Infrared Number Counts of AGN in the GOODS Fields
| dc.creator | Treister, E. | |
| dc.creator | Urry, C. Megan | |
| dc.creator | Team, the GOODS AGN | |
| dc.date | 2005-03-02 | |
| dc.date.accessioned | 2026-07-07T02:17:08Z | |
| dc.date.available | 2026-07-07T02:17:08Z | |
| dc.description | Using the known numbers and evolution of unobscured AGN, and assuming that there is a large number of corresponding obscured AGN -- as expected if AGN unification is correct -- we predict the infrared number counts of AGN. These agree well with the observed GOODS Spitzer data at 3.6, 8 and 24 $μ$m, provided that the dust content of the obscuring torus is $\sim 2$x less than assumed. This strongly supports the AGN unification picture, and implies a large population of infrared bright obscured AGN at all redshifts and luminosities. | |
| dc.description | To appear in the conference proceedings for Spitzer New Views of the Universe, held Nov. 2004 in Pasadena, CA | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0503057 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0503057 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/9059 | |
| dc.subject | Astrophysics | |
| dc.title | Infrared Number Counts of AGN in the GOODS Fields | |
| dc.type | text |