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¹Mathematical Sciences and STAG Research Centre, University of Southampton, Southampton, SO17 1BJ, United Kingdom
²Theoretical Astrophysics Group, California Institute of Technology, Pasadena, California 91125, USA
³Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth, United Kingdom
⁴School of Physics and Astronomy, Cardiff University, Cardiff, CF24 3AA, United Kingdom

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Articles Citing

Use and interpretation of signal-model indistinguishability measures for gravitational-wave astronomy

GW231123 ringdown: Interpretation as multimodal Kerr signal

Inspiral tests of general relativity and waveform geometry

Difference between quark stars and neutron stars in universal relations and their effect on gravitational waves

Uncovering subdominant multipole asymmetries in binary black-hole mergers

Post-Newtonian inspiral waveform model for eccentric precessing binaries with higher-order modes and matter effects

Horizon absorption in eccentric precessing binary black hole inspirals and its importance for gravitational wave data analysis

Lessons from binary dynamics of inspiralling equal-mass boson-star mergers

Angular momentum tail contributions to compact binary dynamics

High-mass-ratio challenge in gravitational waveform modeling

Fast neural network surrogate for multimodal effective-one-body gravitational waveforms from generically precessing compact binaries

Revisiting the coprecessing frame in the presence of orbital eccentricity

Eccentric and unbound compact binaries in the LIGO-Virgo-KAGRA catalog: Parameter estimation and waveform systematics with seobnrv6ehm

Lense-Thirring precession modulates repeated lensing of continuous gravitational wave sources in AGN disks

Estimating the lensing probability for binary black hole mergers in AGN discs by using mismatch thresholds

Improved gravitational wave model linking precessing inspirals and numerical-relativity-calibrated merger-ringdown

Strong-field gravitational-wave lensing in the Kerr background

Comprehensive look into the accuracy of spectral Einstein code binary black hole waveforms

Accuracy of ringdown models calibrated to numerical relativity simulations

Eccentricity in disguise? Insights from GW231123 and numerically simulated binary black hole merger signals

Reconsidering the consistent use of precessing, higher order multipole models for gravitational wave analyses

Environmental Effects in Stellar-mass Gravitational-wave Sources. II. Enhanced Detectability of Phase Shifts in Eccentric Subpopulations

Gravitational memory contributions to waveform and effective action

Spherical inspirals of spinning bodies into Kerr black holes

GW231123: A Binary Black Hole Merger with Total Mass 190–265 M ⊙

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