The construction of a catalogue of galaxy groups from the Two-degree Field Galaxy Redshift Survey (2dFGRS) is described. Groups are identified by means of a friends-of-friends percolation algorithm which has been thoroughly tested on mock versions of the 2dFGRS generated from cosmological N-body simulations. The tests suggest that the algorithm groups all galaxies that it should be grouping, with an additional 40 per cent of interlopers. About 55 per cent of the 190 000 galaxies considered are placed into groups containing at least two members of which 29 000 are found. Of these, 7000 contain at least four galaxies, and these groups have a median redshift of 0.11 and a median velocity dispersion of 260 km s1. This 2dFGRS Percolation-Inferre...
A ``friends-of-friends'' percolation algorithm has been used to extract a catalogue of dn/n = 80 den...
We analyse the observed correlation between galaxy environment and Hα emission-line strength, using ...
We investigate the dependence of galaxy clustering on luminosity and spectral type using the 2dF Gal...
The construction of a catalogue of galaxy groups from the Two-degree Field Galaxy Redshift Survey (2...
The construction of a catalogue of galaxy groups from the Two-degree Field Galaxy Red-shift Survey (...
We measure the clustering of galaxy groups in the 2dFGRS Percolation-Inferred Galaxy Group (2PIGG) c...
The Two-degree Field Galaxy Redshift Survey (2dFGRS) Percolation-Inferred Galaxy Group (2PIGG) catal...
We construct a galaxy groups catalogue from the public 100K data release of the 2dF galaxy redshift ...
The Two-degree Field Galaxy Redshift Survey (2dFGRS) Percolation-Inferred Galaxy Group (2PIGG) catal...
We investigate the dependence of the strength of galaxy clustering on intrinsic luminosity using the...
In this Thesis we analyse in detail the Anglo-Australian 2 degree Field Galaxy Redshift Survey (2dFG...
[[abstract]]A new algorithm is developed, based on the friends-of-friends (FOF) algorithm, to identi...
The 2dF Galaxy Redshift Survey (2dFGRS) is designed to measure redshifts for approximately 250000 ga...
We present a power-spectrum analysis of the final 2dF Galaxy Redshift Survey (2dFGRS), employing a d...
We apply a friends-of-friends algorithm to the combined UZC and SSRS2 redshift surveys to construct ...
A ``friends-of-friends'' percolation algorithm has been used to extract a catalogue of dn/n = 80 den...
We analyse the observed correlation between galaxy environment and Hα emission-line strength, using ...
We investigate the dependence of galaxy clustering on luminosity and spectral type using the 2dF Gal...
The construction of a catalogue of galaxy groups from the Two-degree Field Galaxy Redshift Survey (2...
The construction of a catalogue of galaxy groups from the Two-degree Field Galaxy Red-shift Survey (...
We measure the clustering of galaxy groups in the 2dFGRS Percolation-Inferred Galaxy Group (2PIGG) c...
The Two-degree Field Galaxy Redshift Survey (2dFGRS) Percolation-Inferred Galaxy Group (2PIGG) catal...
We construct a galaxy groups catalogue from the public 100K data release of the 2dF galaxy redshift ...
The Two-degree Field Galaxy Redshift Survey (2dFGRS) Percolation-Inferred Galaxy Group (2PIGG) catal...
We investigate the dependence of the strength of galaxy clustering on intrinsic luminosity using the...
In this Thesis we analyse in detail the Anglo-Australian 2 degree Field Galaxy Redshift Survey (2dFG...
[[abstract]]A new algorithm is developed, based on the friends-of-friends (FOF) algorithm, to identi...
The 2dF Galaxy Redshift Survey (2dFGRS) is designed to measure redshifts for approximately 250000 ga...
We present a power-spectrum analysis of the final 2dF Galaxy Redshift Survey (2dFGRS), employing a d...
We apply a friends-of-friends algorithm to the combined UZC and SSRS2 redshift surveys to construct ...
A ``friends-of-friends'' percolation algorithm has been used to extract a catalogue of dn/n = 80 den...
We analyse the observed correlation between galaxy environment and Hα emission-line strength, using ...
We investigate the dependence of galaxy clustering on luminosity and spectral type using the 2dF Gal...