Probing dark energy with baryonic acoustic oscillations at high redshifts

2006/09/13 by R. Koehler, Ralf S. Koehler, P. Schuecker +2 · 24 citations
Physics and Astronomy · #Amplitude #Astrophysics #Baryon #Baryon acoustic oscillations #Context (archaeology) #Cosmology #Cosmology and Gravitation Theories #Dark energy #Galaxies: Formation, Evolution, Phenomena #Galaxy #Matter power spectrum #Physics #Quantum mechanics #Radio Astronomy Observations and Technology #Redshift #Redshift survey #Redshift-space distortions #Spectral density #astro-ph

paper · pdf · doi:10.1051/0004-6361:20065649

published in Astronomy and Astrophysics 462(1), 7-20 (EDP Sciences) · accepted for publication in Astron. Astrophys., 16 pages, 16 figures

arxiv created 2006/09/13 · openalex publication_date 2006/10/24 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Context.The phases and amplitudes of baryonic acoustic oscillations in the galaxy power spectrum can be used as cosmological probes to constrain different cosmological models and especially the equation of state parameter w of dark energy.

Citations

• The nature of galaxy bias and clustering
• Simulations of the formation, evolution and clustering of galaxies and quasars
• The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications

Cited by

• THE HETDEX PILOT SURVEY. I. SURVEY DESIGN, PERFORMANCE, AND CATALOG OF EMISSION-LINE GALAXIES