Discriminating Topology in Galaxy Distributions using Network Analysis
arXiv:1603.02285 · doi:10.1093/mnras/stw803
Abstract
(abridged) The large-scale distribution of galaxies is generally analyzed using the two-point correlation function. However, this statistic does not capture the topology of the distribution, and it is necessary to resort to higher order correlations to break degeneracies. We demonstrate that an alternate approach using network analysis can discriminate between topologically different distributions that have similar two-point correlations. We investigate two galaxy point distributions, one produced by a cosmological simulation and the other by a Lévy walk. For the cosmological simulation, we adopt the redshift slice from Illustris (Vogelsberger et al. 2014A) and select galaxies with stellar masses greater than . The two point correlation function of these simulated galaxies follows a single power-law, . Then, we generate Lévy walks matching the correlation function and abundance with the simulated galaxies. We find that, while the two simulated galaxy point distributions have the same abundance and two point correlation function, their spatial distributions are very different; most prominently, \emph{filamentary structures}, absent in Lévy fractals. To quantify these missing topologies, we adopt network analysis tools and measure diameter, giant component, and transitivity from networks built by a conventional friends-of-friends recipe with various linking lengths. Unlike the abundance and two point correlation function, these network quantities reveal a clear separation between the two simulated distributions; therefore, the galaxy distribution simulated by Illustris is not a Lévy fractal quantitatively. We find that the described network quantities offer an efficient tool for discriminating topologies and for comparing observed and theoretical distributions.
11 pages, 5 figures, submitted to MNRAS on 12/15/2015, now fully reviewed for publication; more information about our network analyses can be found at https://sites.google.com/site/shongscience/research
References in corpus (43)
- Statistical mechanics of complex networks
- The structure and function of complex networks
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
- Energy input from quasars regulates the growth and activity of black holes and their host galaxies
- Spatial Networks
- E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
- Cosmological SPH simulations: A hybrid multi-phase model for star formation
- Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
- Critical phenomena in complex networks
- Modeling feedback from stars and black holes in galaxy mergers
- Properties of galaxies reproduced by a hydrodynamic simulation
- Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
- A model for cosmological simulations of galaxy formation physics
- The Halo Occupation Distribution: Towards an Empirical Determination of the Relation Between Galaxies and Mass
- Theoretical Models of the Halo Occupation Distribution: Separating Central and Satellite Galaxies
- Baryon Acoustic Oscillations in the Lyα forest of BOSS DR11 quasars
- A unified model for AGN feedback in cosmological simulations of structure formation
- The Illustris Simulation: Public Data Release
- The DESI Experiment, a whitepaper for Snowmass 2013
- Moving mesh cosmology: tracing cosmological gas accretion
- The Spatial Clustering of Star-forming Galaxies at Redshifts 1.4<z<3.5
- The Multiscale Morphology Filter: Identifying and Extracting Spatial Patterns in the Galaxy Distribution
- NEXUS: Tracing the Cosmic Web Connection
- The power spectrum and bispectrum of SDSS DR11 BOSS galaxies I: bias and gravity
- Moving mesh cosmology: numerical techniques and global statistics
- Testing for Non-Gaussianity in the Wilkinson Microwave Anisotropy Probe Data: Minkowski Functionals and the Length of the Skeleton
- The overdensity and masses of the friends-of-friends halos and universality of the halo mass function
- Moving mesh cosmology: the hydrodynamics of galaxy formation
- A Measurement of Small Scale Structure in the 2.2 < z < 4.2 Lyman-alpha Forest
- Moving mesh cosmology: characteristics of galaxies and haloes
- Topology Analysis of the Sloan Digital Sky Survey: I. Scale and Luminosity Dependences
- Crawling the Cosmic Network: Identifying and Quantifying Filamentary Structure
- Limits on Primordial Non-Gaussianity from Minkowski Functionals of the WMAP Temperature Anisotropies
- Redshift-Space Distortions with the Halo Occupation Distribution II: Analytic Model
- Numerical Convergence in Smoothed Particle Hydrodynamics
- The extended Baryon Oscillation Spectroscopic Survey (eBOSS): a cosmological forecast
- The Three-Point Correlation Function of Luminous Red Galaxies in the Sloan Digital Sky Survey
- Measuring the Geometry and Topology of Large Scale Structure using SURFGEN: Methodology and Preliminary Results
- Non Gaussianity and Minkowski Functionals: forecasts for Planck
- Quantifying Cosmic Superstructures
- Degree-Scale CMB Polarization Measurements from Three Years of BICEP1 Data
- Morphology of the galaxy distribution from wavelet denoising
- Network Analysis of Cosmic Structures : Network Centrality and Topological Environment
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