4k citations · 5.5k across the 6 of their papers we have counts for
6 papers
Cosmological Constraints from the Clustering of the Sloan Digital Sky Survey DR7 Luminous Red Galaxies
Beth A. Reid, Will J. Percival, Daniel J. Eisenstein +25
We present the power spectrum of the reconstructed halo density field derived from a sample of Luminous Red Galaxies (LRGs) from the Sloan Digital Sky Survey Seventh Data Release (…
Cosmological parameters from SDSS and WMAP
M. Tegmark, M. Strauss, M. Blanton +34
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 WMAP and ot…
Galaxy Clustering in Early SDSS Redshift Data
SDSS Collaboration, Idit Zehavi, Michael R. Blanton +4
We present the first measurements of clustering in the Sloan Digital Sky Survey (SDSS) galaxy redshift survey. Our sample consists of 29,300 galaxies with redshifts 5,700 km/s < cz…
Galaxy Number Counts from the Sloan Digital Sky Survey Commissioning Data
Naoki Yasuda, Masataka Fukugita, Vijay K. Narayanan +10
We present bright galaxy number counts in five broad bands () from imaging data taken during the commissioning phase of the Sloan Digital Sky Survey (SDSS). The…
Finding Clusters of Galaxies in the Sloan Digital Sky Survey using Voronoi Tessellation
Rita S. J. Kim, Michael A. Strauss, Neta A. Bahcall +5
The Sloan Digital Sky Survey has obtained 450 square degrees of photometric scan data, in five bands (u',g',r',i',z'), which we use to identify clusters of galaxies. We illustrate…
Eigenmode Analysis of Galaxy Redshift Surveys I. Theory and Methods
Michael S. Vogeley, Alexander S. Szalay
We describe a method for estimating the power spectrum of density fluctuations from galaxy redshift surveys that yields improvement in both accuracy and resolution over direct Four…