The 2dF Galaxy Redshift Survey: Higher-order galaxy correlation functions

We 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 hierarchic...

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Հիմնական հեղինակներ: Croton, D, Gaztañaga, E, Baugh, C, Norberg, P, Colless, M, Baldry, L, Bland-Hawthorn, J, Bridges, T, Cannon, R, Cole, S, Collins, C, Couch, W, Dalton, G, De Propris, R, Driver, S, Efstathiou, G, Ellis, R, Frenk, C, Glazebrook, K, Jackson, C, Lahav, O, Lewis, I, Lumsden, S, Maddox, S, Madgwick, D
Ձևաչափ: Journal article
Լեզու:English
Հրապարակվել է: 2004
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author Croton, D
Gaztañaga, E
Baugh, C
Norberg, P
Colless, M
Baldry, L
Bland-Hawthorn, J
Bridges, T
Cannon, R
Cole, S
Collins, C
Couch, W
Dalton, G
De Propris, R
Driver, S
Efstathiou, G
Ellis, R
Frenk, C
Glazebrook, K
Jackson, C
Lahav, O
Lewis, I
Lumsden, S
Maddox, S
Madgwick, D
author_facet Croton, D
Gaztañaga, E
Baugh, C
Norberg, P
Colless, M
Baldry, L
Bland-Hawthorn, J
Bridges, T
Cannon, R
Cole, S
Collins, C
Couch, W
Dalton, G
De Propris, R
Driver, S
Efstathiou, G
Ellis, R
Frenk, C
Glazebrook, K
Jackson, C
Lahav, O
Lewis, I
Lumsden, S
Maddox, S
Madgwick, D
author_sort Croton, D
collection OXFORD
description We 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.
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spelling oxford-uuid:4ed2803b-44e7-46df-bfdb-12823931a23d2022-03-26T16:03:30ZThe 2dF Galaxy Redshift Survey: Higher-order galaxy correlation functionsJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:4ed2803b-44e7-46df-bfdb-12823931a23dEnglishSymplectic Elements at Oxford2004Croton, DGaztañaga, EBaugh, CNorberg, PColless, MBaldry, LBland-Hawthorn, JBridges, TCannon, RCole, SCollins, CCouch, WDalton, GDe Propris, RDriver, SEfstathiou, GEllis, RFrenk, CGlazebrook, KJackson, CLahav, OLewis, ILumsden, SMaddox, SMadgwick, DWe 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.
spellingShingle Croton, D
Gaztañaga, E
Baugh, C
Norberg, P
Colless, M
Baldry, L
Bland-Hawthorn, J
Bridges, T
Cannon, R
Cole, S
Collins, C
Couch, W
Dalton, G
De Propris, R
Driver, S
Efstathiou, G
Ellis, R
Frenk, C
Glazebrook, K
Jackson, C
Lahav, O
Lewis, I
Lumsden, S
Maddox, S
Madgwick, D
The 2dF Galaxy Redshift Survey: Higher-order galaxy correlation functions
title The 2dF Galaxy Redshift Survey: Higher-order galaxy correlation functions
title_full The 2dF Galaxy Redshift Survey: Higher-order galaxy correlation functions
title_fullStr The 2dF Galaxy Redshift Survey: Higher-order galaxy correlation functions
title_full_unstemmed The 2dF Galaxy Redshift Survey: Higher-order galaxy correlation functions
title_short The 2dF Galaxy Redshift Survey: Higher-order galaxy correlation functions
title_sort 2df galaxy redshift survey higher order galaxy correlation functions
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