Non-Gaussianity of the Derived Maps from the First-Year Wilkinson Microwave Anisotropy Probe Data
- 27 May 2003
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 590 (2), L65-L68
- https://doi.org/10.1086/376822
Abstract
We present non-Gaussianity testing on recently-released derived maps from the first-year WMAP data by Tegmark, de Oliveria-Costa and Hamilton. Our test is based on a phase mapping technique which has the advantage of testing non-Gaussianity at separate multipole bands. We show that their foreground-cleaned map is against the random-phase hypothesis at all 4 multipole bands centered around l = 150, 290, 400 and 500. Their Wiener-filtered map, on the other hand, is Gaussian for l < 250, and marginally Gaussian for 224 < l < 350. However, we see the evidence of non-Gaussianity for l > 350 as we detect certain degrees of phase coupling, hence against the random-phase hypothesis. Our phase mapping technique is particularly useful for testing the accuracy of component separation methods.Comment: 4 pages, 5 figures, ApJL accepted with minor changes (2 sentences added in the Discussions). High-resolution figures can be obtained from http://www.tac.dk/~chiang/wmap.htmKeywords
All Related Versions
This publication has 7 references indexed in Scilit:
- High resolution foreground cleaned CMB map from WMAPPhysical Review D, 2003
- TheMicrowave Anisotropy ProbeMissionThe Astrophysical Journal, 2003
- Statistical cosmology with quadratic density fieldsMonthly Notices of the Royal Astronomical Society, 2003
- Return mapping of phases and the analysis of the gravitational clustering hierarchyMonthly Notices of the Royal Astronomical Society, 2002
- Characterizing the nonlinear growth of large-scale structure in the UniverseNature, 2000
- The statistics of cosmic background radiation fluctuationsMonthly Notices of the Royal Astronomical Society, 1987
- The statistics of peaks of Gaussian random fieldsThe Astrophysical Journal, 1986