Journal article

Determining foreground contamination in cosmic microwave background observations: Diffuse Galactic emission in the MAXIMA-I field

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APA Style

Jaffe, A., Balbi, A., Bond, J. R., Borrill, J., Ferreira, P., Finkbeiner, D., Hanany, S., Lee, A., Rabii, B., Richards, P., Smoot, G., Stompor, R., Winant, C., & Wu, J. (2004). Determining foreground contamination in cosmic microwave background observations: Diffuse Galactic emission in the MAXIMA-I field. ASTROPHYSICAL JOURNAL, 615(1), 55–62.

MLA Style

Jaffe, A, et al. “Determining Foreground Contamination in Cosmic Microwave Background Observations: Diffuse Galactic Emission in the MAXIMA-I Field.” ASTROPHYSICAL JOURNAL, vol. 615, no. 1, 2004, pp. 55–62.

Chicago Style

Jaffe, A, A Balbi, JR Bond, et al. 2004. “Determining Foreground Contamination in Cosmic Microwave Background Observations: Diffuse Galactic Emission in the MAXIMA-I Field.” ASTROPHYSICAL JOURNAL 615 (1): 55–62.
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Publisher copy:: 10.1086/422635

Authors

+ Jaffe, A More by this author

Role:: Author

+ Balbi, A More by this author

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+ Bond, JR More by this author

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+ Borrill, J More by this author

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+ Ferreira, P More by this author

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Journal:: ASTROPHYSICAL JOURNAL More from this journal
Volume:: 615
Issue:: 1
Pages:: 55-62
Publication date:: 2004-11-01
DOI:: 10.1086/422635
EISSN:: 1538-4357
ISSN:: 0004-637X

Keywords:: cosmic microwave background

cosmology : observations
Pubs id:: pubs:207718
UUID:: uuid:15232e01-74c8-4656-8ac3-651b33497d8b
Local pid:: pubs:207718
Source identifiers:: 207718
Deposit date:: 2012-12-19
ARK identifier:: ark:/29072/ora_15232e0174c846568ac3651b33497d8b

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Copyright date:: 2004

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

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