Cosmological parameters afterWMAP5: forecasts forPlanckand future galaxy surveys
Open Access
- 17 September 2009
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 398 (4) , 1621-1637
- https://doi.org/10.1111/j.1365-2966.2009.14802.x
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This publication has 57 references indexed in Scilit:
- Constraining inflationJournal of Cosmology and Astroparticle Physics, 2008
- Search for gravitational waves in the CMB after WMAP3: Foreground confusion and the optimal frequency coverage for foreground minimizationPhysical Review D, 2007
- Cosmology from PlanckNew Astronomy Reviews, 2007
- Cosmic microwave background temperature and polarization pseudo-Cℓestimators and covariancesMonthly Notices of the Royal Astronomical Society, 2005
- Cosmic Microwave Background and Inflation ParametersInternational Journal of Theoretical Physics, 2004
- What can WMAP tell us about the very early Universe? New physics as an explanation of the suppressed large scale power and running spectral indexPhysical Review D, 2003
- Running of the scalar spectral index from inflationary modelsPhysical Review D, 2003
- Coupled quintessencePhysical Review D, 2000
- Quintessence and supergravityPhysics Letters B, 1999
- Cosmological Imprint of an Energy Component with General Equation of StatePhysical Review Letters, 1998