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dc.contributor.authorSánchez, Ariel G.
dc.contributor.authorKazin, Eyal A.
dc.contributor.authorBeutler, Florian
dc.contributor.authorChuang, Chia-Hsun
dc.contributor.authorCuesta, Antonio J.
dc.contributor.authorEisenstein, Daniel J.
dc.contributor.authorManera, Marc
dc.contributor.authorMontesano, Francesco
dc.contributor.authorNichol, Robert C.
dc.contributor.authorPadmanabhan, Nikhil
dc.contributor.authorPercival, Will
dc.contributor.authorPrada, Francisco
dc.contributor.authorRoss, Ashley J.
dc.contributor.authorSchlegel, David J.
dc.contributor.authorTinker, Jeremy
dc.contributor.authorTojeiro, Rita
dc.contributor.authorWeinberg, David H.
dc.contributor.authorXu, Xiaoying
dc.contributor.authorBrinkmann, J.
dc.contributor.authorBrownstein, Joel R.
dc.contributor.authorSchneider, Donald P.
dc.contributor.authorThomas, Daniel
dc.identifier.citationSánchez , A G , Kazin , E A , Beutler , F , Chuang , C-H , Cuesta , A J , Eisenstein , D J , Manera , M , Montesano , F , Nichol , R C , Padmanabhan , N , Percival , W , Prada , F , Ross , A J , Schlegel , D J , Tinker , J , Tojeiro , R , Weinberg , D H , Xu , X , Brinkmann , J , Brownstein , J R , Schneider , D P & Thomas , D 2013 , ' The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey : cosmological constraints from the full shape of the clustering wedges ' , Monthly Notices of the Royal Astronomical Society , vol. 433 , no. 2 , pp. 1202-1222 .
dc.identifier.otherPURE: 171421018
dc.identifier.otherPURE UUID: a7bc1ce2-0e31-4bd3-ad27-0123cae7977c
dc.identifier.otherBibCode: 2013MNRAS.433.1202S
dc.identifier.otherScopus: 84880411798
dc.description.abstractWe explore the cosmological implications of the clustering wedges, ξ⊥(s) and ξ∥(s), of the CMASS Data Release 9 sample of the Sloan Digital Sky Survey III (SDSS-III) Baryon Oscillation Spectroscopic Survey. These clustering wedges are defined by averaging the full two-dimensional correlation function, ξ(μ, s),over the ranges 0 <μ <0.5 and 0.5 <μ <1,respectively. These measurements allow us to constrain the parameter combinations DA(z)/rs(zd) = 9.03± 0.21 and cz/(rs(zd)H(z)) = 12.14 ±0.43 at the mean redshift of the sample, z = 0.57. We combine the information from the clustering wedges with recent measurements of cosmic microwave background (CMB), baryon acoustic oscillations and TypeIa supernovae to obtain constraints on the cosmological parameters of the standard Λ cold dark matter (ΛCDM) model and a number of potential extensions. The information encoded in the clustering wedges is most useful when the dark energy equation of state is allowed to deviate from its standard ΛCDM value. The combination of all data sets shows no evidence of a deviation from a constant dark energy equation of state, in which case we find wDE = -1.013± 0.064, in complete agreement with a cosmological constant. We explore potential deviations from general relativity (GR) by constraining the growth rate f(z) = d ln D(a)/d ln a, in which case the combination of the CMASS clustering wedges with CMB data implies f(z =0.57) = 0.719-0.096+0.092, in accordance with the predictions of GR. Our results clearly illustrate the additional constraining power of anisotropic clustering measurements with respectt o that of angle-averaged quantities.
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rightsCopyright © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. This work is made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at:
dc.subjectCosmological parametersen
dc.subjectLarge-scale structure of Universeen
dc.subjectQB Astronomyen
dc.titleThe clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey : cosmological constraints from the full shape of the clustering wedgesen
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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