Ariel G. Sanchez, Eyal A. Kazin, Florian Beutler, Chia-Hsun Chuang, Antonio J. Cuesta, Daniel J. Eisenstein, Marc Manera, Francesco Montesano, Bob Nichol, Nikhil Padmanabhan, Will Percival, Francisco Prada, Ashley J. Ross, David J. Schlegel, Jeremy Tinker, Rita Tojeiro, David H. Weinberg, Xiaoying Xu, J. Brinkmann, Joel R. Brownstein, Donald P. Schneider, Daniel Thomas
We explore the cosmological implications of the clustering wedges, xi_perp(s) and xi_para(s), of the CMASS Data Release 9 (DR9) sample of the Baryon Oscillation Spectroscopic Survey (BOSS). These clustering wedges are defined by averaging the full two-dimensional correlation function, xi(mu,s), over the ranges 0View original: http://arxiv.org/abs/1303.4396
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