papers

Publications (20)

gr-qc2026

Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset

Cailin Plunkett, Thomas Callister, Michael Zevin +1

Repeated black-hole mergers in dense stellar clusters are a plausible mechanism to populate the predicted gap in black hole masses due to the pair-instability supernova process. Th…

astro-ph.IM2019

The US Program in Ground-Based Gravitational Wave Science: Contribution from the LIGO Laboratory

David Reitze, Rich Abbott, Carl Adams +181

Recent gravitational-wave observations from the LIGO and Virgo observatories have brought a sense of great excitement to scientists and citizens the world over. Since September 201…

astro-ph.HE2025

No evidence that the binary black hole mass distribution evolves with redshift

Max Lalleman, Kevin Turbang, Thomas Callister +1

The mass distribution of merging binary black holes is generically predicted to evolve with redshift, reflecting systematic changes in their astrophysical environment, stellar prog…

astro-ph.HE2020

Joint constraints on the field-cluster mixing fraction, common envelope efficiency, and globular cluster radii from a population of binary hole mergers via deep learning

Kaze W. K. Wong, Katelyn Breivik, Kyle Kremer +1

The recent release of the second Gravitational-Wave Transient Catalog (GWTC-2) has increased significantly the number of known GW events, enabling unprecedented constraints on form…

astro-ph.HE2020

Shouts and Murmurs: Combining Individual Gravitational-Wave Sources with the Stochastic Background to Measure the History of Binary Black Hole Mergers

Thomas Callister, Maya Fishbach, Daniel Holz +1

One of the goals of gravitational-wave astronomy is to quantify the evolution of the compact binary merger rate with redshift. The redshift distribution of black hole mergers would…

astro-ph.CO2026

The Stochastic Siren: Astrophysical Gravitational-Wave Background Measurements of the Hubble Constant

Bryce Cousins, Kristen Schumacher, Adrian Ka-Wai Chung +4

We report the first measurement of the Hubble constant using the stochastic gravitational-wave background arising from binary black hole mergers. This astrophysical backgroun…