Multimessenger Probes of the Supermassive Black Hole Binary Population: The Role of Pulsar Timing Arrays

By inferring the gravitational wave background from a population of supermassive black hole binaries (SMBHBs), pulsar timing arrays (PTAs) enable the study of massive black holes. In many ways, PTAs manifest the promise of a multimessenger approach to astronomy: they can constrain SMBHB population c...

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Hlavní autoři:	Nima Laal, Stephen R. Taylor, Cayenne Matt, Kayhan Gültekin
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2026-01-01
Edice:	The Astrophysical Journal
Témata:	Supermassive black holes Gravitational wave sources Bayesian statistics Gravitational wave detectors Gravitational wave astronomy
On-line přístup:	https://doi.org/10.3847/1538-4357/ae6cea
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