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| Paper: |
Large Scale Structure from SWIRE |
| Volume: |
357, The Spitzer Space Telescope: New Views of the Cosmos |
| Page: |
273 |
| Authors: |
Oliver, S.; the SWIRE Team |
| 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−1Mpc; out to z ∼ 2−2.5; after subdividing galaxy samples by factors of 10; or in redshift intervals of Δz ≈ 0.2. |
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