Johan Comparat, Jean-Paul Kneib, Stephanie Escoffier, Julien Zoubian, Anne Ealet, Fabrice Lamareille, N. Mostek, Oliver Steele, Eric Aubourg, Stephen Bailey, Adam S. Bolton, Joel Brownstein, Kyle Dawson, Alexie Leauthaud, Claudia Maraston, Will Percival, Nicholas P. Ross, David J. Schlegel, Donald P. Schneider, Daniel Thomas, Jeremy L. Tinker, Benjamin A. Weaver
The accelerated expansion of the universe can be probed by the Baryonic Acoustic Oscillation (BAO) feature in the power spectrum of galaxies can be used as a standard ruler to probe the accelerated expansion of the Universe. The current surveys covering a comoving volume sufficient to unveil the BAO scale are limited to redshift $z \lesssim 0.7$. In this paper, we study several galaxy selection schemes aiming at building an emission-line-galaxy (ELG) sample in the redshift range $0.6View original: http://arxiv.org/abs/1207.4321
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