Nicolás G. Busca, Timothée Delubac, James Rich, Stephen Bailey, Andreu Font-Ribera, David Kirkby, J. -M. Le Goff, Matthew M. Pieri, Anze Slosar, Éric Aubourg, Julian E. Bautista, Dmitry Bizyaev, Michael Blomqvist, Adam S. Bolton, Jo Bovy, Howard Brewington, Arnaud Borde, J. Brinkmann, Bill Carithers, Rupert A. C. Croft, Kyle S. Dawson, Garrett Ebelke, Daniel J. Eisenstein, Jean-Christophe Hamilton, Shirley Ho, David W. Hogg, Klaus Honscheid, Khee-Gan Lee, Britt Lundgren, Elena Malanushenko, Viktor Malanushenko, Daniel Margala, Claudia Maraston, Kushal Mehta, Jordi Miralda-Escudé, Adam D. Myers, Robert C. Nichol, Pasquier Noterdaeme, Matthew D. Olmstead, Daniel Oravetz, Nathalie Palanque-Delabrouille, Kaike Pan, Isabelle Pâris, Will J. Percival, Patrick Petitjean, N. A. Roe, Emmanuel Rollinde, Nicholas P. Ross, Graziano Rossi, David J. Schlegel, Donald P. Schneider, Alaina Shelden, Erin S. Sheldon, Audrey Simmons, Stephanie Snedden, Jeremy L. Tinker, Matteo Viel, Benjamin A. Weaver, David H. Weinberg, Martin White, Christophe Yèche, Donald G. York, Gong-Bo Zhao
We report a detection of the baryon acoustic oscillation (BAO) feature in the three-dimensional correlation function of the transmitted flux fraction in the \Lya forest of high-redshift quasars. The study uses 48,640 quasars in the redshift range $2.1\le z \le 3.5$ from the Baryon Oscillation Spectroscopic Survey (BOSS) of the third generation of the Sloan Digital Sky Survey (SDSS-III). At a mean redshift $z=2.3$, we measure the monopole and quadrupole components of the correlation function for separations in the range $20\hMpcView original: http://arxiv.org/abs/1211.2616
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