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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

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

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

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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