Revealing Galactic dust beneath the cosmic infrared background anisotropies with Wavelet Phase Harmonics

arXiv:2608.25617 · astro-ph.GA, gr-qc · Submitted 2026-08-26 · Read on arXiv

astro-ph.GA, gr-qc

Submitted: 2026-08-26

Updated: 2026-08-26

Code: https://github.com/bregaldo/pywph

Terminology

Trace — 4× in this paper · explained in 2 episodes
Loss Function — 3× in this paper · explained in 2 episodes
Benchmark — 2× in this paper · explained in 2 episodes
Generative Model — 2× in this paper · explained in 2 episodes
Robustness — 2× in this paper · explained in 5 episodes
Anisotropy — 1× in this paper · explained in 3 episodes
Clustering — 1× in this paper · explained in 2 episodes
Consistency — 1× in this paper · explained in 3 episodes
Generative Models — 1× in this paper · explained in 2 episodes
Gravitational Lensing — 1× in this paper · explained in 2 episodes
Non-Gaussianity — 1× in this paper · explained in 2 episodes
Scattering Covariance — 1× in this paper
Scattering Transform — 1× in this paper
Wavelet Transform — 1× in this paper · explained in 2 episodes

Sources

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