A Measurement of the Quadrupole Power Spectrum in the Clustering of the 2dF QSO Survey
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[1] J. Fry. The Evolution of Bias , 1996 .
[2] L. Amendola,et al. Constraints on perfect fluid and scalar field dark energy models from future redshift surveys , 2004, astro-ph/0404599.
[3] J. Peacock,et al. Power spectrum analysis of three-dimensional redshift surveys , 1993, astro-ph/9304022.
[4] Tom Shanks,et al. The 2dF QSO Redshift survey: XIII. A measurement of Λ from the quasi-stellar object power spectrum, PS(k∥, k⊥) , 2004 .
[5] Oxford,et al. The 2dF QSO Redshift Survey – XII. The spectroscopic catalogue and luminosity function , 2004, astro-ph/0403040.
[6] Fourier analysis of redshift-space distortions and the determination of Ω , 1993, astro-ph/9308003.
[7] Kazuhiro Yamamoto. Optimal Weighting Scheme in Redshift-Space Power Spectrum Analysis and a Prospect for Measuring the Cosmic Equation of State , 2002, astro-ph/0208139.
[8] R. Nichol,et al. Cosmological parameters from SDSS and WMAP , 2003, astro-ph/0310723.
[9] Analytical approximations to the low-order statistics of dark matter distributions , 1996, astro-ph/9607143.
[10] T. Matsubara,et al. Cosmological Redshift Distortion of Correlation Functions as a Probe of the Density Parameter and the Cosmological Constant , 1996, astro-ph/9604142.
[11] R. Ellis,et al. Measurements of $\Omega$ and $\Lambda$ from 42 high redshift supernovae , 1998, astro-ph/9812133.
[12] Eric V. Linder. Baryon oscillations as a cosmological probe , 2003 .
[13] Oxford,et al. The 2dF QSO Redshift Survey — II. Structure and evolution at high redshift , 2001 .
[14] Y. Suto,et al. Light-Cone Effect on Clustering Statistics in Cosmological Redshift Space , 1999, astro-ph/9912367.
[15] Estimating β from redshift‐space distortions in the 2dF galaxy survey , 1999, astro-ph/9905186.
[16] F. Lucchin. CLUSTERING IN THE UNIVERSE , 1986 .
[17] Y. Jing,et al. Deciphering cosmological information from redshift surveys of high-z objects - The cosmological light-cone effect and redshift-space distortion , 1999, astro-ph/9901179.
[18] Kazuhiro Yamamoto. Cosmological constraint from the 2dF QSO spatial power spectrum , 2002 .
[19] Edward J. Wollack,et al. First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Determination of cosmological parameters , 2003, astro-ph/0302209.
[20] N. Kaiser. Clustering in real space and in redshift space , 1987 .
[21] The 2dF QSO Redshift Survey — XI. The QSO power spectrum , 2003, astro-ph/0302280.
[22] B. Paczyński,et al. An evolution free test for non-zero cosmological constant , 1979, Nature.
[23] Donald Hamilton,et al. The evolving universe. Selected topics on large-scale structure and on the properties of galaxies , 1998 .
[24] R. Ellis,et al. The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications , 2005, astro-ph/0501174.
[25] D. Lambert,et al. The emission-line spectrum of the hot R Coronae Borealis star MV Sgr , 1996 .
[26] Kazuhiro Yamamoto. Power Spectrum Analysis of the Two-Degree Field QSO Sample Revisited , 2004, astro-ph/0401039.
[27] A. Taylor,et al. Non-linear cosmological power spectra in real and redshift space , 1996, astro-ph/9604020.
[28] R. Nichol,et al. Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies , 2005, astro-ph/0501171.
[29] A. Szalay,et al. Large-Scale Clustering of Sloan Digital Sky Survey Quasars: Impact of the Baryon Density and the Cosmological Constant , 2004, astro-ph/0412631.
[30] Hee-Jong SeoDaniel J. Eisenstein. Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys , 2003 .
[31] Measuring the cosmological constant with redshift surveys , 1996, astro-ph/9605017.
[32] M. Phillips,et al. Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant , 1998, astro-ph/9805201.
[33] Scott M. Croom,et al. The 2dF QSO Redshift Survey - XIV. Structure and evolution from the two-point correlation function , 2005 .