Full-sky correlations of peaks in the microwave background
Open Access
- 1 July 2001
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 324 (4) , 960-968
- https://doi.org/10.1046/j.1365-8711.2001.04370.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 40 references indexed in Scilit:
- Geometrical estimators as a test of Gaussianity in the cosmic microwave backgroundMonthly Notices of the Royal Astronomical Society, 2001
- Constraints on Cosmological Parameters from MAXIMA-1The Astrophysical Journal, 2000
- Primordial Adiabatic Fluctuations from Cosmic DefectsPhysical Review Letters, 2000
- On the Non‐Gaussianity Observed in theCOBEDifferential Microwave Radiometer Sky MapsThe Astrophysical Journal, 2000
- Is the Cosmic Microwave Background Really Non-Gaussian?The Astrophysical Journal, 1999
- Correlation of excursion sets for non-Gaussian cosmic microwave background temperature distributionsMonthly Notices of the Royal Astronomical Society, 1998
- Peaks in the Cosmic Microwave Background: Flat versus Open ModelsThe Astrophysical Journal, 1997
- Polarization and Anisotropy of the Microwave SkyPhysical Review Letters, 1994
- Statistical geometry and the microwave backgroundMonthly Notices of the Royal Astronomical Society, 1988
- The statistics of cosmic background radiation fluctuationsMonthly Notices of the Royal Astronomical Society, 1987