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Authordc.contributor.authorPâris, Isabelle 
Admission datedc.date.accessioned2014-01-24T14:25:44Z
Available datedc.date.available2014-01-24T14:25:44Z
Publication datedc.date.issued2013-03
Identifierdc.identifier.otherdoi:10.1088/1475-7516/2013/03/024
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/126276
General notedc.descriptionArtículo de publicación ISI.en_US
Abstractdc.description.abstractWe describe tting methods developed to analyze uctuations in the Lyman- forest and measure the parameters of baryon acoustic oscillations (BAO). We apply our methods to BOSS Data Release 9. Our method is based on models of the three-dimensional correlation function in physical coordinate space, and includes the e ects of redshift-space distortions, anisotropic non-linear broadening, and broadband distortions. We allow for independent scale factors along and perpendicular to the line of sight to minimize the dependence on our assumed ducial cosmology and to obtain separate measurements of the BAO angular and relative velocity scales. Our tting software and the input les needed to reproduce our main BOSS Data Release 9 results are publicly available.en_US
Patrocinadordc.description.sponsorshipAlfred P. Sloan Foundationen_US
Lenguagedc.language.isoenen_US
Publisherdc.publisherIOP Publishing Ltd and Sissa Medialab srlen_US
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Keywordsdc.subjectdark energy experimentsen_US
Títulodc.titleFitting methods for baryon acoustic oscillations in the Lyman-en_US
Document typedc.typeArtículo de revista


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Attribution-NonCommercial-NoDerivs 3.0 Chile
Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile