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  Using peak distribution of the cosmic microwave background for WMAP and Planck data analysis : Formalism and simulations

Hernández-Monteagudo, C., Kashlinsky, A., & Atrio-Barandela, F. (2004). Using peak distribution of the cosmic microwave background for WMAP and Planck data analysis: Formalism and simulations. Astronomy & Astrophysics, 413(3), 833-842. doi:10.1051/0004-6361:20031583.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0011-B773-0 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0028-51FE-D
Genre: Journal Article

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 Creators:
Hernández-Monteagudo, C.1, Author           
Kashlinsky, A., Author
Atrio-Barandela, F., Author
Affiliations:
1High Energy Astrophysics, MPI for Astrophysics, Max Planck Society, ou_159881              

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Language(s): eng - English
 Dates: 2004-01
 Publication Status: Issued
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: eDoc: 185727
URI: http://www.edpsciences.org/articles/aa/abs/2004/03/aah4628/aah4628.html
DOI: 10.1051/0004-6361:20031583
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Title: Astronomy & Astrophysics
  Alternative Title : Astron. Astrophys.
Source Genre: Journal
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Pages: - Volume / Issue: 413 (3) Sequence Number: - Start / End Page: 833 - 842 Identifier: ISSN: 0004-6361