천문학회보 (The Bulletin of The Korean Astronomical Society)
- 제39권1호
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- Pages.79.2-79.2
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- 2014
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- 1226-2692(pISSN)
Identification of Electromagnetic Signal from GW Sources
초록
A few years from now, gravitational wave (GW) detectors of LIGO and VIRGO consortiums are expected to reach the sensitivity necessary to detect GW signals from astronomical sources. Identification of the counterparts to the GW sources in electromagnetic wave is very important, since the localization of the GW signals is going to be very poor (~1000
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