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G. D. Meadors

Researcher at Monash University

Publications -  184
Citations -  65748

G. D. Meadors is an academic researcher from Monash University. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 84, co-authored 180 publications receiving 52660 citations. Previous affiliations of G. D. Meadors include Max Planck Society & Albert Einstein Institution.

Papers
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Tests of General Relativity with GW170817

B. P. Abbott, +1240 more
TL;DR: In this paper, the authors place constraints on the dipole radiation and possible deviations from GR in the post-Newtonian coefficients that govern the inspiral regime of a binary neutron star inspiral.
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Bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy

TL;DR: Bilby as mentioned in this paper is a user-friendly Bayesian inference library for gravitational-wave astronomy, which provides expert-level parameter estimation infrastructure with straightforward syntax and tools that facilitate use by beginners.
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GW150914: First results from the search for binary black hole coalescence with Advanced LIGO

B. P. Abbott, +980 more
- 07 Jun 2016 - 
TL;DR: In this paper, the results of a matched-filter search using relativistic models of compact-object binaries that recovered GW150914 as the most significant event during the coincident observations between the two LIGO detectors were reported.
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The Rate of Binary Black Hole Mergers Inferred from Advanced LIGO Observations Surrounding GW150914

B. P. Abbott, +961 more
TL;DR: In this paper, the authors report on the constraints these observations place on the rate of binary black hole coalescences, and estimate a 90% credible range of merger rates between $2$--$53 \, \mathrm{Gpc}^{-3} \mathm{yr}^{ −1}$ (comoving frame).
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Properties and astrophysical implications of the 150 Msun binary black hole merger GW190521.

R. Abbott, +1254 more
TL;DR: The GW190521 signal as mentioned in this paper is consistent with a binary black hole merger source at redshift 0.8 with unusually high component masses, and shows mild evidence for spin-induced orbital precession.