Published 2008
| Published
Book Section - Chapter
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Galaxy Clustering in Far-Infrared SWIRE Fields
Abstract
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.
Additional Information
© 2008 Astronomical Society of the Pacific. Support for this work was provided by NASA through the Jet Propulsion Laboratory, California Institute of Technology under NASA contract 1407.Attached Files
Published - Fang2008p8538Second_Annual_Spitzer_Science_Center_Conference_Infrared_Diagnostics_Of_Galaxy_Evolution.pdf
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Additional details
- Eprint ID
- 19153
- Resolver ID
- CaltechAUTHORS:20100722-084750681
- 1407
- NASA
- Created
-
2010-08-02Created from EPrint's datestamp field
- Updated
-
2020-09-30Created from EPrint's last_modified field
- Caltech groups
- Infrared Processing and Analysis Center (IPAC)
- Series Name
- ASP Conference Series