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Large scale structure from SWIRE

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posted on 2023-06-08, 09:16 authored by Seb OliverSeb Oliver
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 USA

Publisher URL

Volume

357

Page range

273-274

Presentation Type

  • paper

Event name

Meeting on Spitzer Space Telescope - New Views of the Cosmos

Event location

Pasadena, California, USA

Event type

conference

ISBN

978-1-583812-25-9

Department 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 Reach

Legacy Posted Date

2012-02-06

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