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Large scale structure from SWIRE
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.
History
Publication status
- Published
Publisher
ASTRONOMICAL SOC PACIFIC, 390 ASHTON AVE, SAN FRANCISCO, CA 94112 USAPublisher URL
Volume
357Page range
273-274Presentation Type
- paper
Event name
Meeting on Spitzer Space Telescope - New Views of the CosmosEvent location
Pasadena, California, USAEvent type
conferenceISBN
978-1-583812-25-9Department affiliated with
- Physics and Astronomy Publications
Notes
Proceedings of the conference held 9-12 November, 2004.Full text available
- No
Peer reviewed?
- Yes
Editors
L Armus, WT ReachLegacy Posted Date
2012-02-06Usage metrics
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