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Liam Cunningham

Researcher at University of Glasgow

Publications -  196
Citations -  54150

Liam Cunningham is an academic researcher from University of Glasgow. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 74, co-authored 196 publications receiving 43872 citations.

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Model Comparison from LIGO-Virgo Data on GW170817's Binary Components and Consequences for the Merger Remnant

B. P. Abbott, +1280 more
TL;DR: In this paper, the authors perform Bayesian model selection on a wide range of theoretical predictions for the neutron star equation of state, and find that all scenarios from prompt collapse to long-lived or even stable remnants are possible.
Journal ArticleDOI

Improved Analysis of GW150914 Using a Fully Spin-Precessing Waveform Model

B. P. Abbott, +1001 more
- 21 Oct 2016 - 
TL;DR: In this paper, a 15-dimensional precessing-spin waveform model (precessing EOBNR) was developed within the EOB formalism for GW150914.
Journal ArticleDOI

Calibration of the Advanced LIGO detectors for the discovery of the binary black-hole merger GW150914

B. P. Abbott, +719 more
- 28 Mar 2017 - 
TL;DR: In this article, the authors used a dedicated photon radiation pressure actuator, with cross-checks provided by optical and radio frequency references, to validate the model and characterize its uncertainty.
Journal ArticleDOI

Search for gravitational waves associated with gamma-ray bursts during LIGO science run 6 and Virgo science runs 2 and 3

J. Abadie, +807 more
TL;DR: The results of a search for gravitational waves associated with 154 gamma-ray bursts (GRBs) that were detected by satellite-based gamma ray experiments in 2009-2010, during the sixth LIGO science run and the second and third Virgo science runs are presented in this article.
Journal ArticleDOI

Search for gravitational waves from a long-lived remnant of the binary neutron star merger GW170817

B. P. Abbott, +1138 more
TL;DR: In this paper, the authors revisited the binary neutron star coalescence with a focus on longer signal durations up until the end of the Second Advanced LIGO-Virgo Observing run, 8.5 days after the coalescence of GW170817.