Weak Lensing Skew-Spectrum
arXiv:2006.12832 · doi:10.1093/mnras/staa2769
Abstract
We introduce the skew-spectrum statistic for weak lensing convergence maps and test it against state-of-the-art high-resolution all-sky numerical simulations. We perform the analysis as a function of source redshift and smoothing angular scale for individual tomographic bins. We also analyse the cross-correlation between different tomographic bins. We compare the numerical results to fitting-functions used to model the bispectrum of the underlying density field as a function of redshift and scale. We derive a closed form expression for the skew-spectrum for gravity-induced secondary non-Gaussianity. We also compute the skew-spectrum for the projected inferred from Cosmic Microwave Background (CMB) studies. As opposed to the low redshift case we find the post-Born corrections to be important in the modelling of the skew-spectrum for such studies. We show how the presence of a mask and noise can be incorporated in the estimation of a skew-spectrum.
16 pages, 11 figures
References in corpus (9)
- Beyond the Cosmological Standard Model
- Massive neutrinos and cosmology
- Cosmology with Weak Lensing Surveys
- Full-sky Gravitational Lensing Simulation for Large-area Galaxy Surveys and Cosmic Microwave Background Experiments
- CMB Constraints on Primordial non-Gaussianity from the Bispectrum (f_{NL}) and Trispectrum (g_{NL} and τ_{NL}) and a New Consistency Test of Single-Field Inflation
- KiDS-450: Cosmological Constraints from Weak Lensing Peak Statistics-I: Inference from Analytical Prediction of High Signal-to-Noise Ratio Convergence Peaks
- Near optimal bispectrum estimators for large-scale structure
- Cosmology with Phase Statistics: Parameter Forecasts and Detectability of BAO
- Consistency Relations in Effective Field Theory
Cited by in corpus (8)
- Nuw CDM cosmology from the weak lensing convergence PDF
- Cosmological Information in Skew Spectra of Biased Tracers in Redshift Space
- The integrated angular bispectrum of weak lensing
- Skewing the CMBLSS: a Fast Method for Bispectrum Analysis
- Weak Lensing Trispectrum and Kurt-Spectra
- Position-Dependent Correlation Function of Weak Lensing Convergence
- A New Estimator for Phase Statistics
- On Weak Lensing Response Functions