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l-space spectroscopy of the Cosmic Microwave Background with the BOOMERanG experiment

de Bernardis, P., Ade, Peter A. R., Bock, J. J., Bond, J. R., Borrill, J., Boscaleri, A., Coble, K., Contaldi, C. R., Crill, B. P., De Gasperis, G., De Troia, G., Farese, P., Ganga, K., Giacometti, M., Hivon, E., Hristov, V. V., Iacoangeli, A., Jaffe, A. H., Jones, W. C., Lange, A. E., Martinis, L., Masi, S., Mason, P., Mauskopf, Philip Daniel, Melchiorri, A., Natoli, P., Montroy, T., Netterfield, C. B., Pascale, Enzo, Piacentini, F., Pogosyan, D., Polenta, G., Pongetti, F., Prunet, S., Romeo, G., Ruhl, J. E., Scaramuzzi, F. and Vittorio, N. 2002. l-space spectroscopy of the Cosmic Microwave Background with the BOOMERanG experiment. Presented at: 2K1BC Workshop, Valle d'Aosta, Italy, 9-13 July 2001. Published in: De Petris, M. and Gervasi, M. eds. Experimental cosmology at millimetre wavelengths: proceedings of the 2K1BC Workshop, Valle d’Aosta, Italy, 9-13 July 2001. AIP Conference Proceedings , vol. 616. Melville, NY: American Institute of Physics, pp. 3-11. 10.1063/1.1475595

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The BOOMERanG experiment has recently produced detailed maps of the Cosmic Microwave Background, where sub-horizon structures are resolved with good signal to noise ratio. A power spectrum (spherical harmonics) analysis of the maps detects three peaks, at multipoles l=(213+10−13),(541+20−32),(845+12−25). In this paper we discuss the data analysis and the implications of these results for cosmology.

Item Type: Conference or Workshop Item (Paper)
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Publisher: American Institute of Physics
ISBN: 0735400628
Last Modified: 23 Jan 2020 04:02

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