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  Fast and precise way to calculate the posterior for the local non-Gaussianity parameter fnl from cosmic microwave background observations

Dorn, S., Oppermann, N., Khatri, R., Selig, M., & Enßlin, T. A. (2013). Fast and precise way to calculate the posterior for the local non-Gaussianity parameter fnl from cosmic microwave background observations. Physical Review D, 88(10): 103516, pp. 1-12. doi:10.1103/PhysRevD.88.103516.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0015-7A36-9 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-002A-3B63-4
Genre: Journal Article

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 Creators:
Dorn, Sebastian1, Author           
Oppermann, Niels1, Author           
Khatri, Rishi2, Author           
Selig, Marco1, Author           
Enßlin, Torsten A.1, Author           
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1Computational Structure Formation, MPI for Astrophysics, Max Planck Society, ou_2205642              
2High Energy Astrophysics, MPI for Astrophysics, Max Planck Society, ou_159881              

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Language(s): eng - English
 Dates: 2013-11-12
 Publication Status: Issued
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 Rev. Type: Peer
 Identifiers: DOI: 10.1103/PhysRevD.88.103516
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Title: Physical Review D
  Abbreviation : Phys. Rev. D
Source Genre: Journal
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Pages: - Volume / Issue: 88 (10) Sequence Number: 103516 Start / End Page: 1 - 12 Identifier: ISSN: 1550-7998