Detection of a non-Gaussian spot in WMAP
- 1 January 2005
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 356 (1) , 29-40
- https://doi.org/10.1111/j.1365-2966.2004.08419.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 41 references indexed in Scilit:
- First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Preliminary Maps and Basic ResultsThe Astrophysical Journal Supplement Series, 2003
- First‐YearWilkinson Microwave Anisotropy Probe(WMAP) Observations: Foreground EmissionThe Astrophysical Journal Supplement Series, 2003
- Gauge-invariant second-order perturbations and non-Gaussianity from inflationNuclear Physics B, 2003
- Non-Gaussianity: Comparing wavelet and Fourier based methodsAstronomy & Astrophysics, 2003
- Non-Gaussianity in multifield inflationPhysical Review D, 2002
- The discriminating power of wavelets to detect non-Gaussianity in the cosmic microwave backgroundMonthly Notices of the Royal Astronomical Society, 2001
- Spherical Mexican hat wavelet: an application to detect non-Gaussianity in theCOBE-DMR mapsMonthly Notices of the Royal Astronomical Society, 2001
- Testing the Gaussianity of the COBE DMR data with spherical waveletsMonthly Notices of the Royal Astronomical Society, 2000
- Isotropic wavelets: a powerful tool to extract point sources from cosmic microwave background mapsMonthly Notices of the Royal Astronomical Society, 2000
- Wavelets on the n-sphere and related manifoldsJournal of Mathematical Physics, 1998