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

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

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..357..248g&link_type=abstract

The Spitzer Space Telescope: New Views of the Cosmos ASP Conference Series, Volume 357, proceedings of the conference held 9-12

Astronomy and Astrophysics

Astronomy

Scientific paper

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.

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