A New Estimator for Phase Statistics
arXiv:2109.08047 · doi:10.1088/1475-7516/2022/05/006
Abstract
We introduce a novel statistic to probe the statistics of phases of Fourier modes in two-dimensions (2D) for weak lensing convergence field . This statistic contains completely independent information compared to that contained in observed power spectrum. We compare our results against state-of-the-art numerical simulations as a function of source redshift and find good agreement with theoretical predictions. We show that our estimator can achieve better signal-to-noise compared to the commonly employed statistics known as the line correlation function (LCF). Being a two-point statistics, our estimator is also easy to implement in the presence of complicated noise and mask, and can also be generalised to higher-order. While applying this estimator for the study of lensed CMB maps, we show that it is important to include post-Born corrections in the study of statistics of phase.
arXiv comment18 pages, 7 figures
References in corpus (54)
- HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
- SDSS-III: Massive Spectroscopic Surveys of the Distant Universe, the Milky Way Galaxy, and Extra-Solar Planetary Systems
- Large-Scale Structure of the Universe and Cosmological Perturbation Theory
- Beyond the Cosmological Standard Model
- Non-Gaussianity from Inflation: Theory and Observations
- An All-Sky Analysis of Polarization in the Microwave Background
- The Hyper Suprime-Cam SSP Survey: Overview and Survey Design
- The WiggleZ Dark Energy Survey: Survey Design and First Data Release
- Weak Lensing of the CMB: A Harmonic Approach
- Gravitational Lensing Analysis of the Kilo Degree Survey
- The Skewness of the Aperture Mass Statistic
- Cosmology with Weak Lensing Surveys
- Fast likelihood-free cosmology with neural density estimators and active learning
- Cosmology from Cosmic Shear with DES Science Verification Data
- Full-sky Gravitational Lensing Simulation for Large-area Galaxy Surveys and Cosmic Microwave Background Experiments
- Interferometric Observation of Cosmic Microwave Background Anisotropies
- Impact of post-Born lensing on the CMB
- An EFT description of galaxy intrinsic alignments
- LSST: a Complementary Probe of Dark Energy
- Fitting the nonlinear matter bispectrum by the Halofit approach
- Persistent homology in cosmic shear: constraining parameters with topological data analysis
- Impact of the non-Gaussian covariance of the weak lensing power spectrum and bispectrum on cosmological parameter estimation
- Response function of the large-scale structure of the universe to the small scale inhomogeneities
- Matter trispectrum: theoretical modelling and comparison to N-body simulations
- Cosmological constraints with weak lensing peak counts and second-order statistics in a large-field survey
- New Optimised Estimators for the Primordial Trispectrum
- Painting halos from cosmic density fields of dark matter with physically motivated neural networks
- Non-Gaussianity in Large Scale Structure and Minkowski Functionals
- A Robust Measure of Cosmic Structure beyond the Power-Spectrum: Cosmic Filaments and the Temperature of Dark Matter
- Universal Behavior of Phase Correlations in Non-linear Gravitational Clustering
- Weak lensing shear and aperture-mass from linear to non-linear scales
- Phase Correlations in Non-Gaussian Fields
- Exact Extreme Value Statistics and the Halo Mass Function
- Three-point phase correlations: A new measure of non-linear large-scale structure
- The Weak Lensing Bispectrum Induced By Gravity
- Cylinders out of a top hat: counts-in-cells for projected densities
- Studying the morphology of reionisation with the triangle correlation function of phases
- Statistics of Fourier Modes in Non-Gaussian Fields
- The Distribution Function of the Phase Sum as a Signature of Phase Correlations Induced by Nonlinear Gravitational Clustering
- Cosmology with Phase Statistics: Parameter Forecasts and Detectability of BAO
- Higher order statistics of shear field: a machine learning approach
- Cosmological parameters from weak lensing power spectrum and bispectrum tomography: including the non-Gaussian errors
- The position-dependent matter density probability distribution function
- The Integrated Bispectrum in Modified Gravity Theories
- An adapted filter function for density split statistics in weak lensing
- Consistency Relations in Effective Field Theory
- Estimating the Integrated Bispectrum from Weak Lensing Maps
- Weak Lensing Skew-Spectrum
- Morphology of Weak Lensing Convergence Maps
- Probing redshift-space distortions with phase correlations
- Cosmological Constraints from Fourier Phase Statistics
- Constraining the growth rate of structure with phase correlations
- The large-scale Gravitational Bias from the Quasilinear Regime
- Observing Baryonic Acoustic Oscillations in tomographic cosmic shear surveys