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Article: The 6dF Galaxy Survey: Z≈ 0 measurements of the growth rate and σ 8

TitleThe 6dF Galaxy Survey: Z≈ 0 measurements of the growth rate and σ 8
Authors
KeywordsCosmological parameters
Cosmology: observations
Surveys
Galaxies: statistics
Large-scale structure of Universe
Issue Date2012
Citation
Monthly Notices of the Royal Astronomical Society, 2012, v. 423, n. 4, p. 3430-3444 How to Cite?
AbstractWe present a detailed analysis of redshift-space distortions in the two-point correlation function of the 6dF Galaxy Survey (6dFGS). The K-band selected subsample which we employ in this study contains 81971 galaxies distributed over 17000degree 2 with an effective redshift z eff= 0.067. By modelling the 2D galaxy correlation function, , we measure the parameter combination f(z eff)σ 8(z eff) = 0.423 ± 0.055, where is the growth rate of cosmic structure and σ 8 is the rms of matter fluctuations in 8h -1Mpc spheres. Alternatively, by assuming standard gravity we can break the degeneracy between σ 8 and the galaxy bias parameter b. Combining our data with the Hubble constant prior from Riess et al., we measure σ 8= 0.76 ± 0.11 and Ω m= 0.250 ± 0.022, consistent with constraints from other galaxy surveys and the cosmic microwave background data from Wilkinson Microwave Anisotropy Probe 7 (WMAP7). Combining our measurement of fσ 8 with WMAP7 allows us to test the cosmic growth history and the relationship between matter and gravity on cosmic scales by constraining the growth index of density fluctuations, γ. Using only 6dFGS and WMAP7 data we find γ= 0.547 ± 0.088, consistent with the prediction of General Relativity. We note that because of the low effective redshift of the 6dFGS our measurement of the growth rate is independent of the fiducial cosmological model (Alcock-Paczynski effect). We also show that our conclusions are not sensitive to the model adopted for non-linear redshift-space distortions. Using a Fisher matrix analysis we report predictions for constraints on fσ 8 for the Wide-field Australian SKA Pathfinder telescope L-band Legacy All-sky Blind surveY (WALLABY) and the proposed Transforming Astronomical Imaging surveys through Polychromatic Analysis of Nebulae (TAIPAN) survey. The WALLABY survey will be able to measure fσ 8 with a precision of 4-10 percent, depending on the modelling of non-linear structure formation. This is comparable to the predicted precision for the best redshift bins of the Baryon Oscillation Spectroscopic Survey, demonstrating that low-redshift surveys have a significant role to play in future tests of dark energy and modified gravity. © 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS.
Persistent Identifierhttp://hdl.handle.net/10722/208940
ISSN
2015 Impact Factor: 4.952
2015 SCImago Journal Rankings: 2.806

 

DC FieldValueLanguage
dc.contributor.authorBeutler, Florian-
dc.contributor.authorBlake, Chris A.-
dc.contributor.authorColless, Matthew-
dc.contributor.authorJones, Daniel Heath-
dc.contributor.authorStaveley-Smith, Lister-
dc.contributor.authorPoole, Gregory B.-
dc.contributor.authorCampbell, Lachlan A.-
dc.contributor.authorParker, Quentin A.-
dc.contributor.authorSaunders, Will J.-
dc.contributor.authorWatson, Fred G.-
dc.date.accessioned2015-03-23T02:02:17Z-
dc.date.available2015-03-23T02:02:17Z-
dc.date.issued2012-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2012, v. 423, n. 4, p. 3430-3444-
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/10722/208940-
dc.description.abstractWe present a detailed analysis of redshift-space distortions in the two-point correlation function of the 6dF Galaxy Survey (6dFGS). The K-band selected subsample which we employ in this study contains 81971 galaxies distributed over 17000degree 2 with an effective redshift z eff= 0.067. By modelling the 2D galaxy correlation function, , we measure the parameter combination f(z eff)σ 8(z eff) = 0.423 ± 0.055, where is the growth rate of cosmic structure and σ 8 is the rms of matter fluctuations in 8h -1Mpc spheres. Alternatively, by assuming standard gravity we can break the degeneracy between σ 8 and the galaxy bias parameter b. Combining our data with the Hubble constant prior from Riess et al., we measure σ 8= 0.76 ± 0.11 and Ω m= 0.250 ± 0.022, consistent with constraints from other galaxy surveys and the cosmic microwave background data from Wilkinson Microwave Anisotropy Probe 7 (WMAP7). Combining our measurement of fσ 8 with WMAP7 allows us to test the cosmic growth history and the relationship between matter and gravity on cosmic scales by constraining the growth index of density fluctuations, γ. Using only 6dFGS and WMAP7 data we find γ= 0.547 ± 0.088, consistent with the prediction of General Relativity. We note that because of the low effective redshift of the 6dFGS our measurement of the growth rate is independent of the fiducial cosmological model (Alcock-Paczynski effect). We also show that our conclusions are not sensitive to the model adopted for non-linear redshift-space distortions. Using a Fisher matrix analysis we report predictions for constraints on fσ 8 for the Wide-field Australian SKA Pathfinder telescope L-band Legacy All-sky Blind surveY (WALLABY) and the proposed Transforming Astronomical Imaging surveys through Polychromatic Analysis of Nebulae (TAIPAN) survey. The WALLABY survey will be able to measure fσ 8 with a precision of 4-10 percent, depending on the modelling of non-linear structure formation. This is comparable to the predicted precision for the best redshift bins of the Baryon Oscillation Spectroscopic Survey, demonstrating that low-redshift surveys have a significant role to play in future tests of dark energy and modified gravity. © 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS.-
dc.languageeng-
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society-
dc.subjectCosmological parameters-
dc.subjectCosmology: observations-
dc.subjectSurveys-
dc.subjectGalaxies: statistics-
dc.subjectLarge-scale structure of Universe-
dc.titleThe 6dF Galaxy Survey: Z≈ 0 measurements of the growth rate and σ 8-
dc.typeArticle-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1111/j.1365-2966.2012.21136.x-
dc.identifier.scopuseid_2-s2.0-84863630347-
dc.identifier.volume423-
dc.identifier.issue4-
dc.identifier.spage3430-
dc.identifier.epage3444-
dc.identifier.eissn1365-2966-

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