Published 2008
| Published
Book Section - Chapter
Open
Galaxy Clustering in Far-Infrared SWIRE Fields
Chicago
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
Files
Fang2008p8538Second_Annual_Spitzer_Science_Center_Conference_Infrared_Diagnostics_Of_Galaxy_Evolution.pdf
Files
(260.5 kB)
Name | Size | Download all |
---|---|---|
md5:14d24bc6f3c45bf2a8c2a65129b29258
|
260.5 kB | Preview Download |
Additional details
- Eprint ID
- 19153
- Resolver ID
- CaltechAUTHORS:20100722-084750681
- NASA
- 1407
- 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