Galaxy and AGN Evolution in the MIR: a combined Spitzer and X-ray view
| dc.creator | Gruppioni, C. | |
| dc.creator | Pozzi, F. | |
| dc.creator | Comastri, A. | |
| dc.creator | Vignali, C. | |
| dc.creator | Rodighiero, G. | |
| dc.creator | . | |
| dc.date | 2006-10-24 | |
| dc.date.accessioned | 2026-07-07T07:27:07Z | |
| dc.date.available | 2026-07-07T07:27:07Z | |
| dc.description | A proper analysis of the evolution of sources emitting in the Mid-Infrared is strongly dependent on their broad-band spectral properties (SEDs) at different redshifts and luminosities and on a reliable classification allowing to disentangle AGN from star-formation activity. The diagnostic diagrams based on the optical line ratios are often ambiguous and/or misleading not allowing a proper separation of the galaxy/AGN populations. Thanks to the combination of deep Spitzer and X-rays data a much better census of the hidden AGN activity and dust-obscured star-forming galaxies can be obtained, constraining galaxy and AGN evolutionary models. | |
| dc.description | 4 pages. Proceeding of the conference "Studying Galaxy Evolution with Spitzer and Herschel", Crete, May 28 - June 2, 2006. Eds. V. Charmandaris, D. Rigopoulou, N. Kylafis | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0610711 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0610711 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/117267 | |
| dc.subject | Astrophysics | |
| dc.title | Galaxy and AGN Evolution in the MIR: a combined Spitzer and X-ray view | |
| dc.type | text |