The Topology of Weak Lensing Fields
arXiv:astro-ph/0009402 · doi:10.1086/320327
Abstract
The topology of weak lensing fields is studied using the 2-dimensional genus statistic. Simulated fields of the weak lensing convergence are used to focus on the effect of nonlinear gravitional evolution and to model the statistical errors expected in observational surveys. For large smoothing angles, the topology is in agreement with the predictions from linear theory. On smoothing angles smaller than 10', the genus curve shows the non-Gaussian signatures of gravitational clustering and differs for open and flat cold dark matter models. Forthcoming surveys with areas larger than 10 square degrees should have adequate signal-to-noise to measure the non-Gaussian shape and the -dependence of the genus statistic.
6 pages, 3 figures, to be published in ApJL (vol. 552)
References in corpus (4)
Cited by in corpus (26)
- The REFLEX Galaxy Cluster Survey VII: Omega_m and sigma_8 from cluster abundance and large-scale clustering
- Lognormal Property of Weak Lensing Fields
- From Weak Lensing to non-Gaussianity via Minkowski Functionals
- Statistical and Systematic Errors in Measurement of Weak-Lensing Minkowski Functionals: Application to Canada-France-Hawaii Lensing Survey
- The Kurtosis of the Cosmic Shear Field
- Going deep with Minkowski functionals of convergence maps
- Noise reduction for weak lensing mass mapping: An application of generative adversarial networks to Subaru Hyper Suprime-Cam first-year data
- Denoising Weak Lensing Mass Maps with Deep Learning
- Non-Gaussianity in Large Scale Structure and Minkowski Functionals
- Minkowski Functionals of Convergence Maps and the Lensing Figure of Merit
- PSF Anisotropy and Systematic Errors in Weak Lensing Surveys
- Probing Modified Gravity Theories with ISW and CMB Lensing
- New Approaches to Probing Minkowski Functionals
- Weakly non-Gaussian formula for the Minkowski functionals in general dimensions
- Higher order statistics of shear field: a machine learning approach
- Probing Primordial Non-Gaussianity with Weak Lensing Minkowski Functionals
- Cosmological Parameter Estimation Using the Genus Amplitude - Application to Mock Galaxy Catalogs
- Effect of Mask Regions on Weak Lensing Statistics
- Cosmological constraints using Minkowski functionals from the first year data of the Hyper Suprime-Cam
- Two-dimensional Topology of Cosmological Reionization
- Topology of Large-Scale Structures of Galaxies in Two Dimensions - Systematic Effects
- Morphology of Weak Lensing Convergence Maps
- Cosmological model differentiation through weak gravitational lensing
- The effect of primordial non-Gaussianity on the skeleton of cosmic shear maps
- The topology of weak lensing field in the neighborhood of MS1054-03
- On the effect of projections on convergence peak counts and Minkowski functionals