The Submm Extragalactic Background. Star formation history of the Universe

Abstract

The recently discovered Submillimeter Extragalactic Background (submm EB) has opened new perspectives on our understanding of galaxy evolution. We detail in this paper one of the major cosmological consequences of this discovery, the submm luminosity density history of the Universe.

4 pages. To appear in "Astronomy and Space Science"

References in corpus (1)

• Resolving the Submillimeter Background: the 850-micron Galaxy Counts

Cited by in corpus (9)

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• HerMES: SPIRE galaxy number counts at 250, 350 and 500 microns
• Deep Extragalactic Surveys around the Ecliptic Poles with AKARI (ASTRO-F)
• FIRBACK: III. Catalog, Source counts, and cosmological implications of the 170 micron ISO Deep survey
• A multi-wavelength de-blended Herschel view of the statistical properties of dusty star-forming galaxies across cosmic time
• Redshift Distribution of Extragalactic 24 micron Sources
• The co-evolution of black hole growth and star formation from a cross-correlation analysis between quasars and the cosmic infrared background
• The Herschel Virgo Cluster Survey. XVII. SPIRE point-source catalogs and number counts
• Microwave and radio emission of dusty star-forming galaxies: Implication for the cosmic radio background