activity
20062026
most citedObserving IMBH-IMBH Binary Coalescences via Gravitational Radiation

93 citations · 94 across the 6 of their papers we have counts for

collaborators

6 papers

gr-qc2026

Gravitational Wave Hyperbolic Catalog: Reanalyzing High-Mass Gravitational Wave Signals Using Hyperbolic Waveforms

Jacob Lange, Danilo Chiaramello, Peter Lott +4

Close hyperbolic encounters between black holes produce distinctive bursts of gravitational radiation with a time-frequency morphology that is qualitatively different from that of…

gr-qc2025

Measuring Eccentricity and Addressing Waveform Systematics in GW231123

Aasim Jan, Sophia Nicolella, Deirdre Shoemaker +1

The gravitational-wave event GW231123_135430 is the heaviest binary black hole system observed by the LIGO--Virgo--KAGRA Collaboration to date, with the initial analysis indicating…

gr-qc2025★ 1 cited

An Implementation to Identify the Properties of Multiple Population of Gravitational Wave Sources

Meesum Qazalbash, Muhammad Zeeshan, Richard O'Shaughnessy

The rapidly increasing sensitivity of gravitational wave detectors is enabling the detection of a growing number of compact binary mergers. These events are crucial for understandi…

gr-qc2025

GW200105: A detailed study of eccentricity in the neutron star-black hole binary

Aasim Jan, Bing-Jyun Tsao, Richard O'Shaughnessy +2

GW200105_162426 is the first neutron star-black hole merger to be confidently confirmed through either gravitational-wave or electromagnetic observations. Although initially analyz…

gr-qc2025

Parameter Estimation with Targeted Eccentric Numerical-Relativity Simulations for GW200208_22 and GW190620

Patricia McMillin, Katelyn J. Wagner, Giuseppe Ficarra +2

We have analyzed LVK gravitational wave events that show some evidence of eccentricity from TEOBResumS modeling parameter estimations and have confronted them independently with fu…

astro-ph2006★ 93 cited

Observing IMBH-IMBH Binary Coalescences via Gravitational Radiation

John M. Fregeau, Shane L. Larson, M. Coleman Miller +2

Recent numerical simulations have suggested the possibility of forming double intermediate mass black holes (IMBHs) via the collisional runaway scenario in young dense star cluster…