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Jong H. Chow

Researcher at Australian National University

Publications -  255
Citations -  56305

Jong H. Chow is an academic researcher from Australian National University. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 77, co-authored 254 publications receiving 48175 citations. Previous affiliations of Jong H. Chow include Carleton College & University of Sydney.

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GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences

B. P. Abbott, +1144 more
TL;DR: The total background may be detectable with a signal-to-noise-ratio of 3 after 40 months of total observation time, based on the expected timeline for Advanced LIGO and Virgo to reach their design sensitivity.
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Estimating the Contribution of Dynamical Ejecta in the Kilonova Associated with GW170817

B. P. Abbott, +1144 more
TL;DR: In this paper, the mass of the dynamical ejecta can be estimated without a direct electromagnetic observation of the kilonova, using GW measurements and a phenomenological model calibrated to numerical simulations of mergers with dynamical ejecteda.
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Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory

Arnauld Albert, +1990 more
TL;DR: In this paper, the authors search for high-energy neutrinos from the binary neutron star merger in the GeV-EeV energy range using the Antares, IceCube, and Pierre Auger Observatories.
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Search for gravitational waves from binary inspirals in S3 and S4 LIGO data

B. P. Abbott, +463 more
- 07 Mar 2008 - 
TL;DR: In this paper, a search for gravitational waves from the coalescence of compact binary systems during the third and fourth LIGO science runs was reported, which focused on gravitational waves generated during the inspiral phase of the binary evolution.
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Upper limits on gravitational wave emission from 78 radio pulsars

B. P. Abbott, +465 more
- 03 Aug 2007 - 
TL;DR: In this paper, the authors presented upper limits on the gravitational wave emission from 78 radio pulsars based on data from the third and fourth science runs of the LIGO and GEO 600 gravitational wave detectors.