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The Astrophysical Journal, 734:40 (11pp), 2011 June 10 doi:10.1088/0004-637X/734/1/40 C 2011. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
 

Summary: The Astrophysical Journal, 734:40 (11pp), 2011 June 10 doi:10.1088/0004-637X/734/1/40
C 2011. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
THE MID-INFRARED LUMINOSITY FUNCTION AT z < 0.3 FROM 5MUSES: UNDERSTANDING THE STAR
FORMATION/ACTIVE GALACTIC NUCLEUS BALANCE FROM A SPECTROSCOPIC VIEW
Yanling Wu1
, Yong Shi1
, George Helou1
, Lee Armus2
, Daniel A. Dale3
, Casey Papovich4
, Nurur Rahman5
,
Kalliopi Dasyra6
, and Sabrina Stierwalt2
1 Infrared Processing and Analysis Center, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA;
yanling@ipac.caltech.edu, yong@ipac.caltech.edu, gxh@ipac.caltech.edu
2 Spitzer Science Center, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA;
lee@ipac.caltech.edu, sabrina@ipac.caltech.edu
3 Department of Physics & Astronomy, University of Wyoming, WY, USA; ddale@uwyo.edu
4 George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Department of Physics and Astronomy,

  

Source: Adolphs, Ralph - Psychology and Neuroscience, California Institute of Technology

 

Collections: Biology and Medicine