Mid and Far Infrared Surveys with ISO
| dc.creator | Elbaz, David | |
| dc.date | 1999-11-04 | |
| dc.date.accessioned | 2026-07-07T02:34:13Z | |
| dc.date.available | 2026-07-07T02:34:13Z | |
| dc.description | We present the results of the extragalactic surveys performed at 15 and 175 microns using the ISOCAM and ISOPHOT instruments on-board the Infrared Space Observatory (ISO). The number counts at both wavelengths present a strong evolution. The preliminary study of the individual galaxies responsible for this evolution suggest that more star formation was hidden by dust at redshifts around z=1-2 and imply that the population of luminous IR galaxies detected by IRAS in the local universe must have played a major role in the formation and evolution of galaxies and cannot be considered anymore as extreme and rare cases. | |
| dc.description | 10 pages, 4 figures: Proceedings of Rencontres de Moriond, 13-20 March 1999, ``Building Galaxies: from the Primordial Universe to the Present'', ed F. Hammer, T. X. Thuan, V. Cayatte, B. Guiderdoni and J. Tran Thanh Van (Ed. Frontieres) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9911050 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9911050 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/15160 | |
| dc.subject | Astrophysics | |
| dc.title | Mid and Far Infrared Surveys with ISO | |
| dc.type | text |