Multiple peaks in the angular power spectrum of the cosmic microwave background: Significance and consequences for cosmology

de Bernardis, P., Ade, Peter A. R. ORCID: https://orcid.org/0000-0002-5127-0401, Bock, J. J., Bond, J. R., Borrill, J., Boscaleri, A., Coble, K., Contaldi, C. R., Crill, B. P., 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 ORCID: https://orcid.org/0000-0001-6397-5516, Melchiorri, A., Montroy, T., Netterfield, C. B., Pascale, E., Piacentini, F., Pogosyan, D., Polenta, G., Pongetti, F., Prunet, S., Romeo, G., Ruhl, J. E. and Scaramuzzi, F. 2002. Multiple peaks in the angular power spectrum of the cosmic microwave background: Significance and consequences for cosmology. Astrophysical Journal 564 (2) , pp. 559-566. 10.1086/324298

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Item Type:	Article
Date Type:	Publication
Status:	Published
Schools:	Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Uncontrolled Keywords:	cosmic microwave background; cosmological parameters; cosmology: observations
Publisher:	IOP Sciences
ISSN:	0004-637X
Last Modified:	24 Oct 2022 10:06
URI:	https://orca.cardiff.ac.uk/id/eprint/43155

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