The 2dF galaxy Redshift Survey: higher-order glaxy correlation functions

dc.contributor.authorCroton, Darren J
dc.contributor.authorGaztanaga, Enrique
dc.contributor.authorBaugh, Carlton M
dc.contributor.authorNorberg, Peder
dc.contributor.authorColless, Matthew
dc.contributor.authorBaldry, Ivan K
dc.contributor.authorBland-Hawthorn, Joss
dc.contributor.authorBridges, Terry C
dc.contributor.authorCannon, Russell
dc.contributor.authorCole, Shaun
dc.contributor.authorCollins, Chris
dc.contributor.authorCouch, Warrick
dc.contributor.authorDalton, Gavin
dc.contributor.authorDe Propris, Roberto
dc.contributor.authorDriver, Simon
dc.contributor.authorEfstathiou, George
dc.contributor.authorEllis, Richard S
dc.contributor.authorFrenk, Carlos S
dc.contributor.authorGlazebrook, Karl
dc.contributor.authorJackson, Carole A
dc.contributor.authorLahav, Ofer
dc.contributor.authorLewis, Ian
dc.contributor.authorLumsden, Stuart
dc.contributor.authorMaddox, Steve J
dc.contributor.authorMadgwick, Darren
dc.contributor.authorPeacock, John A
dc.contributor.authorPeterson, Bruce
dc.contributor.authorSutherland, William J
dc.contributor.authorTaylor, Keith
dc.date.accessioned2015-12-13T23:10:12Z
dc.date.available2015-12-13T23:10:12Z
dc.date.issued2004
dc.date.updated2015-12-12T08:22:53Z
dc.description.abstractWe measure moments of the galaxy count probability distribution function in the Two-degree Field Galaxy Redshift Survey (2dFGRS). The survey is divided into volume-limited subsamples in order to examine the dependence of the higher-order clustering on galaxy luminosity. We demonstrate the hierarchical scaling of the averaged p-point galaxy correlation functions, ξ̄ p, up to p = 6. The hierarchical amplitudes, S p = S 2S p-1, are approximately independent of the cell radius used to smooth the galaxy distribution on small to medium scales. On larger scales we find that the higher-order moments can be strongly affected by the presence of rare, massive superstructures in the galaxy distribution. The skewness S 3 has a weak dependence on luminosity, approximated by a linear dependence on log luminosity. We discuss the implications of our results for simple models of linear and non-linear bias that relate the galaxy distribution to the underlying mass.
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/87346
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Cosmology: theory; Galaxies: statistics; Large-scale structure of Universe
dc.titleThe 2dF galaxy Redshift Survey: higher-order glaxy correlation functions
dc.typeJournal article
local.bibliographicCitation.lastpage1244
local.bibliographicCitation.startpage1232
local.contributor.affiliationCroton, Darren J, Max Planck Institute for Astrophysics
local.contributor.affiliationGaztanaga, Enrique, University of Durham
local.contributor.affiliationBaugh, Carlton M, University of Durham
local.contributor.affiliationNorberg, Peder, Swiss Federal Institute of Technology (ETH)
local.contributor.affiliationColless, Matthew, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationBaldry, Ivan K, Johns Hopkins University
local.contributor.affiliationBland-Hawthorn, Joss, Anglo-Australian Observatory
local.contributor.affiliationBridges, Terry C, Queen's University
local.contributor.affiliationCannon, Russell, Anglo-Australian Observatory
local.contributor.affiliationCole, Shaun, University of Durham
local.contributor.affiliationCollins, Chris, Liverpool John Moores University
local.contributor.affiliationCouch, Warrick, University of New South Wales
local.contributor.affiliationDalton, Gavin, University of Oxford
local.contributor.affiliationDe Propris, Roberto, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationDriver, Simon, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationEfstathiou, George, University of Cambridge
local.contributor.affiliationEllis, Richard S, California Institute of Technology
local.contributor.affiliationFrenk, Carlos S, University of Durham
local.contributor.affiliationGlazebrook, Karl, Johns Hopkins University
local.contributor.affiliationJackson, Carole A, CSIRO, Australia Telescope National Facility
local.contributor.affiliationLahav, Ofer, University of Cambridge
local.contributor.affiliationLewis, Ian, University of Oxford
local.contributor.affiliationLumsden, Stuart, University of Leeds
local.contributor.affiliationMaddox, Steve J, University of Nottingham
local.contributor.affiliationMadgwick, Darren, University of California
local.contributor.affiliationPeacock, John A, University of Edinburgh
local.contributor.affiliationPeterson, Bruce, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSutherland, William J, University of Cambridge
local.contributor.affiliationTaylor, Keith, Anglo-Australian Observatory
local.contributor.authoremailu9300169@anu.edu.au
local.contributor.authoruidColless, Matthew, u9300169
local.contributor.authoruidDe Propris, Roberto, u4039665
local.contributor.authoruidDriver, Simon, u4041024
local.contributor.authoruidPeterson, Bruce, u8000960
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub16590
local.identifier.citationvolume352
local.identifier.doi10.1111/j.1365-2966.2004.08017.x
local.identifier.scopusID2-s2.0-4344715538
local.identifier.uidSubmittedByMigrated
local.type.statusPublished Version

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