BLAST: Correlations in the Cosmic Submillimeter Background Reveal Clustering at 250, 350 and 500 μ. Implications for observations with Herschel and Planck.

Details BLAST: Correlations in the Cosmic Submillimeter Background Reveal Clustering at 250, 350 and 500 μ. Implications for observations with Herschel and Planck. BLAST: Correlations in the Cosmic Submillimeter Background Reveal Clustering at 250, 350 and 500 μ. Implications for observations with Herschel and Planck.

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21530606v&link_type=abstract

American Astronomical Society, AAS Meeting #215, #306.06; Bulletin of the American Astronomical Society, Vol. 42, p.304

Astronomy and Astrophysics

Astronomy

Scientific paper

We detect correlations in the cosmic far-infrared background due to the clustering of star-forming galaxies in observations made with the Balloon-borne Large Aperture Submillimeter Telescope, BLAST, at 250, 350, and 500 microns. We discuss the significance of this detection, and implications of this measurement for future planned surveys with Herschel and Planck.

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