51猎奇入口

Skip to main content
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • 51猎奇入口
    • Undergraduates
    • Postgraduates
  • Engage
    • For young people
    • For teachers
    • For the public
    • For alumni
    • For business
  • Support
Menu
Part of a WEAVE fibre configuration

Part of the WEAVE focal plane showing optical fibres positioned on a set of targets in the telescope focal plane.

Prof Gavin Dalton

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Astronomical instrumentation
  • Extremely Large Telescope
Gavin.Dalton@physics.ox.ac.uk
  • About
  • Research
  • Publications

The richness dependence of galaxy cluster correlations: results from a redshift survey of rich APM clusters

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 291:2 (1997) 305-313

Authors:

RAC Croft, GB Dalton, G Efstathiou, WJ Sutherland, SJ Maddox

X-ray QSO evolution from a very deep ROSAT survey

(1996)

Authors:

LR Jones, IM McHardy, MR Merrifield, KO Mason, PJ Smith, RG Abraham, G Branduardi-Raymont, AM Newsam, G Dalton, M Rowan-Robinson, G Luppino

Higher order statistics from the APM galaxy survey

Astrophysical Journal 444:2 (1995) 520-531

Authors:

I Szapudi, GB Dalton, G Efstathiou, AS Szalay

Abstract:

We apply a new statistics, the factorial moment correlators, to density maps obtained from the APM survey The resulting correlators are all proportional to the two-point correlation function, substantially amplified with an amplification nearly exponential with the total rank of the correlators. This confirms the validity of the hierarchical clustering assumption on the dynamic range examined, corresponding to 0.5-50 h-1 Mpc in three-dimensional space. The Kirkwood superposition with loop terms is strongly rejected. The structure coefficients of the hierarchy are also fitted. The high quality of the APM catalog enabled us to disentangle the various contributions from the power spectrum, small-scale nonlinear clustering, and combinatorial effects, all of which affect the amplification of the correlators. These effects should appear in correlations of clusters in a similar fashion.

Erratum - the APM Galaxy Survey - Part Four - Redshifts of Rich Clusters of Galaxies

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 273:2 (1995) 528-528

Authors:

GB Dalton, G Efstathiou, SJ Maddox, WJ Sutherland

Variance, Skewness & Kurtosis: results from the APM Cluster Redshift Survey and model predictions

(1995)

Authors:

Enrique Gazta帽aga, Rupert Croft, Gavin Dalton

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 86
  • Page 87
  • Page 88
  • Page 89
  • Current page 90
  • Page 91
  • Page 92
  • Page 93
  • Page 94
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

Department Of Physics text logo

漏 University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

  • Home
  • Research
  • 51猎奇入口
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • 51猎奇入口
  • Giving to Physics