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Simulation-based Inference for Exoplanet Atmospheric Retrieval: Insights from winning the Ariel Data Challenge 2023 using Normalizing Flows

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arxiv 2309.09337 v1 pith:FPIF6T4T submitted 2023-09-17 astro-ph.EP astro-ph.IMcs.LG

classification astro-ph.EPastro-ph.IMcs.LG
keywords atmosphericchallengedataexoplanetmodelsspectraadvancementsanalysis
verification ladder T0 review T1 audit T2 compute T3 formal
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Advancements in space telescopes have opened new avenues for gathering vast amounts of data on exoplanet atmosphere spectra. However, accurately extracting chemical and physical properties from these spectra poses significant challenges due to the non-linear nature of the underlying physics. This paper presents novel machine learning models developed by the AstroAI team for the Ariel Data Challenge 2023, where one of the models secured the top position among 293 competitors. Leveraging Normalizing Flows, our models predict the posterior probability distribution of atmospheric parameters under different atmospheric assumptions. Moreover, we introduce an alternative model that exhibits higher performance potential than the winning model, despite scoring lower in the challenge. These findings highlight the need to reevaluate the evaluation metric and prompt further exploration of more efficient and accurate approaches for exoplanet atmosphere spectra analysis. Finally, we present recommendations to enhance the challenge and models, providing valuable insights for future applications on real observational data. These advancements pave the way for more effective and timely analysis of exoplanet atmospheric properties, advancing our understanding of these distant worlds.

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Cited by 3 Pith papers

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  1. Magnetic field strengths of hot giant exoplanets consistent with Solar System values

    astro-ph.EP 2026-06 unverdicted novelty 6.0 of 10

    Wind speed measurements in seven ultra-hot Jupiters decrease with temperature, consistent with magnetic drag and implying magnetic field strengths of a few gauss.

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    astro-ph.EP 2025-07 unverdicted novelty 6.0 of 10

    A 1D CNN trained on over a million synthetic Earth-analog spectra retrieves gas abundances and planet properties in seconds, with Monte Carlo Dropout uncertainties.

  3. Supervised Machine Learning Methods with Uncertainty Quantification for Exoplanet Atmospheric Retrievals from Transmission Spectroscopy

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    On a synthetic JWST/Ariel-style spectral database, XGBoost and SVM with per-spectrum normalization and log-abundance targets outperform random forests and other classical regressors for exoplanet atmospheric retrievals.

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