Coherence of Supermassive Black Hole Binary Demographics with the nHz Stochastic Gravitational-wave Background
We present a refined estimation of the stochastic gravitational-wave background (SGWB) based on observed dual active galactic nuclei (AGNs) together with AGN X-ray luminosity functions, in light of recent Pulsar Timing Array (PTA) detections of an nHz SGWB. We identify a characteristic luminosity de...
Guardat en:
| Autors principals: | , , |
|---|---|
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
IOP Publishing
2026-01-01
|
| Col·lecció: | The Astrophysical Journal |
| Matèries: | |
| Accés en línia: | https://doi.org/10.3847/1538-4357/ae3962 |
| Etiquetes: |
Sense etiquetes, Sigues el primer a etiquetar aquest registre!
|