CMB polarization with Boomerang 2003

Piacentini, F., Ade, Peter A. R. ORCID: https://orcid.org/0000-0002-5127-0401, Bock, J. J., Bond, J. R., Borrill, J., Boscaleri, A., Cabella, P., Contaldi, C. R., Crill, B. P., de Bernardis, P., De Gasperis, G., de Oliveira-Costa, A., De Troia, G., Di Stefano, G., Hivon, E., Jaffe, A. H., Kisner, T. S., Jones, W. C., Lange, A. E., Marini-Bettolo, C., Masi, S., Mauskopf, Philip Daniel ORCID: https://orcid.org/0000-0001-6397-5516, MacTavish, C. J., Melchiorri, A., Montroy, T.E., Nati, F., Nati, L., Natoli, P., Netterfield, C. B., Pascale, Enzo ORCID: https://orcid.org/0000-0002-3242-8154, Pogosyan, D., Polenta, G., Prunet, S., Ricciardi, S., Romeo, G., Ruhl, J. E., Santini, P., Tegmark, M., Veneziani, M. and Vittorio, N. 2007. CMB polarization with Boomerang 2003. New Astronomy Reviews 51 (3-4) , pp. 244-249. 10.1016/j.newar.2006.11.058

Full text not available from this repository.

Abstract

This paper reports results from the Boomerang 2003 flights, devoted to the measurement of intensity and polarization of the cosmic microwave background radiation. In particular, it is focused on the power angular power spectra and on the control of possible contamination from systematic effects and foregrounds.

Item Type:	Article
Date Type:	Publication
Status:	Published
Schools:	Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Uncontrolled Keywords:	Cosmology; CMB; Polarization
Publisher:	Elsevier
ISSN:	1387-6473
Last Modified:	21 Oct 2022 10:10
URI:	https://orca.cardiff.ac.uk/id/eprint/39312

Citation Data

Cited 1 time in Scopus. View in Scopus. Powered By Scopus® Data

Actions (repository staff only)

Edit Item