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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 ShupeWe 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.
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Publication status
- Published
Publisher
Astronomical Society of the Pacific Conference SeriesPublisher URL
Volume
357Presentation Type
- paper
Event name
The Spitzer Space Telescope: New Views of the Cosmos ASP Conference SeriesEvent location
Pasadena, California, USA.Event type
conferenceEvent date
9-12 November, 2004.Department affiliated with
- Physics and Astronomy Publications
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- No
Peer reviewed?
- Yes
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2012-02-06Usage metrics
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