We measure cosmological parameters using the three-dimensional power spectrum P (k)
from over 200 000 galaxies in the Sloan Digital Sky Survey (SDSS) in combination with …

The accelerating expansion of the universe is the most surprising cosmological discovery in
many decades, implying that the universe is dominated by some form of “dark energy” with …

We combine the constraints from the recent Ly α forest analysis of the Sloan Digital Sky Survey
(SDSS) and the SDSS galaxy bias analysis with previous constraints from SDSS galaxy …

The Sloan Digital Sky Survey (SDSS) will provide the data to support detailed investigations
of the distribution of luminous and nonluminous matter in the universe: a photometrically …

We present cosmological results from the final galaxy clustering data set of the Baryon
Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III. Our combined galaxy …

We present a one per cent measurement of the cosmic distance scale from the detections of
the baryon acoustic oscillations (BAO) in the clustering of galaxies from the Baryon …

Building on the legacy of the Sloan Digital Sky Survey (SDSS-I and II), SDSS-III is a program
of four spectroscopic surveys on three scientific themes: dark energy and cosmological …

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 …

We measure the large-scale real-space power spectrum P (k) by using a sample of 205,443
galaxies from the Sloan Digital Sky Survey, covering 2417 effective square degrees with …

The spectroscopic Sloan Digital Sky Survey (SDSS) Data Release 7 (DR7) galaxy sample
represents the final set of galaxies observed using the original SDSS target selection criteria. …