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

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Hernández-Monteagudo,  C.
High Energy Astrophysics, MPI for Astrophysics, Max Planck Society;

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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.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0011-B773-0
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