Fast Generation of Weak Lensing Maps with Analytical Point Transformation Functions
Kunhao Zhong, Gary Bernstein, Supranta S. Boruah, Bhuvnesh Jain, and, Sanjit Kobla

TL;DR
This paper introduces a new analytical point transform method that generates more accurate weak lensing maps than traditional lognormal models, enabling fast, high-fidelity simulations for cosmological research.
Contribution
The authors develop a General Point-Transformed Gaussian (GPTG) function that surpasses the lognormal transform in accuracy for weak lensing map generation, matching complex statistical properties with minimal computational cost.
Findings
GPTG maps match N-body simulation statistics within expected uncertainties.
The five-parameter GPTG outperforms lognormal by 2 to 5 times.
Method enables rapid, high-accuracy map generation for cosmological analysis.
Abstract
Nonlinear cosmological fields like galaxy density and lensing convergence can be approximately related to Gaussian fields via analytic point transforms. The lognormal transform (LN) has been widely used and is a simple example of a function that relates nonlinear fields to Gaussian fields. We consider more accurate General Point-Transformed Gaussian (GPTG) functions for such a mapping and apply them to convergence maps. We show that we can create maps that preserve the LN's ability to exactly match any desired power spectrum but go beyond LN by significantly improving the accuracy of the probability distribution function (PDF). With the aid of symbolic regression, we find a remarkably accurate GPTG function for convergence maps: its higher-order moments, scattering wavelet transform, Minkowski functionals, and peak counts match those of N-body simulations to the statistical uncertainty…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Orbital Angular Momentum in Optics · Antenna Design and Optimization
