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
docType_s :
Journal articles
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>


http://hal.in2p3.fr/in2p3-00719510
Contributor : Danielle Cristofol <>
Submitted on : Friday, July 20, 2012 - 9:00:23 AM
Last modification on : Tuesday, October 28, 2014 - 7:00:02 PM

Identifiers

Citation

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>

Export

Share

Metrics

Consultation de la notice

61