Adapted method for separating kinetic SZ signal from primary CMB fluctuations

DOI10.1155/ASP.2005.2413zbMath1141.94313OpenAlexW2164018243WikidataQ60011279 ScholiaQ60011279MaRDI QIDQ2502686

Nabila Aghanim, Olivier Forni

Publication date: 13 September 2006

Published in: EURASIP Journal on Applied Signal Processing (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1155/asp.2005.2413

zbMATH Keywords

data analysiscosmic microwave background

Mathematics Subject Classification ID

Signal theory (characterization, reconstruction, filtering, etc.) (94A12) Computational methods for problems pertaining to astronomy and astrophysics (85-08) Statistical astronomy (85A35)

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