The IRAC galaxy correlation functions from SWIRE

Details The IRAC galaxy correlation functions from SWIRE The IRAC galaxy correlation functions from SWIRE

2005-03-02

arxiv.org/abs/astro-ph/0503037v2

Astronomy and Astrophysics

Astrophysics

To appear in The Spitzer Space Telescope: New Views of the Cosmos (Pasadena, November 2004), ASP Conference Series, L. Armus e

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

The IRAC galaxy correlation functions from SWIRE does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The IRAC galaxy correlation functions from SWIRE, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The IRAC galaxy correlation functions from SWIRE will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-284687