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dc.contributor.authorSánchez, Ariel G.
dc.contributor.authorMontesano, Francesco
dc.contributor.authorKazin, Eyal A.
dc.contributor.authorAubourg, Eric
dc.contributor.authorBeutler, Florian
dc.contributor.authorBrinkmann, Jon
dc.contributor.authorBrownstein, Joel R.
dc.contributor.authorCuesta, Antonio J.
dc.contributor.authorDawson, Kyle S.
dc.contributor.authorEisenstein, Daniel J.
dc.contributor.authorHo, Shirley
dc.contributor.authorHonscheid, Klaus
dc.contributor.authorManera, Marc
dc.contributor.authorMaraston, Claudia
dc.contributor.authorMcBride, Cameron K.
dc.contributor.authorPercival, Will J.
dc.contributor.authorRoss, Ashley J.
dc.contributor.authorSamushia, Lado
dc.contributor.authorSchlegel, David J.
dc.contributor.authorSchneider, Donald P.
dc.contributor.authorSkibba, Ramin
dc.contributor.authorThomas, Daniel
dc.contributor.authorTinker, Jeremy L.
dc.contributor.authorTojeiro, Rita
dc.contributor.authorWake, David A.
dc.contributor.authorWeaver, Benjamin A.
dc.contributor.authorWhite, Martin
dc.contributor.authorZehavi, Idit
dc.identifier.citationSánchez , A G , Montesano , F , Kazin , E A , Aubourg , E , Beutler , F , Brinkmann , J , Brownstein , J R , Cuesta , A J , Dawson , K S , Eisenstein , D J , Ho , S , Honscheid , K , Manera , M , Maraston , C , McBride , C K , Percival , W J , Ross , A J , Samushia , L , Schlegel , D J , Schneider , D P , Skibba , R , Thomas , D , Tinker , J L , Tojeiro , R , Wake , D A , Weaver , B A , White , M & Zehavi , I 2014 , ' The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey : cosmological implications of the full shape of the clustering wedges in the data release 10 and 11 galaxy samples ' , Monthly Notices of the Royal Astronomical Society , vol. 440 , no. 3 , pp. 2692-2713 .
dc.identifier.otherPURE: 157307454
dc.identifier.otherPURE UUID: 746daff8-77df-4ac9-a4b6-6029cae2cc46
dc.identifier.otherBibCode: 2014MNRAS.440.2692S
dc.identifier.otherScopus: 84898782040
dc.description.abstractWe explore the cosmological implications of the angle-averaged correlation function, ξ(s), and the clustering wedges, ξ⊥(s) and ξ∥(s), of the LOWZ and CMASS galaxy samples from Data Releases 10 and 11 of the Sloan Digital Sky Survey III (SDSS-III) Baryon Oscillation Spectroscopic Survey. Our results show no significant evidence for a deviation from the standard Λ cold dark matter model. The combination of the information from our clustering measurements with recent data from the cosmic microwave background is sufficient to constrain the curvature of the Universe to Ωk = 0.0010 ± 0.0029, the total neutrino mass to ∑mν < 0.23 eV (95 per cent confidence level), the effective number of relativistic species to Neff = 3.31 ± 0.27 and the dark energy equation of state to wDE = −1.051 ± 0.076. These limits are further improved by adding information from Type Ia supernovae and baryon acoustic oscillations from other samples. In particular, this data set combination is completely consistent with a time-independent dark energy equation of state, in which case we find wDE = −1.024 ± 0.052. We explore the constraints on the growth rate of cosmic structures assuming f(z) = Ωm(z)γ and obtain γ = 0.69 ± 0.15, consistent with the predictions of general relativity of γ = 0.55.
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rightsThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society, © 2014 The Authors, Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.en
dc.subjectcosmological parametersen
dc.subjectlarge-scale structure of Universeen
dc.titleThe clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey : cosmological implications of the full shape of the clustering wedges in the data release 10 and 11 galaxy samplesen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.description.statusPeer revieweden

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