Power Spectrum of Cosmic Infrared Background Anisotropies

Details Power Spectrum of Cosmic Infrared Background Anisotropies Power Spectrum of Cosmic Infrared Background Anisotropies

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21724320p&link_type=abstract

American Astronomical Society, AAS Meeting #217, #243.20; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

Studies of both correlations in the spatial distribution of infrared galaxies as a function of redshift and individual high redshift infrared-luminous galaxies are essential to understanding galaxy formation and evolution. Due to confusion at far-infrared and sub-millimeter wavelengths, these correlations must be searched for in the anisotropies of the Cosmic Infrared Background. We present Planck measurements of the CIBA power spectrum, and interpret the results in terms of large-scale bias and clustering of star-forming galaxies.

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