Universal bolometric corrections for active galactic nuclei over seven luminosity decades

Context. The AGN bolometric correction is a key element for understanding black hole (BH) demographics and computing accurate BH accretion histories from AGN luminosities. However, current estimates still differ from each other by up to a factor of two to three, and rely on extrapolations at the low...

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Detalles Bibliográficos
Autores principales: Duras, F., Bongiorno, A., Ricci, F., Piconcelli, E., Shankar, F., Lusso, E., Bianchi, S., Fiore, F., Maiolino, R., Marconi, A., Onori, F., Sani, E., Schneider, R., Vignali, C., La Franca, F.
Formato: Artículo (Article)
Idioma:Inglés (English)
Publicado: 2025
Materias:
black hole physics
galaxies
active
quasars
supermassive black holes
evolution
fundamental parameters
X-rays
Acceso en línea:https://repositorio.uc.cl/handle/11534/100610

Internet

https://repositorio.uc.cl/handle/11534/100610

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