Filaments and Pancakes in the IRAS 1.2 Jy Redshift Catalogue
arXiv:astro-ph/9805265 · doi:10.1086/311689
Abstract
We explore shapes of clusters and superclusters in the IRAS 1.2 Jy redshift survey with three reconstructions spanning the range β= 0.1, 0.5, 1.0, where β= Ω^{0.6}/b, b is the bias factor and Ωthe present value of the dimensionless matter density. Comparing our results to Gaussian randomized reconstructions of the IRAS catalogue, we find structures having both planar and filamentary properties. For β= 0.5, 1.0 the largest structures in the survey have a distinct tendency to be filament-like} in general agreement with the results of N-body simulations.
arXiv commentLatex (7 pages with aas2pp4.sty)
References in corpus (9)
- How Filaments are Woven into the Cosmic Web
- The IRAS 1.2 Jy Survey: Redshift Data
- Approximation Methods for Non-linear Gravitational Clustering
- Shapefinders: A new shape diagnostic for large scale structure
- Wiener Reconstruction of Density, Velocity, and Potential Fields from All-Sky Galaxy Redshift Surveys
- On the Shape of the First Collapsed Objects
- Universality of the Network and Bubble Topology in Cosmological Gravitational Simulations
- Percolation Analysis of a Wiener Reconstruction of the IRAS 1.2 Jy Redshift Catalog
- Emergence of Filamentary Structure in Cosmological Gravitational Clustering
Cited by in corpus (17)
- Reconstruction of the early Universe as a convex optimization problem
- Crawling the Cosmic Network: Identifying and Quantifying Filamentary Structure
- The Topology of the Cosmic Web in Terms of Persistent Betti Numbers
- Topology and Geometry of Gaussian random fields I: on Betti Numbers, Euler characteristic and Minkowski functionals
- Evidence for Filamentarity in the Las Campanas Redshift Survey
- PSCz Superclusters: Detection, Shapes & Cosmological Implications
- The Size of the Longest Filaments in the Universe
- The Shape of Poor Groups of Galaxies
- Shape Statistics of Sloan Digital Survey superclusters
- Supercluster Properties as a Cosmological Probe
- Unexpected Topology of the Temperature Fluctuations in the Cosmic Microwave Background
- Morphological & Dynamical Properties of low redshift 2dFGRS Groups
- Extended percolation analysis of the cosmic web
- Topology and Geometry of the CfA2 Redshift Survey
- Topology of the Las Campanas Redshift Survey
- Anomalies in the topology of the temperature fluctuations in the cosmic microwave background: An analysis of the and data releases
- Homology reveals significant anisotropy in the cosmic microwave background