Evolution of the dusty infrared luminosity function from z=0 to z=2.3 using observations from Spitzer

Details Evolution of the dusty infrared luminosity function from z=0 to z=2.3 using observations from Spitzer Evolution of the dusty infrared luminosity function from z=0 to z=2.3 using observations from Spitzer

2011-01-12

arxiv.org/abs/1101.2467v1

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

19 pages, 14 figures. Accepted for publication in A&A. Online catalog at CDS soon

Scientific paper

We derive the evolution of the infrared (IR) luminosity function (LF) over the last 4/5ths of cosmic time, using deep 24um and 70um imaging of the GOODS North and South fields. We use an extraction technique based on prior source positions at shorter wavelengths to build the 24 and 70um source catalogs. The majority (93%) of the sources have a spectroscopic (39%) or a photometric redshift (54%) and, in our redshift range of interest (i.e., 1.3

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