The construction of a catalogue of galaxy groups from the Two-degree Field Galaxy Red-shift 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 s -1. This 2dFGRS Percolation-I...
The abundance of galaxy clusters as a function of mass is determined using the 2dFGRS Percolation-In...
Context. Groups form the most abundant class of galaxy systems. They act as the principal drivers of...
Context. Friends-of-friends algorithms are a common tool to detect galaxy groups and clusters in lar...
The construction of a catalogue of galaxy groups from the Two-degree Field Galaxy Red-shift Survey (...
The construction of a catalogue of galaxy groups from the Two-degree Field Galaxy Redshift Survey (2...
The Two-degree Field Galaxy Redshift Survey (2dFGRS) Percolation-Inferred Galaxy Group (2PIGG) catal...
We measure the clustering of galaxy groups in the 2dFGRS Percolation-Inferred Galaxy Group (2PIGG) c...
We construct a galaxy groups catalogue from the public 100K data release of the 2dF galaxy redshift ...
[[abstract]]A new algorithm is developed, based on the friends-of-friends (FOF) algorithm, to identi...
A galaxy group catalog is constructed from the 2MASS Redshift Survey (2MRS) with the use of a halo-b...
We present a structure-finding algorithm designed to identify galaxy groups in photometric-redshift ...
Context. Galaxy groups provide the means for a great diversity of studies that contribute to a bette...
8 pages, 5 figures, accepted in A&A, shortened abstractWe present an automated method to detect popu...
We use the first 25% of the DEEP2 Galaxy Redshift Survey spectroscopic data to identify groups and c...
We present a catalogue of galaxy groups and clusters selected using a friends-of-friends algorithm w...
The abundance of galaxy clusters as a function of mass is determined using the 2dFGRS Percolation-In...
Context. Groups form the most abundant class of galaxy systems. They act as the principal drivers of...
Context. Friends-of-friends algorithms are a common tool to detect galaxy groups and clusters in lar...
The construction of a catalogue of galaxy groups from the Two-degree Field Galaxy Red-shift Survey (...
The construction of a catalogue of galaxy groups from the Two-degree Field Galaxy Redshift Survey (2...
The Two-degree Field Galaxy Redshift Survey (2dFGRS) Percolation-Inferred Galaxy Group (2PIGG) catal...
We measure the clustering of galaxy groups in the 2dFGRS Percolation-Inferred Galaxy Group (2PIGG) c...
We construct a galaxy groups catalogue from the public 100K data release of the 2dF galaxy redshift ...
[[abstract]]A new algorithm is developed, based on the friends-of-friends (FOF) algorithm, to identi...
A galaxy group catalog is constructed from the 2MASS Redshift Survey (2MRS) with the use of a halo-b...
We present a structure-finding algorithm designed to identify galaxy groups in photometric-redshift ...
Context. Galaxy groups provide the means for a great diversity of studies that contribute to a bette...
8 pages, 5 figures, accepted in A&A, shortened abstractWe present an automated method to detect popu...
We use the first 25% of the DEEP2 Galaxy Redshift Survey spectroscopic data to identify groups and c...
We present a catalogue of galaxy groups and clusters selected using a friends-of-friends algorithm w...
The abundance of galaxy clusters as a function of mass is determined using the 2dFGRS Percolation-In...
Context. Groups form the most abundant class of galaxy systems. They act as the principal drivers of...
Context. Friends-of-friends algorithms are a common tool to detect galaxy groups and clusters in lar...