Gaussianizing the non-Gaussian lensing convergence field II: the applicability to noisy data
arXiv:1201.4527 · doi:10.1103/PhysRevD.86.023515
Abstract
In paper I (Yu et al. [1]), we show through N-body simulation that a local monotonic Gaussian transformation can significantly reduce non-Gaussianity in a noise-free lensing convergence field. This makes the Gaussianization a promising theoretical tool to understand high-order lensing statistics. Here we present a study of its applicability in lensing data analysis, in particular when shape measurement noise is presented in lensing convergence maps. (i) We find that shape measurement noise significantly degrades the Gaussianization performance and the degradation increases for shallower surveys. (ii) The Wiener filter is efficient in reducing the impact of shape measurement noise. The Gaussianization of the Wiener-filtered lensing maps is able to suppress skewness, kurtosis, and the 5th- and 6th-order cumulants by a factor of 10 or more. It also works efficiently to reduce the bispectrum to zero.
13 pages, 10 figures. Match the published version. Accepted by PRD
References in corpus (6)
- Rejuvenating Power Spectra II: the Gaussianized galaxy density field
- On the inadequacy of N-point correlation functions to describe nonlinear cosmological fields: explicit examples and connection to simulations
- Re-capturing cosmic information
- Information escaping the correlation hierarchy of the convergence field in the study of cosmological parameters
- Gaussianizing the non-Gaussian lensing convergence field I: the performance of the Gaussianization
- Dark Energy from the log-transformed convergence field
Cited by in corpus (9)
- Cosmology with cosmic shear observations: a review
- CMB Lensing Beyond the Power Spectrum: Cosmological Constraints from the One-Point PDF and Peak Counts
- Linearisation with Cosmological Perturbation Theory
- One-point remapping of Lagrangian perturbation theory in the mildly non-linear regime of cosmic structure formation
- Tomography and Weak lensing Statistics
- Fast generation of weak lensing maps by the inverse-Gaussianization method
- One-point statistics of the Lagrangian displacement field
- The copula of the cosmological matter density field is non-Gaussian
- Numerical investigation of non-Gaussianities in the phase and modulus of density Fourier modes