A new statistic for picking out non-Gaussianity in the CMB
Open Access
- 1 January 1999
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 302 (1) , 131-138
- https://doi.org/10.1046/j.1365-8711.1999.02104.x
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This publication has 27 references indexed in Scilit:
- Cosmic-String–Seeded Structure FormationPhysical Review Letters, 1998
- Structure Formation by Cosmic Strings with a Cosmological ConstantPhysical Review Letters, 1998
- The Case against Scaling Defect Models of Cosmic Structure FormationPhysical Review Letters, 1997
- Microwave background anisotropies from scaling seed perturbationsPhysical Review D, 1997
- Small-angle anisotropies in the CMBR from active sourcesPhysical Review D, 1997
- Non-Gaussian spectra in cosmic microwave background temperature anisotropiesPhysical Review D, 1997
- Patterns of the cosmic microwave background from evolving string networksNature, 1988
- 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
- Gauge-invariant cosmological perturbationsPhysical Review D, 1980