Non-linear galaxy power spectrum and cosmological parameters
- 1 February 2004
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 348 (1) , 250-260
- https://doi.org/10.1111/j.1365-2966.2004.07358.x
Abstract
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This publication has 48 references indexed in Scilit:
- Probing Dark Energy Using Baryonic Oscillations in the Galaxy Power Spectrum as a Cosmological RulerThe Astrophysical Journal, 2003
- The Halo Occupation Distribution and the Physics of Galaxy FormationThe Astrophysical Journal, 2003
- Halo models of large scale structurePhysics Reports, 2002
- Second Moment of Halo Occupation NumberThe Astrophysical Journal, 2002
- The Halo Occupation Distribution: Toward an Empirical Determination of the Relation between Galaxies and MassThe Astrophysical Journal, 2002
- The 2dF Galaxy Redshift Survey: spectra and redshiftsMonthly Notices of the Royal Astronomical Society, 2001
- Power Spectrum Covariance of Weak Gravitational LensingThe Astrophysical Journal, 2001
- Weak gravitational lensingPhysics Reports, 2001
- The nature of galaxy bias and clusteringMonthly Notices of the Royal Astronomical Society, 2000
- The real-space power spectrum of IRAS galaxies on large scales and the redshift distortionMonthly Notices of the Royal Astronomical Society, 1995