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http://dx.doi.org/10.3938/jkps.73.1197

Sensing and Vetoing Loud Transient Noises for the Gravitational-wave Detection  

Jung, Pil-Jong (School of Physics and Chemistry, Gwangju Institute of Science and Technology)
Kim, Keun-Young (School of Physics and Chemistry, Gwangju Institute of Science and Technology)
Oh, John J. (Division of Basic Researches for Industrial Mathematics, National Institute for Mathematical Sciences)
Oh, Sang Hoon (Division of Basic Researches for Industrial Mathematics, National Institute for Mathematical Sciences)
Son, Edwin J. (Division of Basic Researches for Industrial Mathematics, National Institute for Mathematical Sciences)
Kim, Young-Min (School of Natural Science, Ulsan National Institute of Science and Technology)
Publication Information
Journal of the Korean Physical Society / v.73, no.9, 2018 , pp. 1197-1210 More about this Journal
Abstract
Since the first detection of gravitational-wave (GW), GW150914, September 14th 2015, the multi-messenger astronomy added a new way of observing the Universe together with electromagnetic (EM) waves and neutrinos. After two years, GW together with its EM counterpart from binary neutron stars, GW170817 and GRB170817A, has been observed. The detection of GWs opened a new window of astronomy/astrophysics and will be an important messenger to understand the Universe. In this article, we briefly review the gravitational-wave and the astrophysical sources and introduce the basic principle of the laser interferometer as a gravitational-wave detector and its noise sources to understand how the gravitational-waves are detected in the laser interferometer. Finally, we summarize the search algorithms currently used in the gravitational-wave observatories and the detector characterization algorithms used to suppress noises and to monitor data quality in order to improve the reach of the astrophysical searches.
Keywords
Gravitational-wave; Data analysis; Detector characterization;
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