• 저자B. P. Abbottt el al,C. Adams,F. Acernese,K. Ackley,M. R. Abernathy,R. Abbott,T. D. Abbott,김환선,손재주,오상훈,오정근
• 학술지Living Reviews in Relativity (1433-8351), 21:3, 1 ~ 57
• 등재유형SCIE
• 게재일자 20181201

We present possible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next decade, with the intention of providing information to the astronomy community to facilitate planning for multi-messenger astronomy with gravitational waves. We estimate the sensitivity of the network to transient gravitational-wave signals, and study the capability of the network to determine the sky location of the source. We report our findings for gravitational-wave transients, with particular focus on gravitational-wave signals from the inspiral of binary neutron star systems, which are the most promising targets for multi-messenger astronomy. The ability to localize the sources of the detected signals depends on the geographical distribution of the detectors and their relative sensitivity, and 90% credible regions can be as large as thousands of square degrees when only two sensitive detectors are operational. Determining the sky position of a sign