Application of Monte Carlo algorithms to the Bayesian analysis of the cosmic microwave background
- Author
- JEWELL, J1 ; LEVIN, S1 ; ANDERSON, C. H1
[1] Jet Propulsion Laboratory, California Institute of Technology, MS 126-347, 4800 Oak Grove Drive, Pasadena, CA 91109-8099, United States - Source
The Astrophysical journal. 2004, Vol 609, Num 1, pp 1-14, 14 p ; 1 ; ref : 16 ref
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- University of Chicago Press, Chicago, IL
- Publication country
- United States
- Document type
- Article
- Language
- English
- Keyword (fr)
- Algorithme Analyse donnée Analyse statistique Bruit blanc Maximum vraisemblance Méthode Monte Carlo Méthode gradient conjugué Rayonnement fond cosmique Spectre puissance
- Keyword (en)
- Algorithms Data analysis Statistical analysis White noise Maximum likelihood Monte Carlo methods Conjugate gradient methods Cosmic background radiation Power spectra
- Keyword (es)
- Maxima verosimilitud
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03A Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations / 001E03A75 Observation and data reduction techniques. Computer modeling and simulation / 001E03A75P Mathematical procedures and computer techniques
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D70 Unidentified sources and radiation outside the solar system / 001E03D70V Background radiations
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 15997916
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1086/383515 
https://dx.doi.org/10.1086/383515
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