arXiv · 1911.09138
Large Scale Distribution of Galaxies in The Field HS 47.5-22. I. Data Analysis Technique
Abstract
We present the results of methodological works on automated analysis of the large scale distribution of galaxies. Selecting candidates for clusters and groups of galaxies was carried out using two complementary methods of determining the density contrast maps in the narrow layers of the three-dimensional large scale distribution of galaxies: the filtering algorithm with an adaptive core and the Voronoi tesselation. The developed algorithms were tested on 10 data sets of the MICE model catalog; additionally, we determined the statistical parameters of the obtained results (completeness, sample purity, etc.). The constructed density contrast maps were also used to determine voids.
Explore related subjects
Keep this discovery
Aleksandra Grokhovskaya, Sergei N. Dodonov. 2019-11-20. Large Scale Distribution of Galaxies in The Field HS 47.5-22. I. Data Analysis Technique. https://doi.org/10.1134/s1990341319040047
Cite the original work for its findings. Save a collection to share your selection of sources.