A statistical framework for quantitative spectroscopy of luminous blue stars
Miguel A. Urbaneja (Universit\"at Innsbruck, Institut f\"ur Astro- und Teilchenphysik)

TL;DR
This paper introduces MAUI, a Bayesian inference framework using Gaussian-process emulators to efficiently analyze stellar spectra, significantly reducing computational costs while maintaining accuracy for luminous blue stars.
Contribution
The paper presents a novel emulator-based Bayesian method for stellar spectroscopy that drastically improves efficiency without sacrificing model fidelity.
Findings
Emulators reproduce full atmosphere model predictions within uncertainties.
The approach reduces computational costs by orders of magnitude.
Posterior distributions are well calibrated and conservative.
Abstract
Context: Quantitative spectroscopy of luminous blue stars relies on detailed non-LTE model atmospheres whose increasing physical realism makes direct, iterative analyses computationally demanding. Aims: We introduce MAUI (Machine-learning Assisted Uncertainty Inference), a statistical framework designed for efficient Bayesian inference of stellar parameters using emulator-based spectral models. Methods: MAUI employs Gaussian-process-based emulators trained on a limited set of non-LTE simulations, combined with Markov Chain Monte Carlo (MCMC) sampling to explore posterior distributions. We validate the approach with recovery experiments and demonstrate it on Galactic late-type O dwarf and early-type B dwarf/subgiant stars. Results: The emulator reproduces the predictions of full atmosphere models within quoted uncertainties while reducing computational cost by orders of magnitude.…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Gamma-ray bursts and supernovae
