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dc.contributor.authorWang, Dandan
dc.contributor.authorZhao, Gong-Bo
dc.contributor.authorWang, Yuting
dc.contributor.authorPercival, Will J.
dc.contributor.authorRuggeri, Rossana
dc.contributor.authorZhu, Fangzhou
dc.contributor.authorTojeiro, Rita
dc.contributor.authorMyers, Adam D.
dc.contributor.authorChuang, Chia-Hsun
dc.contributor.authorBaumgarten, Falk
dc.contributor.authorZhao, Cheng
dc.contributor.authorGil-Marín, Héctor
dc.contributor.authorRoss, Ashley J.
dc.contributor.authorBurtin, Etienne
dc.contributor.authorZarrouk, Pauline
dc.contributor.authorBautista, Julian
dc.contributor.authorBrinkmann, Jonathan
dc.contributor.authorDawson, Kyle
dc.contributor.authorBrownstein, Joel R.
dc.contributor.authorde la Macorra, Axel
dc.contributor.authorSchneider, Donald P.
dc.contributor.authorShafieloo, Arman
dc.date.accessioned2018-03-16T09:30:10Z
dc.date.available2018-03-16T09:30:10Z
dc.date.issued2018-03-10
dc.identifier.citationWang , D , Zhao , G-B , Wang , Y , Percival , W J , Ruggeri , R , Zhu , F , Tojeiro , R , Myers , A D , Chuang , C-H , Baumgarten , F , Zhao , C , Gil-Marín , H , Ross , A J , Burtin , E , Zarrouk , P , Bautista , J , Brinkmann , J , Dawson , K , Brownstein , J R , de la Macorra , A , Schneider , D P & Shafieloo , A 2018 , ' The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample : anisotropic Baryon Acoustic Oscillations measurements in Fourier-space with optimal redshift weights ' Monthly Notices of the Royal Astronomical Society . https://doi.org/10.1093/mnras/sty654en
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 252360418
dc.identifier.otherPURE UUID: 48db13ce-f1b9-4e80-9c64-17304ddf01c1
dc.identifier.otherBibCode: 2018arXiv180103077W
dc.identifier.otherScopus: 85047131177
dc.identifier.urihttps://arxiv.org/abs/1801.03077en
dc.identifier.urihttp://adsabs.harvard.edu/abs/2018arXiv180103077Wen
dc.description.abstractWe present a measurement of the anisotropic and isotropic Baryon Acoustic Oscillations (BAO) from the extended Baryon Oscillation Spectroscopic Survey Data Release 14 quasar sample with optimal redshift weights. Applying the redshift weights improves the constraint on the BAO dilation parameter α(zeff) by 17%. We reconstruct the evolution history of the BAO distance indicators in the redshift rangeof 0.8 < z < 2.2. This paper is part of a set that analyses the eBOSS DR14 quasar sample.
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rights© 2018, the Author(s). This work has been made available online in accordance with the publisher’s policies. This is the author created, accepted version manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at https://doi.org/10.1093/mnras/sty654en
dc.subjectBaryon acoustic oscillationsen
dc.subjectOptimal redshift weightingen
dc.subjectDark energyen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleThe clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample : anisotropic Baryon Acoustic Oscillations measurements in Fourier-space with optimal redshift weightsen
dc.typeJournal articleen
dc.description.versionPreprinten
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1093/mnras/sty654
dc.description.statusPeer revieweden


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