Acoustic oscillations in the SDSS DR4 Luminous Red Galaxy sample power spectrum

dc.creatorHuetsi, Gert
dc.date2005-12-07
dc.date.accessioned2026-07-07T11:42:28Z
dc.date.available2026-07-07T11:42:28Z
dc.descriptionWe calculate the redshift-space power spectrum of the Sloan Digital Sky Survey (SDSS) Data Release 4 (DR4) Luminous Red Galaxy (LRG) sample, finding evidence for a full series of acoustic features down to the scales of \sim 0.2 hMpc^{-1}. This corresponds up to the 7th peak in the CMB angular power spectrum. The acoustic scale derived, (105.4 \pm 2.3) h^{-1}Mpc, agrees very well with the ``concordance'' model prediction and also with the one determined via the analysis of the spatial two-point correlation function by Eisenstein et al. (2005). The models with baryonic features are favored by 3.3 σover their ``smoothed-out'' counterparts without any oscillatory behavior.
dc.descriptionExtended version of the previous work astro-ph/0507678, now including new data from the SDSS DR4. 17 pages, 18 figures, accepted for publication in A&A
dc.identifierhttps://arxiv.org/abs/astro-ph/0512201
dc.identifierhttp://arxiv.org/abs/astro-ph/0512201
dc.identifierAstron.Astrophys.449:891-902,2006
dc.identifierdoi:10.1051/0004-6361:20053939
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/200897
dc.subjectAstrophysics
dc.titleAcoustic oscillations in the SDSS DR4 Luminous Red Galaxy sample power spectrum
dc.typetext

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