From ISO to SIRTF Cosmological Surveys: Exploring the Cosmic Infrared Background

Details From ISO to SIRTF Cosmological Surveys: Exploring the Cosmic Infrared Background From ISO to SIRTF Cosmological Surveys: Exploring the Cosmic Infrared Background

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..17..248d&link_type=abstract

Galaxy Evolution: Theory & Observations (Eds. Vladimir Avila-Reese, Claudio Firmani, Carlos S. Frenk & Christine Allen) Revista

Mathematics

Logic

Cosmology: Observations, Infrared: Galaxies

Scientific paper

Understanding and observing the sources contributing to the extragalactic background at all wavelengths has become one of the most rapidly evolving fields in observational cosmology since the discovery of the Cosmic Infrared Background (CIB, Puget et al, 1996; Hauser & Dwek, 2000). Cosmological surveys conducted from space with ISO (Infrared Space Observatory) and from the ground in the mm/submm range, together with observations at other wavelengths for source identification, begin to provide a global view of galaxy evolution. In particular, ISO (Genzel & Cesarsky, 2000, Franceschini et al, 2001) performed many deep surveys in the mid and far infrared, mainly at 15 mu m (Elbaz et al, 2002) and at 170 mu m (Dole et al, 2001).

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