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¹Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Am Mühlenberg 1, Potsdam 14476, Germany
²Department of Physics, University of Maryland, College Park, Maryland 20742, USA
³Nikhef, Science Park 105, 1098 XG Amsterdam, The Netherlands
⁴Department of Astronomy and Joint Space-Science Institute, University of Maryland, College Park, Maryland 20742, USA
⁵Max Planck Institute for Intelligent Systems, Max-Planck-Ring 4, 72076 Tübingen, Germany
⁶School of Mathematical Sciences, University of Nottingham, University Park, Nottingham NG7 2RD, United Kingdom
⁷Department of Physics, East Hall, University of Rhode Island, Kingston, Rhode Island 02881, USA
⁸Center for Computational Research, Carothers Library, University of Rhode Island, Kingston, Rhode Island 02881, USA
⁹Department of Applied Mathematics and Theoretical Physics, Cambridge CB3 0WA, United Kingdom
¹⁰Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom

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Articles Citing

Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA

Theory-agnostic searches for non-gravitational modes in black hole ringdown

Neural Post-Einsteinian Test of General Relativity with the Third Gravitational Wave Transient Catalog

Time-domain phenomenological multipolar waveforms for aligned-spin binary black holes in elliptical orbits

Identification and characterization of distorted gravitational waves by lensing using deep learning

Testing modified gravity with the eccentric neutron star-black hole merger GW200105

Adding equatorial-asymmetric effects for spin-precessing binaries into the seobnrv5phm waveform model

Systematic bias due to eccentricity in parameter estimation for merging binary neutron stars: Spinning case

Fast frequency-domain phenomenological modeling of eccentric aligned-spin binary black holes

Spin-precession effects in the phasing formula of eccentric compact binary inspirals up to the second post-Newtonian order

Gravitational waves from the late inspiral, transition, and plunge of small-mass-ratio eccentric binaries

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

Biased parameter inference of eccentric, spin-precessing binary black holes

Orbital eccentricity can make neutron star g -mode resonances observable with current gravitational-wave detectors

Accelerated inference of microlensed gravitational waves with machine learning

Population properties of binary black holes with eccentricity

Test for eccentric binaries based on the spin-induced quadrupole moment

Gravitational-wave signatures of highly eccentric stellar-mass binary black holes in galactic nuclei

Residual test for the third gravitational-wave transient catalog

The Maximum Mass Ratio of Hierarchical Binary Black Hole Mergers May Cause the q–χ eff Correlation

Orbital Eccentricity in a Neutron Star–Black Hole Merger

Gravitational-wave Observations Suggest Most Black Hole Mergers Form in Triples

First Eccentric Inspiral–Merger–Ringdown Analysis of Neutron Star–Black Hole Mergers

Testing the Nature of GW200105 by Probing the Frequency Evolution of Eccentricity

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