中文

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

天体物理仪器与方法 2026-05-28 v1 宇宙学与河外天体物理 星系天体物理

摘要

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 QQ and UU 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 \sim500500 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.

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引用

@article{arxiv.2605.27538,
  title  = {VROOM-SBI: A Fast Simulation-Based Bayesian Inference Methodology for QU-Fitting},
  author = {Arpan Pal and Preshanth Jagannathan},
  journal= {arXiv preprint arXiv:2605.27538},
  year   = {2026}
}

备注

Submitted in AJ; Comments are welcome. 10 figures, 2 tables