Measuring the Matter Density Using Baryon Oscillations in the SDSS
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Andrew J. Connolly | Robert C. Nichol | Neta A. Bahcall | Jon Brinkmann | Donald P. Schneider | Michael S. Vogeley | Avery Meiksin | Idit Zehavi | Masataka Fukugita | Will J. Percival | Daniel J. Eisenstein | R. Nichol | A. Szalay | A. Connolly | J. Brinkmann | M. Fukugita | W. Percival | D. Eisenstein | D. Weinberg | I. Zehavi | J. Loveday | A. Pope | M. Vogeley | N. Bahcall | A. Meiksin | David H. Weinberg | Jon Loveday | Adrian C. Pope | Alex S. Szalay | D. Schneider | D. Schneider | D. Schneider
[1] R. Ellis,et al. Parameter constraints for flat cosmologies from cosmic microwave background and 2dFGRS power spectra , 2002, astro-ph/0206256.
[2] B. Yanny,et al. The Sloan Digital Sky Survey monitor telescope pipeline , 2006 .
[3] J. Peacock,et al. Simulations of the formation, evolution and clustering of galaxies and quasars , 2005, Nature.
[4] R. Ellis,et al. The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications , 2005, astro-ph/0501174.
[5] P. Peebles,et al. Primeval Adiabatic Perturbation in an Expanding Universe , 1970 .
[6] F. M. Maley,et al. An Efficient Targeting Strategy for Multiobject Spectrograph Surveys: the Sloan Digital Sky Survey “Tiling” Algorithm , 2001, astro-ph/0105535.
[7] J. Silk. COSMIC BLACK-BODY RADIATION AND GALAXY FORMATION. , 1968 .
[8] V. Narayanan,et al. Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample , 2002, astro-ph/0206225.
[9] W. Percival,et al. Fourier analysis of luminosity-dependent galaxy clustering , 2003, astro-ph/0306511.
[10] Anisotropies in the cosmic microwave background : an analytic approach , 1994, astro-ph/9407093.
[11] J. P. Huchra,et al. Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant , 1998, astro-ph/9801080.
[12] J. Gunn,et al. A Photometricity and Extinction Monitor at the Apache Point Observatory , 2001, astro-ph/0106511.
[13] John E. Davis,et al. Sloan Digital Sky Survey: Early Data Release , 2002 .
[14] J. Holtzman. Microwave background anisotropies and large-scale structure in universes with cold dark matter, baryons, radiation, and massive and massless neutrinos , 1989 .
[15] Baryonic Acoustic Oscillations in Simulated Galaxy Redshift Surveys , 2005, astro-ph/0507338.
[16] V. Narayanan,et al. Spectroscopic Target Selection for the Sloan Digital Sky Survey: The Luminous Red Galaxy Sample , 2001, astro-ph/0108153.
[17] G. Huetsi. Acoustic oscillations in the SDSS DR4 luminous red galaxy sample power spectrum , 2005, astro-ph/0507678.
[18] J. R. Bond,et al. Cosmic background radiation anisotropies in universes dominated by nonbaryonic dark matter , 1984 .
[19] R. Nichol,et al. Cosmological constraints from the SDSS luminous red galaxies , 2006, astro-ph/0608632.
[20] M. Fukugita,et al. The Sloan Digital Sky Survey Photometric System , 1996 .
[21] E. Bertschinger,et al. Position-space description of the cosmic microwave background and its temperature correlation function. , 2000, Physical review letters.
[22] M. Halpern,et al. First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Interpretation of the TT and TE Angular Power Spectrum Peaks , 2003, astro-ph/0302220.
[23] et al,et al. The Sloan Digital Sky Survey Photometric Camera , 1998, astro-ph/9809085.
[24] Napp,et al. SDSS data management and photometric quality assessment , 2008 .
[25] R. Nichol,et al. The Fourth Data Release of the Sloan Digital Sky Survey , 2005 .
[26] Hee-Jong SeoDaniel J. Eisenstein. Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys , 2003 .
[27] R. Lupton,et al. Astrometric Calibration of the Sloan Digital Sky Survey , 2002, astro-ph/0211375.
[28] Dynamics of cosmological perturbations in position space , 2002, astro-ph/0202215.
[29] Christopher J. Miller,et al. Possible Detection of Baryonic Fluctuations in the Large-Scale Structure Power Spectrum , 2001, astro-ph/0103018.
[30] J. Peacock,et al. Power spectrum analysis of three-dimensional redshift surveys , 1993, astro-ph/9304022.
[31] E. al.,et al. The Sloan Digital Sky Survey: Technical summary , 2000, astro-ph/0006396.
[32] Baryonic signatures in Large-Scale Structure , 1998, astro-ph/9812214.
[33] Walter A. Siegmund,et al. The 2.5 m Telescope of the Sloan Digital Sky Survey , 2006, astro-ph/0602326.
[34] 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.
[35] R. Ellis,et al. The 2dF Galaxy Redshift Survey: the power spectrum and the matter content of the Universe , 2001, astro-ph/0105252.
[36] Wayne Hu,et al. Baryonic Features in the Matter Transfer Function , 1997, astro-ph/9709112.
[37] Baryon oscillations , 2005, astro-ph/0507307.
[38] J. R. Bond,et al. The statistics of cosmic background radiation fluctuations , 1987 .