Large-Scale Structure in the Spitzer Wide-Area Infrared Extragalactic Survey

Details Large-Scale Structure in the Spitzer Wide-Area Infrared Extragalactic Survey Large-Scale Structure in the Spitzer Wide-Area Infrared Extragalactic Survey

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...207.6349f&link_type=abstract

American Astronomical Society Meeting 207, #63.49; Bulletin of the American Astronomical Society, Vol. 37, p.1255

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We present results of the large-scale structure analysis from the largest of the Spitzer Legacy programs, the Spitzer Wide-Area Infrared Extragalactic Survey (SWIRE). As the widest-area survey using Spitzer covering 50 square degrees, SWIRE provides unprecedented grand view of the galaxies and structures in infrared universe from 3.6 to 160 microns, tracing their evolution to a redshift of 2.5 and beyond. We use a variety of techniques to analyze the spatial distribution of SWIRE galaxies from mid- to far-infrared wavelengths. We discuss our analysis and implications of our results on underlying structures and evolution models from the infrared view.

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