On Departures from a Power Law in the Galaxy Correlation Function

We measure the projected correlation function w sub(p) [image] from the Sloan Digital Sky Survey for a flux-limited sample of 118,000 galaxies and a volume-limited subset of 22,000 galaxies with absolute magnitude M sub(r)

Saved in:
Bibliographic Details
Published in:The Astrophysical journal 2004-06, Vol.608 (1), p.16-24
Main Authors: Zehavi, Idit, Weinberg, David H, Zheng, Zheng, Berlind, Andreas A, Frieman, Joshua A, Scoccimarro, Román, Sheth, Ravi K, Blanton, Michael R, Tegmark, Max, Mo, Houjun J, Bahcall, Neta A, Brinkmann, Jon, Burles, Scott, Csabai, István, Fukugita, Masataka, Gunn, James E, Lamb, Don Q, Loveday, Jon, Lupton, Robert H, Meiksin, Avery, Munn, Jeffrey A, Nichol, Robert C, Schlegel, David, Schneider, Donald P, SubbaRao, Mark, Szalay, Alexander S, Uomoto, Alan, York, Donald G
Format: Article
Language:English
Subjects:
Astronomy
Earth, ocean, space
Exact sciences and technology
Galaxy groups, clusters, and superclusters. Large-scale structure of the universe
Stellar systems. Galactic and extragalactic objects and systems. The universe
Superclusters. Large-scale structure of the universe (including voids, pancakes, great wall, etc.)
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:We measure the projected correlation function w sub(p) [image] from the Sloan Digital Sky Survey for a flux-limited sample of 118,000 galaxies and a volume-limited subset of 22,000 galaxies with absolute magnitude M sub(r)
ISSN:0004-637X
1538-4357
DOI:10.1086/386535