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A. M. Cruise

Researcher at University of Birmingham

Publications -  163
Citations -  22452

A. M. Cruise is an academic researcher from University of Birmingham. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 65, co-authored 158 publications receiving 19804 citations. Previous affiliations of A. M. Cruise include National Science Foundation & Rutherford Appleton Laboratory.

Papers
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Journal ArticleDOI

Observation of Gravitational Waves from a Binary Black Hole Merger

B. P. Abbott, +1011 more
TL;DR: This is the first direct detection of gravitational waves and the first observation of a binary black hole merger, and these observations demonstrate the existence of binary stellar-mass black hole systems.
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Predictions for the rates of compact binary coalescences observable by ground-based gravitational-wave detectors

J. Abadie, +722 more
TL;DR: In this paper, Kalogera et al. presented an up-to-date summary of the rates for all types of compact binary coalescence sources detectable by the initial and advanced versions of the ground-based gravitational-wave detectors LIGO and Virgo.
Journal ArticleDOI

Predictions for the Rates of Compact Binary Coalescences Observable by Ground-based Gravitational-wave Detectors

J. Abadie, +709 more
TL;DR: In this article, the authors present an up-to-date summary of the rates for all types of compact binary coalescence sources detectable by the Initial and Advanced versions of the ground-based LIGO and Virgo Astrophysical estimates for compact-binary coalescence rates depend on a number of assumptions and unknown model parameters.
Journal ArticleDOI

A gravitational wave observatory operating beyond the quantum shot-noise limit

J. Abadie, +614 more
- 11 Sep 2011 - 
TL;DR: In this paper, the authors demonstrate the squeezed-light enhancement of GEO600, which will be the GW observatory operated by the LIGO Scientific Collaboration in its search for GWs for the next 3-4 years.
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Sub-Femto-g Free Fall for Space-Based Gravitational Wave Observatories: LISA Pathfinder Results

Michele Armano, +118 more
TL;DR: The first results of the LISA Pathfinder in-flight experiment demonstrate that two free-falling reference test masses, such as those needed for a space-based gravitational wave observatory like LISA, can be put in free fall with a relative acceleration noise with a square root of the power spectral density.