Electromagnetic Counterparts of Stellar-mass Binary Black Hole Mergers in AGN Accretion Disks: Theoretical Models and Observational Status
astro-ph.HE, astro-ph.CO
Submitted: 2026-09-30
Updated: 2026-09-30
Terminology
Sources
- GWTC-5.0: Population Properties of Merging Compact Binaries
- GWTC-5.0: Observations from the Second Part of the Fourth LIGO-Virgo-KAGRA Observing Run and Updates to the Gravitational-Wave Transient Catalog
- Evidence for additional structure in the effective spin distribution hints at multiple formation pathways in GWTC-5.0
- High-Spin BBH Subpopulation from AGN Accretion
- GW190521 as a black-hole merger coincident with the ZTF19abanrhr flare
- Global simulations of accretion flows onto perturbers embedded in magnetized disks -I. MRI and jet formation in ideal MHD
- Searching for Binary Black Hole Merger Emission in AGN Disks: Optical and Spectroscopic Follow-up of S240413p
- Prospects for the formation of GW231123 from the AGN channel
- Reconstructing the origin of black hole mergers using sparse astrophysical models
- Electromagnetic Follow-up of the Sub-Solar Mass Gravitational Wave Candidate S251112cm: Kilonova Constraints and a Coincident IIb Supernova
- Exploring Hierarchical Merger Scenarios for GW241011 and GW241110
- The Hierarchical Merger Scenario for GW231123
- WFST Follow-up of S251112cm: Searching for an Optical Counterpart to a Subsolar-mass Compact-binary Merger Candidate
- First measurement of the Hubble parameter from bright binary black hole GW190521
- Reversible-jump MCMC reveals binary black hole subpopulations with distinct redshift evolution
- When the black holes align: a subpopulation of aligned massive binary black holes observed via gravitational waves
- Evidence for an accretion-driven subpopulation of black holes in GWTC-5.0
- The Universal Eccentricity Distribution for Dynamical Gravitational-Wave Merger Channels
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