HierArchical Wavelet Coefficients on the Sphere (HAWCS): the Scattering Transform on Spherical Maps

arXiv:2609.25548 · astro-ph.CO, astro-ph.IM · Submitted 2026-09-22 · Read on arXiv

astro-ph.CO, astro-ph.IM

Submitted: 2026-09-22

Updated: 2026-09-22

Code: https://github.com/ArefeAbghari/scattering-transform-spherical

License: http://creativecommons.org/licenses/by/4.0/

The gist: Extracting Gaussian information from data is well understood, but characterizing non-Gaussianity is challenging.

Terminology

Abstract

Extracting Gaussian information from data is well understood, but characterizing non-Gaussianity is challenging. We introduce HAWCS, a healpy-based Python package for efficiently computing wavelet scattering transform coefficients from full-sky maps. These coefficients provide compact summary statistics that are sensitive to higher-order structure and interactions across angular scales. We test the implementation on controlled Gaussian and non-Gaussian fields and demonstrate its computational efficiency. We then apply HAWCS to thermal Sunyaev-Zeldovich maps derived from Planck observations and four simulations, quantifying and comparing their higher-order statistical properties. We also use the method to expose the signatures of gravitational lensing in cosmic microwave background (CMB) temperature maps. These results demonstrate that HAWCS is a practical tool for validating component-separation pipelines and cosmological simulations, and a promising summary statistic for characterizing non-Gaussian structures beyond the power spectrum. These coefficients could also be used to constrain or generate simulated maps that reproduce the same statistical features of real data.

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