Journal article

Implications of the cosmic background imager polarization data

Abstract:: We present new measurements of the power spectra of the E mode of cosmic microwave background (CMB) polarization, the temperature T, the cross-correlation of E and T, and upper limits on the B mode from 2.5 yr of dedicated Cosmic Background Imager (CBI) observations. Both raw maps and optimal signal images in the (u, v)-plane and the sky plane show strong detections of the E mode (11.7 σ for the EE power spectrum overall) and no detection of the B mode. The power spectra are used to constrain...
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APA Style

Sievers, J., Achermann, C., Bond, J. R., Bronfman, L., Bustos, R., Contaldi, C., Dickinson, C., Ferreira, P., Jones, M., Lewis, A., Mason, B., May, J., Myers, S., Oyarce, N., Padin, S., Pearson, T., Pospieszalski, M., Readhead, A., Reeves, R., … Torres, S. (2007). Implications of the cosmic background imager polarization data. Astrophysical Journal, 660(2 I), 976–987.

MLA Style

Sievers, J., et al. “Implications of the Cosmic Background Imager Polarization Data.” Astrophysical Journal, vol. 660, no. 2 I, 2007, pp. 976–87.

Chicago Style

Sievers, J, C Achermann, JR Bond, L Bronfman, R Bustos, C Contaldi, C Dickinson, et al. 2007. “Implications of the Cosmic Background Imager Polarization Data.” Astrophysical Journal 660 (2 I): 976–87.
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Publisher copy:: 10.1086/510504

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+ Sievers, J More by this author

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+ Achermann, C More by this author

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+ Bond, JR More by this author

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+ Bronfman, L More by this author

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+ Bustos, R More by this author

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Bibliographic Details

Journal:: Astrophysical Journal More from this journal
Volume:: 660
Issue:: 2 I
Pages:: 976-987
Publication date:: 2007-05-10
DOI:: 10.1086/510504
EISSN:: 1538-4357
ISSN:: 0004-637X

Item Description

Language:: English
Keywords:: Cosmic microwave background

Polarization
Pubs id:: pubs:103463
UUID:: uuid:d3f1cc89-63ef-45a5-aab4-72daa951d50c
Local pid:: pubs:103463
Source identifiers:: 103463
Deposit date:: 2012-12-19

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Copyright date:: 2007

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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