Non-parametric reconstruction of the primordial power spectrum at horizon scales from WMAP data

Monthly Notices of the Royal Astronomical Society

Volumn 367, Issue 3, 2006, Pages 1095-1102

  Tocchini Valentini, Domenico ^a,b   Hoffman, Yehuda ^c   Silk, Joseph ^a  

^a UNIVERSITY OF OXFORD   (United Kingdom)

^b JOHNS HOPKINS UNIVERSITY   (United States)

^c HEBREW UNIVERSITY OF JERUSALEM   (Israel)

Author keywords

Cosmic microwave background; Cosmological parameters; Early Universe; Methods: data analysis

Indexed keywords

COSMOLOGY; INTELLIGENT SYSTEMS; MONTE CARLO METHODS; SPECTRUM ANALYSIS;

COSMIC MICROWAVES BACKGROUND; COSMOLOGICAL PARAMETERS; EARLY UNIVERSE; INDEX N; METHODS. DATA ANALYSIS; POWER-SPECTRA; SCALE-FREE; SPECTRA'S; SPECTRAL INDICES; WILKINSON MICROWAVE ANISOTROPY PROBE;

POWER SPECTRUM;

EID: 33645401901     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10031.x     Document Type: Article

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