Can a large-scale structure probe cosmic microwave background-constrained non-Gaussianity?

Kang, X.; Norberg, P.; Silk, J.

doi:10.1111/j.1365-2966.2007.11435.x

Can a large-scale structure probe cosmic microwave background-constrained non-Gaussianity?

Kang, X.; Norberg, P.; Silk, J.

Authors

X. Kang

Professor Peder Norberg peder.norberg@durham.ac.uk
Professor

J. Silk

Citation

Kang, X., Norberg, P., & Silk, J. (2007). Can a large-scale structure probe cosmic microwave background-constrained non-Gaussianity?. Monthly Notices of the Royal Astronomical Society, 376, 343-347. https://doi.org/10.1111/j.1365-2966.2007.11435.x

Journal Article Type	Article
Publication Date	2007-03
Deposit Date	Jun 3, 2014
Journal	\mnras
Print ISSN	0035-8711
Electronic ISSN	1365-2966
Publisher	Royal Astronomical Society
Volume	376
Pages	343-347
DOI	https://doi.org/10.1111/j.1365-2966.2007.11435.x
Public URL	https://durham-repository.worktribe.com/output/1450784
Publisher URL	http://ukads.nottingham.ac.uk/abs/2007MNRAS.376..343K

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