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Foregrounds in the BOOMERANG-LDB data: a preliminary rms analysis

Masi, S., Ade, Peter A. R., Bock, J., Boscaleri, A., Crill, B. P., de Bernardis, P., Ganga, K., Giacometti, M., Hivon, E., Hristov, V. V., Lange, A. E., Martinis, L., Mauskopf, Philip Daniel, Montroy, T., Netterfield, v, Pascale, Enzo, Piacentini, F., Prunet, S. and Romeo, G. 2002. Foregrounds in the BOOMERANG-LDB data: a preliminary rms analysis. Presented at: Energy Densities in the Universe, Les Arcs, France, 22-29 January 2000. Published in: Van Tran, J. Thanh, Ansari, R. and Giraud-Héraud, Y . eds. Energy densities in the universe : proceedings of the XXXVth Rencontres de Moriond, Les Arcs, Savoie France, January 22-29, 2000. Moriond workshops (Series) Vietnam: Thê' Giói Publishers,

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Abstract

We present a preliminary analysis of the BOOMERanG LDB maps, focused on foregrounds. BOOMERanG detects dust emission at moderately low galactic latitudes (b>−20 o ) in bands centered at 90, 150, 240, 410 GHz. At higher Galactic latitudes, we use the BOOMERanG data to set conservative upper limits on the level of contamination at 90 and 150 GHz. We find that the mean square signal correlated with the IRAS/DIRBE dust template is less than 3% of the mean square signal due to CMB anisotropy.

Item Type: Conference or Workshop Item (Paper)
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Publisher: Thê' Giói Publishers
Last Modified: 20 Dec 2017 01:47
URI: http://orca-mwe.cf.ac.uk/id/eprint/64585

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