The deepest field

Bernardis, P. de, Ade, Peter A. R. ORCID: https://orcid.org/0000-0002-5127-0401, Bock, J. J., Bond, J. R., Borrill, J., Boscaleri, A., Coble, K., Crill, B. P., Gasperis, G. De, Troia, G. De, Farese, P. C., Ferreira, P. G., Ganga, K., Giacometti, M., Hivon, E., Hristov, V. V., Iacoangeli, A., Jaffe, A. H., Lange, A. E., Martinis, L., Masi, S., Mason, P., Mauskopf, Philip Daniel ORCID: https://orcid.org/0000-0001-6397-5516, Melchiorri, A., Miglio, L., Montroy, T., Netterfield, C. B., Pascale, Enzo ORCID: https://orcid.org/0000-0002-3242-8154, Piacentini, F., Pogosyan, D., Polenta, G., Pongetti, F., Prunet, S., Rao, S., Romeo, G., Ruhl, J. E., Scaramuzzi, F., Sforna, D. and Vittorio, N. 2001. The deepest field. Presented at: The Deepest Field: Proceedings of the ESO Workshop, Garching, Germany, 9-12 October 2000. Published in: Cristiani, S., Renzini, A. and Williams, R. E. eds. The Deep Fields: Proceedings of the ESO Workshop Held at Garching, Germany, 9-12 October 2000. Eso Astrophysics Symposia New York: Springer, pp. 362-368. 10.1007/10854354_101

Full text not available from this repository.

Abstract

The Cosmic Microwave Background (CMB) anisotropy experiments are starting to map the last scattering surface at z∼1100 with significant detail and accuracy. Here we focus on the results of the BOOMERanG experiment, which mapped the CMB over ∼3% of the sky, detecting hundreds of hot and cold spots in the microwave sky. The analysis of the characteristic sizes and shapes of the temperature fluctuations provides direct evidence for acoustic oscillations in the primeval plasma and for a flat geometry of our universe.

Item Type:	Conference or Workshop Item (Paper)
Date Type:	Publication
Status:	Published
Schools:	Physics and Astronomy
Publisher:	Springer
ISBN:	9783540427995
ISSN:	1431-2433
Related URLs:	Publisher
Last Modified:	27 Oct 2022 08:59
URI:	https://orca.cardiff.ac.uk/id/eprint/64063

Actions (repository staff only)

Edit Item