We present a modified version of the friends-of-friends (FOF) structure finding algorithm, designed specifically to locate groups or clusters of galaxies in photometric redshift datasets. The main objective of this paper is to show that this extended friends-of-friends (hereafter EXT-FOF) algorithm yields results almost identical to the original FOF, if applied to a spectroscopic redshift dataset, and a rather conservative catalogue of structures, in case of a dataset with simulated photometric redshifts. Therefore, we create group catalogues for the first Center for Astrophysics Redshift Survey (CFA1), as well as for the Las Campanas Redshift Survey (LCRS), both of which being spectroscopic surveys, using FOF-algorithms. We then apply our ...
Context. Galaxy groups provide the means for a great diversity of studies that contribute to a bette...
International audienceContext. The discovery of new galaxy clusters is important for two reasons. Fi...
Aims. We study galaxy clustering and explore the dependence of galaxy properties on the the environm...
We present a structure-finding algorithm designed to identify galaxy groups in photometric-redshift ...
[[abstract]]A new algorithm is developed, based on the friends-of-friends (FOF) algorithm, to identi...
Aims. We have performed a detailed analysis of the ability of the friends-of-friends algorithm to id...
Aims. We have performed a detailed analysis of the ability of the friends-of-friends algorithm to id...
Aims. We have performed a detailed analysis of the ability of the friends-of-friends algorithm to id...
We investigate the dependence of galaxy populations on environment. Our samples are selected from th...
Context. Counting clusters is one of the methods to constrain cosmological parameters, but has been ...
8 pages, 5 figures, accepted in A&A, shortened abstractWe present an automated method to detect popu...
Context. Cosmological parameters can be constrained by counting clusters of galaxies as a function o...
International audienceThe specific star formation rates of galaxies are influenced both by their mas...
We describe a new method (Poisson Probability Method, PPM) to search for high redshift galaxy cluste...
Context. Groups form the most abundant class of galaxy systems. They act as the principal drivers of...
Context. Galaxy groups provide the means for a great diversity of studies that contribute to a bette...
International audienceContext. The discovery of new galaxy clusters is important for two reasons. Fi...
Aims. We study galaxy clustering and explore the dependence of galaxy properties on the the environm...
We present a structure-finding algorithm designed to identify galaxy groups in photometric-redshift ...
[[abstract]]A new algorithm is developed, based on the friends-of-friends (FOF) algorithm, to identi...
Aims. We have performed a detailed analysis of the ability of the friends-of-friends algorithm to id...
Aims. We have performed a detailed analysis of the ability of the friends-of-friends algorithm to id...
Aims. We have performed a detailed analysis of the ability of the friends-of-friends algorithm to id...
We investigate the dependence of galaxy populations on environment. Our samples are selected from th...
Context. Counting clusters is one of the methods to constrain cosmological parameters, but has been ...
8 pages, 5 figures, accepted in A&A, shortened abstractWe present an automated method to detect popu...
Context. Cosmological parameters can be constrained by counting clusters of galaxies as a function o...
International audienceThe specific star formation rates of galaxies are influenced both by their mas...
We describe a new method (Poisson Probability Method, PPM) to search for high redshift galaxy cluste...
Context. Groups form the most abundant class of galaxy systems. They act as the principal drivers of...
Context. Galaxy groups provide the means for a great diversity of studies that contribute to a bette...
International audienceContext. The discovery of new galaxy clusters is important for two reasons. Fi...
Aims. We study galaxy clustering and explore the dependence of galaxy properties on the the environm...