Oliver, Seb (2006) Large scale structure from SWIRE. In: Meeting on Spitzer Space Telescope - New Views of the Cosmos, Pasadena, California, USA.

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Abstract

We show that the Spitzer Wide-area InfraRed Extragalactic Legacy Survey (SWIRE) will provide the galaxy catalogues that can be used to measure the clustering of galaxies and its evolution for star-forming galaxies and galaxies selected on the basis of their stellar mass. High signal-to-noise measurements will be possible on co-moving scales around 10h(-1)Mpc; out to z similar to 2 - 2.5; after subdividing galaxy samples by factors of 10; or in redshift intervals of Delta z approximate to 0.2.

Item Type:	Conference or Workshop Item (Paper)
Additional Information:	Proceedings of the conference held 9-12 November, 2004.
Schools and Departments:	School of Mathematical and Physical Sciences > Physics and Astronomy
Subjects:	Q Science > QC Physics
Depositing User:	Seb Oliver
Date Deposited:	06 Feb 2012 21:12
Last Modified:	23 Jul 2012 11:50
URI:	http://srodev.sussex.ac.uk/id/eprint/30209

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