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dc.contributor.authorVargas-Magaña, Mariana
dc.contributor.authorHo, Shirley
dc.contributor.authorCuesta, Antonio J.
dc.contributor.authorO'Connell, Ross
dc.contributor.authorRoss, Ashley J.
dc.contributor.authorEisenstein, Daniel J.
dc.contributor.authorPercival, Will J.
dc.contributor.authorGrieb, Jan Niklas
dc.contributor.authorSánchez, Ariel G.
dc.contributor.authorTinker, Jeremy L.
dc.contributor.authorTojeiro, Rita
dc.contributor.authorBeutler, Florian
dc.contributor.authorChuang, Chia-Hsun
dc.contributor.authorKitaura, Francisco-Shu
dc.contributor.authorPrada, Francisco
dc.contributor.authorRodríguez-Torres, Sergio A.
dc.contributor.authorRossi, Graziano
dc.contributor.authorSeo, Hee-Jong
dc.contributor.authorBrownstein, Joel R.
dc.contributor.authorOlmstead, Matthew
dc.contributor.authorThomas, Daniel
dc.identifier.citationVargas-Magaña , M , Ho , S , Cuesta , A J , O'Connell , R , Ross , A J , Eisenstein , D J , Percival , W J , Grieb , J N , Sánchez , A G , Tinker , J L , Tojeiro , R , Beutler , F , Chuang , C-H , Kitaura , F-S , Prada , F , Rodríguez-Torres , S A , Rossi , G , Seo , H-J , Brownstein , J R , Olmstead , M & Thomas , D 2018 , ' The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey : theoretical systematics and Baryon Acoustic Oscillations in the galaxy correlation function ' , Monthly Notices of the Royal Astronomical Society , vol. 477 , no. 1 , pp. 1153-1188 .
dc.description.abstractWe investigate the potential sources of theoretical systematics in the anisotropic Baryon Acoustic Oscillation (BAO) distance scale measurements from the clustering of galaxies in configuration space using the final Data Release (DR12) of the Baryon Oscillation Spectroscopic Survey (BOSS). We perform a detailed study of the impact on BAO measurements from choices in the methodology such as fiducial cosmology, clustering estimators, random catalogues, fitting templates, and covariance matrices. The theoretical systematic uncertainties in BAO parameters are found to be 0.002 in the isotropic dilation α and 0.003 in the quadrupolar dilation ε. The leading source of systematic uncertainty is related to the reconstruction techniques. Theoretical uncertainties are sub-dominant compared with the statistical uncertainties for BOSS survey, accounting 0.2σstat for α and 0.25σstat for ε (σα, stat ∼ 0.010 and σε, stat ∼ 0.012, respectively). We also present BAO-only distance scale constraints from the anisotropic analysis of the correlation function. Our constraints on the angular diameter distance DA(z) and the Hubble parameter H(z), including both statistical and theoretical systematic uncertainties, are 1.5 per cent and 2.8 per cent at zeff = 0.38, 1.4 per cent and 2.4 per cent at zeff = 0.51, and 1.7 per cent and 2.6 per cent at zeff = 0.61. This paper is part of a set that analyses the final galaxy clustering data set from BOSS. The measurements and likelihoods presented here are cross-checked with other BAO analysis in Alam et al. The systematic error budget concerning the methodology on post-reconstruction BAO analysis presented here is used in Alam et al. to produce the final cosmological constraints from BOSS.
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.subjectGalaxies: distance and redshiftsen
dc.subjectCosmology: observationsen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.titleThe clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey : theoretical systematics and Baryon Acoustic Oscillations in the galaxy correlation functionen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.description.statusPeer revieweden

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