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Angular correlation of 3.6 and 24 micron galaxies in the SWIRE N1 field.

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posted on 2023-06-08, 09:11 authored by E. A. González-Solares, I Waddington, Seb OliverSeb Oliver, M Rowan-Robinson, M Vaccari, F Masci, C Lonsdale, J Surace, F Fang, D Shupe
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.

History

Publication status

  • Published

Publisher

Astronomical Society of the Pacific Conference Series

Publisher URL

Volume

357

Presentation Type

  • paper

Event name

The Spitzer Space Telescope: New Views of the Cosmos ASP Conference Series

Event location

Pasadena, California, USA.

Event type

conference

Event date

9-12 November, 2004.

Department affiliated with

  • Physics and Astronomy Publications

Full text available

  • No

Peer reviewed?

  • Yes

Legacy Posted Date

2012-02-06

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