# Improved simulation of non-Gaussian temperature and polarization CMB maps

## TL;DR

This paper presents an efficient algorithm for generating non-Gaussian CMB temperature and polarization maps with arbitrary local non-Gaussianity, improving accuracy, speed, and memory usage, and providing validated simulations to the community.

## Contribution

The authors introduce an optimized quadrature-based algorithm for simulating non-Gaussian CMB maps that enhances computational efficiency and accuracy over previous methods.

## Key findings

- Successfully generated 1000 non-Gaussian CMB maps up to l_max=1024.
- Validated the simulations using power spectrum and bispectrum estimators.
- Achieved significant reductions in memory consumption and computation time.

## Abstract

We describe an algorithm to generate temperature and polarization maps of the cosmic microwave background radiation containing non-Gaussianity of arbitrary local type. We apply an optimized quadrature scheme that allows us to predict and control integration accuracy, speed up the calculations, and reduce memory consumption by an order of magnitude. We generate 1000 non-Gaussian CMB temperature and polarization maps up to a multipole moment of l_max = 1024. We validate the method and code using the power spectrum and the fast cubic (bispectrum) estimator and find consistent results. The simulations are provided to the community.