the response
Externí odkaz:
http://arxiv.org/abs/2103.03557
Publikováno v:
SCIENCE CHINA Physics, Mechanics & Astronomy; Dec2024, Vol. 67 Issue 12, p1-17, 17p
Publikováno v:
In Optics Communications 1 March 2020 458
Publikováno v:
In Journal of Solid State Chemistry October 2017 254:132-137
Publikováno v:
In Journal of Alloys and Compounds 5 September 2016 678:109-112
Publikováno v:
In Inorganica Chimica Acta 1 June 2015 432:56-63
Publikováno v:
RSC Advances; 2017, Vol. 7 Issue 42, p26089-26096, 8p
Autor:
Wang, Zhongyu1,2, Li, Yucai1, Li, Hengtao1, Harran, Ismail1, Jia, Mingzhen1, Wang, Hui1, Chen, Yuanzheng1 cyz@calypso.org.cn, Wang, Hongyan1, Wu, Nannan3
Publikováno v:
Journal of Alloys & Compounds. Apr2017, Vol. 702, p132-137. 6p.