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Paper: Angular correlation of 3.6 and 24 micron galaxies in the SWIRE N1 field
Volume: 357, The Spitzer Space Telescope: New Views of the Cosmos
Page: 248
Authors: Gonzalez-Solares, E.A.; Waddington, I.; Oliver, S.; Rowan-Robinson, M.; Vaccari, M.; Masci, F.; Lonsdale, C.; Surace, J.; Fang, F.; Shupe, D.
Abstract: We report the first calculation of the angular cross correlation function of and 3.6; 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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