Cosmological constraints from the SDSS luminous red galaxies

Космологические ограничения по данным о ярких красных галактиках SDSS
Max Tegmark, Daniel J. Eisenstein, Michael A. Strauss, David H. Weinberg, Michael R. Blanton, Joshua A. Frieman, M. Fukugita, James E. Gunn, A. Hamilton, G. R. Knapp, Robert C. Nichol, Jeremiah P. Ostriker, Nikhil Padmanabhan, Will J. Percival, David J. Schlegel, Donald P. Schneider, Román Scoccimarro, Uroš Seljak, Hee‐Jong Seo, M. E. C. Swanson, Alexander S. Szalay, Michael S. Vogeley, Jaiyul Yoo, Idit Zehavi, Kevork N. Abazajian, Scott F. Anderson, James Annis, Neta A. Bahcall, Bruce A. Bassett, Andreas A. Berlind, J. Brinkmann, Tamás Budavári, F. J. Castander, Andrew J. Connolly, István Csabai, Mamoru Doi, Douglas P. Finkbeiner, Bruce Gillespie, Karl Glazebrook, G. S. Hennessy, David W. Hogg, Željko Ivezić, Bhuvnesh Jain, David Johnston, S. Kent, Donald Q. Lamb, Brian Lee, H. Lin, J. Loveday, Robert H. Lupton, Jeffrey A. Munn, Kaike Pan, Changbom Park, J. Peoples, Jeffrey R. Pier, Adrian Pope, M. Richmond, Constance M. Rockosi, Ryan Scranton, Ravi K. Sheth, Albert Stebbins, Christopher Stoughton, István Szapudi, D. L. Tucker, D. E. vanden Berk, B. Yanny, Donald G. York
2006-12-11

SDSScosmological parametersluminous red galaxiespower spectrum estimationredshift-space distortions
We measure the large-scale real-space power spectrum $P(k)$ using luminous red galaxies (LRGs) in the Sloan Digital Sky Survey (SDSS) and use this measurement to sharpen constraints on cosmological parameters from the Wilkinson Microwave Anisotropy Probe (WMAP). We employ a matrix-based power spectrum estimation method using Pseudo-Karhunen-Lo\`eve eigenmodes, producing uncorrelated minimum-variance measurements in 20 $k$-bands of both the clustering power and its anisotropy due to redshift-space distortions, with narrow and well-behaved window functions in the range $0.01h/\mathrm{Mpc} 0.1h/\mathrm{Mpc}$ and associated nonlinear complications, yet agree well with more aggressive published analyses where nonlinear modeling is crucial.
1
A matrix-based estimator using Pseudo-Karhunen–Loève eigenmodes yields uncorrelated, minimum-variance measurements in 20 wavenumber bands.
2
Results agree with more aggressive published analyses despite avoiding regimes where nonlinear modeling is crucial.
3
The SDSS LRG power-spectrum measurement sharpens cosmological-parameter constraints derived from WMAP.
4
The analysis jointly measures clustering power and redshift-space-distortion anisotropy over 0.01–0.1 h/Mpc with narrow, well-behaved window functions.
5
The study measures the large-scale real-space power spectrum using luminous red galaxies from the Sloan Digital Sky Survey.

Large-scale galaxy clustering of luminous red galaxies (LRGs) in the Sloan Digital Sky Survey (SDSS)

The real-space power spectrum, redshift-space distortion anisotropy, and resulting cosmological parameter constraints

Publication Details
Publication Date
2006-12-11
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Authors
Max Tegmark
Daniel J. Eisenstein
Michael A. Strauss
David H. Weinberg
Michael R. Blanton
Joshua A. Frieman
M. Fukugita
James E. Gunn
A. Hamilton
G. R. Knapp
Robert C. Nichol
Jeremiah P. Ostriker
Nikhil Padmanabhan
Will J. Percival
David J. Schlegel
Donald P. Schneider
Román Scoccimarro
Uroš Seljak
Hee‐Jong Seo
M. E. C. Swanson
Alexander S. Szalay
Michael S. Vogeley
Jaiyul Yoo
Idit Zehavi
Kevork N. Abazajian
Scott F. Anderson
James Annis
Neta A. Bahcall
Bruce A. Bassett
Andreas A. Berlind
J. Brinkmann
Tamás Budavári
F. J. Castander
Andrew J. Connolly
István Csabai
Mamoru Doi
Douglas P. Finkbeiner
Bruce Gillespie
Karl Glazebrook
G. S. Hennessy
David W. Hogg
Željko Ivezić
Bhuvnesh Jain
David Johnston
S. Kent
Donald Q. Lamb
Brian Lee
H. Lin
J. Loveday
Robert H. Lupton
Jeffrey A. Munn
Kaike Pan
Changbom Park
J. Peoples
Jeffrey R. Pier
Adrian Pope
M. Richmond
Constance M. Rockosi
Ryan Scranton
Ravi K. Sheth
Albert Stebbins
Christopher Stoughton
István Szapudi
D. L. Tucker
D. E. vanden Berk
B. Yanny
Donald G. York
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