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Motoyuki Saijo

Researcher at Waseda University

Publications -  54
Citations -  3995

Motoyuki Saijo is an academic researcher from Waseda University. The author has contributed to research in topics: Gravitational wave & Instability. The author has an hindex of 25, co-authored 54 publications receiving 3072 citations. Previous affiliations of Motoyuki Saijo include Kyoto University & University of Southampton.

Papers
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Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA

B. P. Abbott, +1138 more
TL;DR: In this article, the authors 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.
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The Japanese space gravitational wave antenna DECIGO

Seiji Kawamura, +144 more
Journal ArticleDOI

The Japanese space gravitational wave antenna?DECIGO

Seiji Kawamura, +131 more
TL;DR: DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) as discussed by the authors is the future Japanese space gravitational wave antenna, which aims at detecting various kinds of gravitational waves between 1 mHz and 100 Hz frequently enough to open a new window of observation for gravitational wave astronomy.
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KAGRA: 2.5 Generation Interferometric Gravitational Wave Detector

Tomotada Akutsu, +202 more
- 01 Jan 2019 - 
TL;DR: KAGRA as discussed by the authors is a 2.5-generation GW detector with two 3'km baseline arms arranged in an 'L' shape, similar to the second generations of Advanced LIGO and Advanced Virgo, but it will be operating at cryogenic temperatures with sapphire mirrors.
Journal Article

Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA

B. P. Abbott, +1101 more
TL;DR: The sensitivity of the LIGO network to transient gravitational-wave signals is estimated, and the capability of the network to determine the sky location of the source is studied, to facilitate planning for multi-messenger astronomy with gravitational waves.