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The population properties of spinning black holes using Gravitational-wave Transient Catalog 3
Hui Tong, Shanika Galaudage, Eric Thrane
Binary black holes formed via different pathways are predicted to have distinct spin properties. Measuring these properties with gravitational waves provides an opportunity to unve…
Model exploration in gravitational-wave astronomy with the maximum population likelihood
Ethan Payne, Eric Thrane
Hierarchical Bayesian inference is an essential tool for studying the population properties of compact binaries with gravitational waves. The basic premise is to infer the unknown…
Meet the parents: the progenitor binary for the supermassive black hole candidate in E1821+643
James Paynter, Eric Thrane
The remnants of binary black hole mergers can be given recoil kick velocities up to $5,000\text{ km s$^{-1}$}$ due to anisotropic emission of gravitational waves. E1821+643 is a re…
Self-Supervised Clustering on Image-Subtracted Data with Deep-Embedded Self-Organizing Map
Y. -L. Mong, K. Ackley, T. L. Killestein +45
Developing an effective automatic classifier to separate genuine sources from artifacts is essential for transient follow-ups in wide-field optical surveys. The identification of t…
Do unequal-mass binary black hole systems have larger ? Probing correlations with copulas in gravitational-wave astronomy
Christian Adamcewicz, Eric Thrane
The formation history of binary black hole systems is imprinted on the distribution of their masses, spins, and eccentricity. While much has been learned studying these parameters…
A Rosetta Stone for eccentric gravitational waveform models
Alan M. Knee, Isobel M. Romero-Shaw, Paul D. Lasky +2
Orbital eccentricity is a key signature of dynamical binary black hole formation. The gravitational waves from a coalescing binary contain information about its orbital eccentricit…