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..
Full text not available from this repository.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) |
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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 |