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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 Power Spectrum of Rich Clusters of Galaxies on Large Spatial Scales

(1997)

Authors:

Helen Tadros, George Efstathiou, Gavin Dalton
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The Origin of the Cosmic Soft X-Ray Background: Optical Identification of an Extremely Deep ROSAT Survey

(1997)

Authors:

IM McHardy, LR Jones, MR Merrifield, KO Mason, RG Abraham, AM Newsam, GB Dalton, F Carrera, PJ Smith, M Rowan-Robinson, GA Wegner, TJ Ponman, HJ Lehto, G Branduardi-Raymont, GA Luppino, G Efstathiou, DJ Allan, JJ Quenby
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The APM Galaxy Survey:- V. Catalogues of Galaxy Clusters

(1997)

Authors:

Gavin Dalton, Steve Maddox, Will Sutherland, George Efstathiou
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The richness dependence of galaxy cluster correlations: Results from a redshift survey of rich APM clusters

(1997)

Authors:

Rupert AC Croft, Gavin B Dalton, George Efstathiou, Will Sutherland, Steve Maddox
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The APM galaxy survey - V. Catalogues of galaxy clusters

Monthly Notices of the Royal Astronomical Society 289:2 (1997) 263-284

Authors:

GB Dalton, SJ Maddox, WJ Sutherland, G Efstathiou

Abstract:

We describe the construction of catalogues of galaxy clusters from the APM Galaxy survey using an automated algorithm based on Abell-like selection criteria. We investigate the effects of varying several parameters in our selection algorithm, including the magnitude range and radius from the cluster centre used to estimate the cluster richnesses. We quantify the accuracy of the photometric distance estimates by comparing them with measured redshifts, and we investigate the stability and completeness of the resulting catalogues. We find that the angular correlation functions for different cluster catalogues are in good agreement with one another, and are also consistent with the observed amplitude of the spatial correlation function of rich clusters. © 1997 RAS.
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