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Masashi Ohkawa

Researcher at Niigata University

Publications -  166
Citations -  5484

Masashi Ohkawa is an academic researcher from Niigata University. The author has contributed to research in topics: Laser & Gravitational wave. The author has an hindex of 23, co-authored 165 publications receiving 3504 citations. Previous affiliations of Masashi Ohkawa include University of Central Florida.

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

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

B. P. Abbott, +1318 more
TL;DR: In this paper, the authors present the current best estimate of the plausible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA detectors over the next several years, with the intention of providing information to facilitate planning for multi-messenger astronomy with gravitational waves.
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Observation of Gravitational Waves from Two Neutron Star–Black Hole Coalescences

Richard J. Abbott, +1695 more
TL;DR: In this article, the authors reported the observation of gravitational waves from two compact binary coalescences in LIGO's and Virgo's third observing run with properties consistent with neutron star-black hole (NSBH) binaries.
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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.