The WiggleZ Dark Energy Survey: constraining galaxy bias and cosmic growth with three-point correlation functions

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dc.contributor.authorMarin, Felipe
dc.contributor.authorBlake, Chris
dc.contributor.authorPoole, Gregory B
dc.contributor.authorMcBride, Cameron K
dc.contributor.authorBrough, Sarah
dc.contributor.authorColless, Matthew
dc.contributor.authorContreras, Carlos
dc.contributor.authorCouch, Warrick
dc.contributor.authorCroton, Darren
dc.contributor.authorCroom, S
dc.contributor.authorSharp, Robert
dc.contributor.authorForster, Karl
dc.contributor.authorGilbank, David
dc.contributor.authorMadore, Barry
dc.contributor.authorWyder, Ted
dc.date.accessioned2015-12-13T22:29:11Z
dc.date.issued2013
dc.date.updated2016-02-24T09:22:43Z
dc.description.abstractHigher order statistics are a useful and complementary tool for measuring the clustering of galaxies, containing information on the non-Gaussian evolution and morphology of large-scale structure in the Universe. In this work we present measurements of the
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/74571
dc.publisherBlackwell Publishing Ltd
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Methods; Observations - large-scale structure of - Universe; Statistical - cosmological parameters - cosmology
dc.titleThe WiggleZ Dark Energy Survey: constraining galaxy bias and cosmic growth with three-point correlation functions
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue4
local.bibliographicCitation.lastpage2668
local.bibliographicCitation.startpage2654
local.contributor.affiliationMarin, Felipe, Swinburne University of Technology
local.contributor.affiliationBlake, Chris, Swinburne University of Technology
local.contributor.affiliationPoole, Gregory B, Swinburne University of Technology
local.contributor.affiliationMcBride, Cameron K, Harvard-Smithsonian Center for Astrophysics
local.contributor.affiliationBrough, Sarah, Australian Astronomical Observatory
local.contributor.affiliationColless, Matthew, Australian Astronomical Observatory
local.contributor.affiliationContreras, Carlos, Swinburne University of Technology
local.contributor.affiliationCouch, Warrick, Swinburne University of Technology
local.contributor.affiliationCroton, Darren, Swinburne University of Technology
local.contributor.affiliationCroom, S, University of Sydney
local.contributor.affiliationSharp, Robert, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationForster, Karl, California Institute of Technology
local.contributor.affiliationGilbank, David, South African Astronomical Observatory
local.contributor.affiliationMadore, Barry, Observatories of the Carnegie Institution of Washington
local.contributor.affiliationWyder, Ted, California Institute of Technology
local.contributor.authoruidSharp, Robert, u4954956
local.description.notesImported from ARIES
local.identifier.absfor020103 - Cosmology and Extragalactic Astronomy
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationf5625xPUB4191
local.identifier.ariespublicationu4630950xPUB76
local.identifier.citationvolume432
local.identifier.doi10.1093/mnras/stt520
local.identifier.scopusID2-s2.0-84880022878
local.identifier.thomsonID000321053500005
local.type.statusPublished Version

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