Testing the AGN models for the X-ray background

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dc.creatorGilli, R.
dc.date2000-07-14
dc.date.accessioned2026-07-07T01:54:24Z
dc.date.available2026-07-07T01:54:24Z
dc.descriptionWe will briefly examine the following three issues related to the AGN synthesis models for X-ray background: 1) the possibility that absorbed AGNs evolve faster than unabsorbed ones; 2) the existence of the still debated population of luminous absorbed AGNs, the so-called QSO2s; 3) the behavior of the AGN density at a redshift above ~3.
dc.description3 pages, 2 figures, to appear in the Proceedings of the 4th Italian Conference on AGNs, Mem SAIt
dc.identifierhttps://arxiv.org/abs/astro-ph/0007207
dc.identifierhttp://arxiv.org/abs/astro-ph/0007207
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1334
dc.subjectAstrophysics
dc.titleTesting the AGN models for the X-ray background
dc.typetext

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