The distribution of galaxies and clusters of galaxies on the mega-parsec scale of the Universe follows an intricate pattern now famously known as the Large-Scale Structure or the Cosmic Web. To study the environments of this network, several techniques have been developed that are able to describe its properties and the properties of groups of galaxies as a function of their environment. In this work, we analyse the previously introduced framework: 1-Dimensional Recovery, Extraction, and Analysis of Manifolds (1-DREAM) on N-body cosmological simulation data of the Cosmic Web. The 1-DREAM toolbox consists of five Machine Learning methods, whose aim is the extraction and modelling of one-dimensional structures in astronomical big data setting...
The cosmic web is one of the most striking features of the distribution of galaxies and dark matter ...
This study is the first in a series in which we analyse the structure and topology of the Cosmic Web...
Next-generation wide-field spectroscopic surveys will observe the infall regions around large number...
The distribution of galaxies and clusters of galaxies on the mega-parsec scale of the Universe follo...
The distribution of galaxies and clusters of galaxies on the mega-parsec scale of the Universe follo...
The late-time matter distribution depicts a complex pattern commonly called the cosmic web. In this ...
Filamentary structures (one-dimensional manifolds) are ubiquitous in astronomical data sets. Be it i...
Recent application of the Bayesian algorithm \textsc{borg} to the Sloan Digital Sky Survey (SDSS) ma...
The cosmic web is one of the most striking features of the distribution of galaxies and dark matter ...
The cosmic web is the largest scale manifestation of the anisotropic gravitational collapse of matte...
Abstract: We discuss the intimate relationship between the filamentary features and the rare dense c...
The cosmic web is the largest scale manifestation of the anisotropic gravitational collapse of matte...
We present the SpineWeb framework for the topological analysis of the Cosmic Web and the identificat...
The cosmic web is one of the most striking features of the distribution of galaxies and dark matter ...
This study is the first in a series in which we analyse the structure and topology of the Cosmic Web...
Next-generation wide-field spectroscopic surveys will observe the infall regions around large number...
The distribution of galaxies and clusters of galaxies on the mega-parsec scale of the Universe follo...
The distribution of galaxies and clusters of galaxies on the mega-parsec scale of the Universe follo...
The late-time matter distribution depicts a complex pattern commonly called the cosmic web. In this ...
Filamentary structures (one-dimensional manifolds) are ubiquitous in astronomical data sets. Be it i...
Recent application of the Bayesian algorithm \textsc{borg} to the Sloan Digital Sky Survey (SDSS) ma...
The cosmic web is one of the most striking features of the distribution of galaxies and dark matter ...
The cosmic web is the largest scale manifestation of the anisotropic gravitational collapse of matte...
Abstract: We discuss the intimate relationship between the filamentary features and the rare dense c...
The cosmic web is the largest scale manifestation of the anisotropic gravitational collapse of matte...
We present the SpineWeb framework for the topological analysis of the Cosmic Web and the identificat...
The cosmic web is one of the most striking features of the distribution of galaxies and dark matter ...
This study is the first in a series in which we analyse the structure and topology of the Cosmic Web...
Next-generation wide-field spectroscopic surveys will observe the infall regions around large number...