González-Solares, E. A., Waddington, I, Oliver, S, Rowan-Robinson, M, Vaccari, M, Masci, F, Lonsdale, C, Surace, J, Fang, F and Shupe, D (2006) Angular correlation of 3.6 and 24 micron galaxies in the SWIRE N1 field. In: The Spitzer Space Telescope: New Views of the Cosmos ASP Conference Series, 9-12 November, 2004., Pasadena, California, USA..

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Abstract

We report the first calculation of the angular cross correlation function of 3.6 and 24μm galaxies detected in the SWIRE survey. We have selected a volume limited sample of luminous galaxies based on photometric redshifts. Their angular auto-correlation function show that their clustering is larger than the full sample of galaxies. While the auto-correlation functions of 3.6 and 24μm sources are similar, their cross correlation function shows an excess of galaxy-galaxy pairs at distances larger than 20 arcmin.

Item Type:	Conference or Workshop Item (Paper)
Schools and Departments:	School of Mathematical and Physical Sciences > Physics and Astronomy
Depositing User:	Seb Oliver
Date Deposited:	06 Feb 2012 21:11
Last Modified:	04 Apr 2012 15:54
URI:	http://sro.sussex.ac.uk/id/eprint/30089

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