pith:KVYG6DU5
SE3D: Building a radiative transfer emulator to fit panchromatic resolved galaxy observations with 3D models of dust and stars
A Bayesian neural network emulator reproduces 3D radiative transfer outputs for galaxies to 0.05 dex accuracy.
arxiv:2511.19623 v2 · 2025-11-24 · astro-ph.GA · astro-ph.IM
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Claims
The computationally efficient machine learning emulator uses a Bayesian neural network architecture, and reproduces the spectral distributions at an accuracy of ~ 0.05 dex or less across the dynamic range of input parameters, and across the rest-frame UVJ colour space spanned by observed galaxies.
The library of toy models with chosen stellar and dust geometries plus radial population gradients is representative enough of real galaxies that the emulator can be used to fit actual panchromatic resolved observations.
SE3D builds a Bayesian neural network emulator that reproduces galaxy spectral distributions and structural parameters from 3D dust radiative transfer models at ~0.05 dex accuracy across UVJ colors and input ranges.
Receipt and verification
| First computed | 2026-05-20T00:05:37.942776Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
55706f0e9d5cd0143aa213a902a50ebb6247df97aa7ac71db29537b1ad565b6f
Aliases
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Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/KVYG6DU5LTIBIOVCCOUQFJIOXN \
| jq -c '.canonical_record' \
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Canonical record JSON
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