The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the full shape of the clustering wedges in the data release 10 and 11 galaxy samples

@inproceedings{Snchez2014TheCO,
  title={The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the full shape of the clustering wedges in the data release 10 and 11 galaxy samples},
  author={A. G. Soriano S{\'a}nchez and Francesco Saverio Montesano and Eyal A. Kazin and {\'E}ric Aubourg and Florian Beutler and Jon Brinkmann and Joel R. Brownstein and Antonio J. Cuesta and Kyle S. Dawson and Daniel J. Eisenstein and Shirley Ho and Klaus Honscheid and Marc Manera and Claudia Maraston and Cameron Keith McBride and Will J. Percival and Ashley J Ross and Lado Samushia and David J. Schlegel and Donald P. Schneider and Ramin A. Skibba and Daniel Thomas and Jeremy L. Tinker and Rita Tojeiro and David A. Wake and Benjamin Alan Weaver and Martin S. White and Idit Zehavi},
  year={2014}
}
We explore the cosmological implications of the angle-averaged correlation function, ξ (s), and the clustering wedges, ξ ⊥(s) and ξ � (s), of the LOWZ and CMASS galaxy samples from Data Releases 10 and 11 of the Sloan Digital Sky Survey III (SDSS-III) Baryon Oscillation Spectroscopic Survey. Our results show no significant evidence for a deviation from the standard � cold dark matter model. The combination of the information from our clustering measurements with recent data from the cosmic… CONTINUE READING

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