Extragalactic background light inferred from AEGIS galaxy-SED-type fraction

ADA. DomínguezJRJoel R. PrimackFPF. PradaGRGilmore, Rudy C.SRSomerville, Rachel S.

Instituto de Astrofísica de Andalucía · Universidad de Sevilla · +2 more institutions

Abstract

The extragalactic background light (EBL) is of fundamental importance both for understanding the entire process of galaxy evolution and for γ-ray astronomy, but the overall spectrum of the EBL between 0.1 and 1000 μm has never been determined directly from galaxy spectral energy distribution (SED) observations over a wide redshift range. The evolving, overall spectrum of the EBL is derived here utilizing a novel method based on observations only. This is achieved from the observed evolution of the rest-frame K-band galaxy luminosity function up to redshift 4, combined with a determination of galaxy-SED-type fractions. These are based on fitting Spitzer Wide-Area Infrared Extragalactic Survey (SWIRE) templates…

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630
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Authors

6

Topics & keywords

Keywords
  • Physics
  • Astrophysics
  • Galaxy
  • Astronomy
  • Redshift
  • Luminous infrared galaxy
  • Extragalactic background light
  • Spectral energy distribution
UN Sustainable Development Goals
  • Affordable and clean energy
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