The IRAC galaxy correlation functions from SWIRE
Abstract
We present an analysis of large-scale structure from the Spitzer Wide-area Infrared Extragalactic legacy survey, SWIRE. The two-point angular correlation functions were computed for galaxies detected in the 3.6-micron IRAC band, on angular scales up to a degree. Significant evolution in the clustering amplitude was detected, as the median redshift of the samples increases from z=0.2 to 0.6. The galaxy clustering in the GALICS semi-analytic models was compared with the observed correlation functions and found to disagree with the data at faint flux limits.
Keywords
Cite
@article{arxiv.astro-ph/0503037,
title = {The IRAC galaxy correlation functions from SWIRE},
author = {Ian Waddington},
journal= {arXiv preprint arXiv:astro-ph/0503037},
year = {2019}
}
Comments
To appear in The Spitzer Space Telescope: New Views of the Cosmos (Pasadena, November 2004), ASP Conference Series, L. Armus et al (eds). 4 pages, 3 figures. V2 includes a reference missing from V1