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

Viero, M. P., Ade, Peter A. R. ORCID: https://orcid.org/0000-0002-5127-0401, Bock, J., Chapin, E., Devlin, M., Griffin, Matthew Joseph ORCID: https://orcid.org/0000-0002-0033-177X, Gundersen, J., Halpern, M., Hargrave, Peter ORCID: https://orcid.org/0000-0002-3109-6629, Hughes, D., Klein, J., MacTavish, C., Marsden, G., Martin, P., Mauskopf, Philip Daniel ORCID: https://orcid.org/0000-0001-6397-5516, Monchelsi, L., Negrello, M., Netterfield, C., Olmi, L., Pascale, Enzo ORCID: https://orcid.org/0000-0002-3242-8154, Patanchon, G. and Rex, M. 2010. BLAST: Correlations in the Cosmic Submillimeter Background Reveal Clustering at 250, 350 and 500 μ. Implications for observations with Herschel and Planck. Presented at: 215th Meeting of the American Astronomical Society, Washington, USA, Bulletin of the American Astronomical Society,

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Abstract

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.

Item Type:	Conference or Workshop Item (Paper)
Schools:	Physics and Astronomy
Publisher:	Bulletin of the American Astronomical Society
Last Modified:	18 Oct 2022 13:42
URI:	https://orca.cardiff.ac.uk/id/eprint/14950

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