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

J. Comparat; J.-P. Kneib; S. Escoffier; J. Zoubian; A. Ealet; F. Lamareille; N. Mostek; O. Steele; E. Aubourg; 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

doi:10.1093/mnras/sts127

Journal Articles Monthly Notices of the Royal Astronomical Society Year : 2013

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

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J. Comparat

Function : Author

Laboratoire d'Astrophysique de Marseille

J.-P. Kneib

Function : Author

Laboratoire d'Astrophysique de Marseille

S. Escoffier

Function : Author
PersonId : 179794
IdHAL : stephanie-escoffier
ORCID : 0000-0002-2847-7498
IdRef : 068869215

Centre de Physique des Particules de Marseille

J. Zoubian

Function : Author
PersonId : 753544
IdHAL : julien-zoubian
ORCID : 0000-0003-1962-9805
IdRef : 170320561

Laboratoire d'Astrophysique de Marseille

A. Ealet

Function : Author

Centre de Physique des Particules de Marseille

F. Lamareille

Function : Author

Institut de recherche en astrophysique et planétologie

N. Mostek

Function : Author

O. Steele

Function : Author

E. Aubourg

Function : Author
PersonId : 14010
IdHAL : eric-aubourg
ORCID : 0000-0002-5592-023X
IdRef : 078069823

APC - Cosmologie

AstroParticule et Cosmologie

S. Bailey

Function : Author

A.-S. Bolton

Function : Author

J. Brownstein

Function : Author

K. Dawson

Function : Author

A. Leauthaud

Function : Author

C. Maraston

Function : Author

W. Percival

Function : Author

N.-P. Ross

Function : Author

D.-J. Schlegel

Function : Author

D.-P. Schneider

Function : Author

D. Thomas

Function : Author

J.-L. Tinker

Function : Author

B.-A. Weaver

Function : Author

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

Domains

Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]

Danielle Cristofol : Connect in order to contact the contributor

https://in2p3.hal.science/in2p3-00719510

Submitted on : Friday, July 20, 2012-9:23:28 AM

Last modification on : Thursday, June 20, 2024-8:36:04 AM

Dates and versions

in2p3-00719510 , version 1 (20-07-2012)

Identifiers

HAL Id : in2p3-00719510 , version 1
ARXIV : 1207.4321
BIBCODE : 2013MNRAS.428.1498C
DOI : 10.1093/mnras/sts127

Cite

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, 2013, 428 (2), pp.1498-1517. ⟨10.1093/mnras/sts127⟩. ⟨in2p3-00719510⟩

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

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