dc.contributor.author |
Netterfield, C. B. |
en_US |
dc.contributor.author |
Ade, P. A. R. |
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dc.contributor.author |
Bock, J. J. |
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dc.contributor.author |
Bond, J. R. |
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dc.contributor.author |
Borrill, J. |
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dc.contributor.author |
Boscaleri, A. |
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dc.contributor.author |
Coble, K. |
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dc.contributor.author |
Contaldi, C. R. |
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dc.contributor.author |
Crill, B. P. |
en_US |
dc.contributor.author |
Bernardis, P. de |
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dc.contributor.author |
Farese, P. |
en_US |
dc.contributor.author |
Ganga, K. |
en_US |
dc.contributor.author |
Giacometti, M. |
en_US |
dc.contributor.author |
Hivon, E. |
en_US |
dc.contributor.author |
Hristov, V. V. |
en_US |
dc.contributor.author |
Iacoangeli, A. |
en_US |
dc.contributor.author |
Jaffe, A. H. |
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dc.contributor.author |
Jones, W. C. |
en_US |
dc.contributor.author |
Lange, A. E. |
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dc.contributor.author |
Martinis, L. |
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dc.contributor.author |
Masi, S. |
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dc.contributor.author |
Mason, P. |
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Mauskopf, P. |
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Melchiorri, A. |
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dc.contributor.author |
Montroy, T. |
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dc.contributor.author |
Pascale, E. |
en_US |
dc.contributor.author |
Piacentini, F. |
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dc.contributor.author |
Pogosyan, D. |
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dc.contributor.author |
Pongetti, F. |
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dc.contributor.author |
Prunet, S. |
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dc.contributor.author |
Romeo, G. |
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dc.contributor.author |
Ruhl, J. E. |
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dc.contributor.author |
Scaramuzzi, F. |
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dc.date.accessioned |
2004-09-22T23:45:55Z |
|
dc.date.available |
2004-09-22T23:45:55Z |
|
dc.date.issued |
2001-07-12 |
en_US |
dc.identifier.citation |
International Europhysics Conference on High Energy Physics |
en_US |
dc.identifier.citation |
Budapest, Hungary |
en_US |
dc.identifier.clearanceno |
01-1282 |
en_US |
dc.identifier.uri |
http://hdl.handle.net/2014/12912 |
|
dc.description.abstract |
This paper presents a measurement of the angular power spectrum of the Cosmic Microwave Background from l = 75 to l = 1025 (~10' to 5 degrees) from a combined analysis of four 150 GHz channels in the BOOMERANG experiment. The spectrum contains multiple peaks and minima, as predicted by standard adiabatic-inflationary models in which the primordial plasma undergoes acoustic oscillations. |
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dc.format.extent |
19155380 bytes |
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application/pdf |
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dc.language.iso |
en_US |
|
dc.subject.other |
BOOMERANG spectrum cosmos microwave |
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dc.title |
A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background |
en_US |