Constraints on perfect fluid and scalar field dark energy models from future redshift surveys
Open Access
- 1 February 2005
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 357 (2) , 429-439
- https://doi.org/10.1111/j.1365-2966.2004.08558.x
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This publication has 35 references indexed in Scilit:
- Cosmic Acceleration versus Axion‐Photon MixingThe Astrophysical Journal, 2004
- Growth rate of large-scale structure as a powerful probe of dark energyPhysical Review D, 2004
- Probing Dark Energy Using Baryonic Oscillations in the Galaxy Power Spectrum as a Cosmological RulerThe Astrophysical Journal, 2003
- Tracking and coupled dark energy as seen by the Wilkinson Microwave Anisotropy ProbePhysical Review D, 2003
- TheMicrowave Anisotropy ProbeMissionThe Astrophysical Journal, 2003
- Spectroscopic Target Selection for the Sloan Digital Sky Survey: The Luminous Red Galaxy SampleThe Astronomical Journal, 2001
- Coupled quintessencePhysical Review D, 2000
- Cosmic Complementarity: Joint Parameter Estimation from Cosmic Microwave Background Experiments and Redshift SurveysThe Astrophysical Journal, 1999
- A Counts‐in‐Cells Analysis of Lyman‐Break Galaxies at Redshiftz∼ 3The Astrophysical Journal, 1998
- Cosmic Complementarity: [ITAL]H[/ITAL][TINF]0[/TINF] and Ω[TINF][CLC][ITAL]m[/ITAL][/CLC][/TINF] from Combining Cosmic Microwave Background Experiments and Redshift SurveysThe Astrophysical Journal, 1998