Near-infrared background anisotropies from diffuse intrahalo light of galaxies

Asantha Cooray (), Joseph Smidt, Francesco De Bernardis, Yan Gong, Daniel Stern, Matthew L. N. Ashby, Peter R. Eisenhardt, Christopher C. Frazer, Anthony H. Gonzalez, Christopher S. Kochanek, Szymon Kozłowski and Edward L. Wright
Additional contact information
Asantha Cooray: University of California
Joseph Smidt: University of California
Francesco De Bernardis: University of California
Yan Gong: University of California
Daniel Stern: Jet Propulsion Laboratory, California Institute of Technology
Matthew L. N. Ashby: Harvard-Smithsonian Center for Astrophysics, 60 Garden Street
Peter R. Eisenhardt: Jet Propulsion Laboratory, California Institute of Technology
Christopher C. Frazer: University of California
Anthony H. Gonzalez: University of Florida
Christopher S. Kochanek: The Ohio State University
Szymon Kozłowski: The Ohio State University
Edward L. Wright: University of California

Nature, 2012, vol. 490, issue 7421, 514-516

Abstract: Measurements of the anisotropy power spectrum of the cosmic near-infrared background radiation show the clustering amplitude to be larger than existing model predictions involving distant primordial galaxies or nearby faint galaxies: the fluctuations are proposed to originate from intrahalo stars of all galaxies with dark-matter haloes of 109 to 1012 solar masses at redshifts of about 1 to 4.

Date: 2012
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DOI: 10.1038/nature11474

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