collaborators

8 papers

astro-ph.IM2026

A Foundation for Gravitational-Wave Population Inference within the LISA Global Fit

Alexander W. Criswell, Sharan Banagiri, Vera Delfavero +3

Population inference in gravitational-wave astronomy allows us to connect individual detections to the astrophysics of compact objects and their environments. Current approaches em…

astro-ph.HE2026

McFACTS. IV. Electromagnetic Counterparts to AGN-disk-embedded Binary Black Hole Mergers

Emily McPike, Rosalba Perna, K. E. Saavik Ford +10

The accretion disks of active galactic nuclei (AGNs) are promising environments for producing binary black hole (BBH) mergers, which have been detected via gravitational waves (GWs…

astro-ph.HE2025

McFACTS II: Mass Ratio--Effective Spin Relationship of Black Hole Mergers in the AGN Channel

Harrison E. Cook, Barry McKernan, K. E. Saavik Ford +6

We use the Monte Carlo For AGN (active galactic nucleus) Channel Testing and Simulation (McFACTS, https://www.github.com/mcfacts/mcfacts) code to study the effect of AGN disk and n…

gr-qc2025

Prospects for the formation of GW231123 from the AGN channel

V. Delfavero, S. Ray, H. E. Cook +6

The recent binary black hole (BBH) merger GW231123 consisted of the merger of two intermediate mass black holes (IMBH) which appear to have large spin magnitudes. Active galactic n…

astro-ph.HE2025

McFACTS I: Testing the LVK AGN channel with Monte Carlo For AGN Channel Testing & Simulation (McFACTS)

Barry McKernan, K. E. Saavik Ford, Harrison E. Cook +6

Active galactic nuclei (AGN) are a promising source of the binary black hole (BBH) mergers observed in gravitational waves with LIGO-Virgo-Kagra (LVK). Constraining the AGN channel…

astro-ph.HE2025

McFacts III: Compact binary mergers from AGN disks over an entire synthetic universe

Vera Delfavero, K. E. Saavik Ford, Barry McKernan +6

The Active Galactic Nuclei (AGN) channel for the formation of binary black hole (BBH) mergers has been previously studied as a potential formation channel for the merging compact b…