Investigating Emission Line Galaxy Surveys with the Sloan Digital Sky Survey Telescope

J. Comparat 1 J.-P. Kneib 1 S. Escoffier 2 J. Zoubian 1 A. Ealet 2 F. Lamareille 3 N. Mostek O. Steele E. Aubourg 4 S. Bailey A.-S. Bolton J. Brownstein K. Dawson A. Leauthaud C. Maraston W. Percival N.-P. Ross D.-J. Schlegel D.-P. Schneider D. Thomas J.-L. Tinker B.-A. Weaver
1 LAM - Laboratoire d'Astrophysique de Marseille
2 CPPM - Centre de Physique des Particules de Marseille
3 IRAP - Institut de recherche en astrophysique et planétologie
4 APC - Cosmologie
PCC - Physique Corpusculaire et Cosmologie - Collège de France, APC - UMR 7164 - AstroParticule et Cosmologie
Abstract : The Baryon 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 $0.6
Type de document :
Article dans une revue
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P - Oxford Open Option A, 2013, 428, pp.1498-1517. <10.1093/mnras/sts127>
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Contributeur : Danielle Cristofol <>
Soumis le : vendredi 20 juillet 2012 - 09:23:28
Dernière modification le : mardi 11 octobre 2016 - 15:23:40

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J. Comparat, J.-P. Kneib, S. Escoffier, J. Zoubian, A. Ealet, et al.. Investigating Emission Line Galaxy Surveys with the Sloan Digital Sky Survey Telescope. Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P - Oxford Open Option A, 2013, 428, pp.1498-1517. <10.1093/mnras/sts127>. <in2p3-00719510>

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