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Deirdre Shoemaker

Researcher at Georgia Institute of Technology

Publications -  131
Citations -  6066

Deirdre Shoemaker is an academic researcher from Georgia Institute of Technology. The author has contributed to research in topics: Gravitational wave & Binary black hole. The author has an hindex of 46, co-authored 131 publications receiving 5049 citations. Previous affiliations of Deirdre Shoemaker include Cornell University & University of Texas at Austin.

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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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Introduction to isolated horizons in numerical relativity

TL;DR: In this article, the authors present a coordinate-independent method for extracting the mass and angular momentum of a black hole in numerical simulations, based on the isolated horizon framework, which is applicable both at late times when the black hole has reached equilibrium, and at early times where the black holes are widely separated.
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Gravitational Recoil from Spinning Binary Black Hole Mergers

TL;DR: In this paper, the authors consider the case of black holes with opposite spins of magnitude a aligned and antialigned with the orbital angular momentum, with a dimensionless spin parameter of the individual holes.
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Upper limits on the isotropic gravitational-wave background from Advanced LIGO and Advanced Virgo’s third observing run

Richard J. Abbott, +1681 more
- 15 Jul 2021 - 
TL;DR: In this article, the authors report results of a search for an isotropic gravitational-wave background (GWB) using data from Advanced LIGO's and Advanced Virgo's third observing run (O3) combined with upper limits from the earlier O1 and O2 runs.
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Unequal mass binary black hole plunges and gravitational recoil

TL;DR: In this article, the authors present results from fully nonlinear simulations of unequal mass binary black holes plunging from close separations well inside the innermost stable circular orbit with mass ratios q ≡ M1/M2 = {1, 0.85, 0., 0.78, 0, 55, 0.32}, or equivalently, with reduced mass parameters η ≡ M 1M2/(M 1 + M 2)2 ={0.25, 0..25,0.34, 0.34,