CONICET | Buscador de Institutos y Recursos Humanos

Context. Galaxy groups provide the means for a great diversity of studies that contribute to a better understanding of the structure ofthe universe on a large scale and allow the properties of galaxies to be linked to those of the host halos. However, the identification ofgalaxy systems is a challenging task and therefore it is necessary to improve the techniques involved as much as possible.Aims. In view of the large present and forthcoming galaxy catalogues, we propose, implement, and evaluate an algorithm that combines the two most popular techniques used to identify galaxy systems. The algorithm can be easily applied to any spectroscopicgalaxy catalogue, but here we demonstrate its use on the Sloan Digital Sky Survey.Methods. Assuming that a galaxy group is a gravitationally bounded system that has at least one bright galaxy, we begin by identifying groups with a friends-of-friends algorithm adapted to fit this definition. In view of the shortcomings of this method, particularlythe lack of ability to identify low-number groups, and consequently the inability to study the occupation of halos throughout the massrange, we improve it by adding a halo-based procedure. To assess the performance, we construct a mock catalogue from a semianalytical model to compare the groups identified using our method with those obtained from the simulation.Results. The comparison of groups extracted using our method with those of a mock catalogue shows that the proposed algorithmprovides excellent results. The modifications introduced to the friends-of-friends algorithm in the first part of the procedure to fit theadopted group definition gave reliable groups. Furthermore, incorporation of the halo-based method reduces the interlopers whilemore accurately reproducing the number of galaxies per group. As a specific application, we use the algorithm to extract groups fromthe Sloan Digital Sky Survey