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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological constraints from the full shape of the clustering wedges
Journal article published in 2013 by
Ariel G. Sanchez,
Ariel G. Sánchez,
Eyal A. Kazin,
Florian Beutler,
Chia-Hsun Chuang 
,
Antonio J. Cuesta,
Daniel J. Eisenstein,
Marc Manera,
Francesco Montesano,
Bob Nichol,
Robert C. Nichol,
R. C. Nichol,
Nikhil Padmanabhan,
Will Percival,
Francisco Prada
and other authors.
,
Antonio J. Cuesta,
Daniel J. Eisenstein,
Marc Manera,
Francesco Montesano,
Bob Nichol,
Robert C. Nichol,
R. C. Nichol,
Nikhil Padmanabhan,
Will Percival,
Francisco Prada
and other authors.
Abstract
We explore the cosmological implications of the clustering wedges, ξ ⊥ (s) and ξ ∥ (s), of the CMASS Data Release 9 sample of the Sloan Digital Sky Survey III (SDSS-III) Baryon Oscillation Spectroscopic Survey. These clustering wedges are defined by averaging the full two-dimensional correlation function, ξ(μ, s), over the ranges 0