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F. Fang (IPAC/SSC), S. Oliver (University of Sussex), D. L. Shupe (IPAC/SSC), I. Waddington (University of Sussex), F. Masci (SSC), E. Gonzales-Solares (University of Cambridge), D. M. Salaman (University of Sussex), M. Vaccari (Imperial College), J. Surace (IPAC/SSC), C. J. Lonsdale (IPAC), SWIRE Team
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.
The author(s) of this abstract have provided an email address for comments about the abstract: fan@ipac.caltech.edu
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Bulletin of the American Astronomical Society, 37 #4
© 2005. The American Astronomical Soceity.