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Determining the motion of the Solar system relative to the cosmic microwave background using Type Ia supernovae

Publication status:: Published

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APA Style

Gordon, C., Land, K., & Slosar, A. (2008). Determining the motion of the Solar system relative to the cosmic microwave background using Type Ia supernovae. Monthly Notices of the Royal Astronomical Society, 387(1), 371–376.

MLA Style

Gordon, C., et al. “Determining the Motion of the Solar System Relative to the Cosmic Microwave Background Using Type Ia Supernovae.” Monthly Notices of the Royal Astronomical Society, vol. 387, no. 1, 2008, pp. 371–76.

Chicago Style

Gordon, C, K Land, and A Slosar. 2008. “Determining the Motion of the Solar System Relative to the Cosmic Microwave Background Using Type Ia Supernovae.” Monthly Notices of the Royal Astronomical Society 387 (1): 371–76.
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Publisher copy:: 10.1111/j.1365-2966.2008.13239.x

Authors

+ Gordon, C More by this author

Institution:: University of Oxford
Division:: MPLS
Department:: Physics
Sub department:: Astrophysics
Role:: Author

+ Land, K More by this author

Role:: Author

+ Slosar, A More by this author

Role:: Author

Journal:: Monthly Notices of the Royal Astronomical Society More from this journal
Volume:: 387
Issue:: 1
Pages:: 371-376
Publication date:: 2008-06-11
DOI:: 10.1111/j.1365-2966.2008.13239.x
EISSN:: 1365-2966
ISSN:: 0035-8711

Keywords:: cosmic microwave background

Solar system : general

supernovae : general
Pubs id:: pubs:885
UUID:: uuid:f1efa690-3e93-4aa4-9faa-3aed894f6c16
Local pid:: pubs:885
Source identifiers:: 885
Deposit date:: 2012-12-19

Terms of use

Copyright date:: 2008

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

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