pith. sign in

arxiv: 2605.27538 · v1 · pith:3XQQG72Onew · submitted 2026-05-26 · 🌌 astro-ph.IM · astro-ph.CO· astro-ph.GA

VROOM-SBI: A Fast Simulation-Based Bayesian Inference Methodology for QU-Fitting

classification 🌌 astro-ph.IM astro-ph.COastro-ph.GA
keywords inferencequ-fittingfaradaybayesiancomparableline-of-sightmodelssimulation-based
0
0 comments X
read the original abstract

Bayesian QU-fitting is among the most accurate approaches for line-of-sight Faraday inference, but its per-pixel computational cost has made survey-scale application infeasible. QU-fitting is an alternative to Faraday synthesis with comparable accuracy in recovering line-of-sight Faraday components, but it has historically been computationally prohibitive at survey scale. Fitting to the Stokes spectra in $Q$ and $U$ through Bayesian inference is effective but slow. We introduce \texttt{VROOM-SBI}, which uses simulation-based inference, particularly neural posterior estimation, to speed up inference. Our results are comparable to both Faraday synthesis and QU-fitting, and deliver a speedup of $\sim$$500$ over classical QU-fitting implementations. We provide an open code repository and tools along with trained models via HuggingFace for the four standard depolarization models in common use, trained on VLA L-band frequency coverage.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.