Witnessing Galaxy-SMBH Co-Evolution at Redshift ~ 2
| dc.creator | Renzini, Alvio | |
| dc.creator | Daddi, Emanuele | |
| dc.date | 2008-04-01 | |
| dc.date | 2008-04-02 | |
| dc.date.accessioned | 2026-07-07T09:29:38Z | |
| dc.date.available | 2026-07-07T09:29:38Z | |
| dc.description | In a recent multiwavelength study of galaxies at redshift ~ 2 by Daddi et al. (2007a,b) it is shown that galaxies with a Mid-IR excess most likely harbor a Compton-thick AGN, thus bringing to about 1/3 the fraction of z ~ 2 galaxies hosting an AGN. This finding opens a number of intriguing issues concerning the concomitant growth of galaxies and supermassive black holes, AGN feedback, and downsizing, at the cosmic epoch of most intense star formation and nuclear activity. | |
| dc.description | 6 pages, 5 figures, to appear on the proceedings of the conference "Panoramic Views of Galaxy Formation and Evolution", Hayama, Japan, December 11-16, 2007; Ed. Tadayuki Kodama, ASP Conf. Ser. New version (v2) with figure numbering corrected | |
| dc.identifier | https://arxiv.org/abs/0804.0094 | |
| dc.identifier | http://arxiv.org/abs/0804.0094 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/157858 | |
| dc.subject | Astrophysics | |
| dc.title | Witnessing Galaxy-SMBH Co-Evolution at Redshift ~ 2 | |
| dc.type | text |