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

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
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Submitted on : Friday, July 20, 2012 - 9:23:28 AM
Last modification on : Monday, April 5, 2021 - 2:26:13 PM

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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 (2), pp.1498-1517. ⟨10.1093/mnras/sts127⟩. ⟨in2p3-00719510⟩

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