Galaxy Clustering in Far-Infrared SWIRE Fields

Details Galaxy Clustering in Far-Infrared SWIRE Fields Galaxy Clustering in Far-Infrared SWIRE Fields

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..381..225f&link_type=abstract

The Second Annual Spitzer Science Center Conference: Infrared Diagnostics of Galaxy Evolution. ASP Conference Series, Vol. 381,

Mathematics

Probability

Scientific paper

We present measurements of galaxy clustering detected in the six SWIRE
fields in all MIPS channels at 24, 70, and 160 microns. The measurements
include the low-order 2-point angular correlation functions, and
high-order probes including probability distribution functions and
Rényi information.

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