arXiv (OAI Expanded)
open access
The Loud Tail of the Supermassive Black Hole Binary Population: Multimessenger Candidates and Prospects for SKAO
cosmology-and-nongalactic-astrophysicsgeneral-relativity-and-quantum-cosmologyhigh-energy-astrophysical-phenomena
We assess whether electromagnetically identified supermassive black hole (SMBH) binary candidates populate the rare, high-amplitude tail of the gravitational wave (GW) amplitude distribution. Using an SMBH binary population model fitted to the NANOGrav 15-year data, we find that 3C~66B and Mrk~501 a
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- GW230814: Investigation of a Loud Gravitational-wave Signal Observed with a Single Detector#386995
- GW230814: Investigation of a Loud Gravitational-wave Signal Observed with a Single Detector#326035
- GW230814: Investigation of a Loud Gravitational-wave Signal Observed with a Single Detector#294015
- Higher-order statistics of the stochastic gravitational wave background from supermassive black hole binaries#1131539
- The Stochastic Siren: Astrophysical Gravitational-Wave Background Measurements of the Hubble Constant#799849
Record · ID 1071159
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive