Non-Gaussianity detections in the Bianchi VIIh corrected WMAP one-year data made with directional spherical wavelets

Monthly Notices of the Royal Astronomical Society

Volumn 369, Issue 4, 2006, Pages 1858-1868

  McEwen, J D ^a   Hobson, M P ^a   Lasenby, A N ^a   Mortlock, D J ^b,c  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^c IMPERIAL COLLEGE LONDON   (United Kingdom)

Author keywords

Cosmic microwave background; Methods: data analysis; Methods: numerical

Indexed keywords

COSMOLOGY; HIGHER ORDER STATISTICS; NUMERICAL METHODS; SPHERES;

'CURRENT; COSMIC MICROWAVES BACKGROUND; DARK ENERGY; ENERGY COMPONENTS; GAUSSIANITY; METHOD: NUMERICAL; METHODS. DATA ANALYSIS; MEXICAN HAT WAVELET; NONGAUSSIANITY; SPHERICAL WAVELETS;

WAVELET TRANSFORMS;

EID: 33745577257     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10434.x     Document Type: Article

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