Spherical Mexican hat wavelet: An application to detect non-Gaussianity in the COBE-DMR maps

Monthly Notices of the Royal Astronomical Society

Volumn 326, Issue 4, 2001, Pages 1243-1248

  Cayon L ^a   Sanz, J L ^a   Martinez Gonzalez E ^a   Banday, A J ^b   Argueso F ^c   Gallegos, J E ^a   Gorski K M ^d   Hinshaw, G ^e  

^a INSTITUTO DE FÍSICA DE CANTABRIA CSIC UC   (Spain)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^c UNIVERSITY OF OVIEDO   (Spain)

^d EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^e NASA HEADQUARTERS   (United States)

Author keywords

Data analysis cosmic microwave background; Methods

Indexed keywords

GAUSSIAN DISTRIBUTION; HIGHER ORDER STATISTICS; PIXELS; WAVELET ANALYSIS;

BACKGROUND TEMPERATURE; COSMIC MICROWAVES BACKGROUND; DATA ANALYSE - COSMIC MICROWAVE BACKGROUND; GAUSSIAN SIMULATIONS; METHOD; MEXICAN HAT WAVELET; NONGAUSSIANITY; TEMPERATURE FLUCTUATION; TEMPERATURE VALUES;

COSMOLOGY;

EID: 0001193710     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2001.04641.x     Document Type: Article

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