Testing the Gaussianity of the COBE DMR data with spherical wavelets |
| |
| Authors: | R B Barreiro M P Hobson A N Lasenby A J Banday K M Górski G Hinshaw |
| |
| Institution: | Astrophysics Group, Cavendish Laboratory, Madingley Road, Cambridge CB3 0HE;Max-Planck Institut für Astrophysik (MPA), Karl-Schwarzschild Strasse 1, D-85740 Garching, Germany;European Southern Observatory (ESO), Karl-Schwarzschild Strasse 2, D-85740 Garching, Germany;Warsaw University Observatory, Aleje Ujazdowskie 4, 00-478 Warszawa, Poland;NASA/GSFC, Greenbelt, MD 20771, USA |
| |
| Abstract: | We investigate the Gaussianity of the 4-yr COBE DMR data (in HEALPix pixelization) using an analysis based on spherical Haar wavelets. We use all the pixels lying outside the Galactic cut and compute the skewness, kurtosis and scale–scale correlation spectra for the wavelet coefficients at each scale. We also take into account the sensitivity of the method to the orientation of the input signal. We find a detection of non-Gaussianity at >99 per cent level in just one of our statistics. Taking into account the total number of statistics computed, we estimate that the probability of obtaining such a detection by chance for an underlying Gaussian field is 0.69. Therefore, we conclude that the spherical wavelet technique shows no strong evidence of non-Gaussianity in the COBE DMR data. |
| |
| Keywords: | methods: data analysis cosmic microwave background |
|
|
