Large-scale structure in the Spitzer wide-area infrared extragalactic survey

Fang, F, Oliver, S, Shupe, D L, Waddington, I, Masci, F, Gonzales-Solares, E, Salaman, D M, Vaccari, M, Surace, J, Lonsdale, C J and SWIRE Team, (2005) Large-scale structure in the Spitzer wide-area infrared extragalactic survey. Bulletin of the American Astronomical Society, 37. p. 1255. ISSN 0002-7537

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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.

Item Type: Article
Schools and Departments: School of Mathematical and Physical Sciences > Physics and Astronomy
Depositing User: Seb Oliver
Date Deposited: 06 Feb 2012 21:28
Last Modified: 22 Oct 2019 14:19
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