Flow Matching for Atmospheric Retrieval of Exoplanets: Where Reliability meets Adaptive Noise Levels
Timothy D. Gebhard, Jonas Wildberger, Maximilian Dax and, Annalena Kofler, Daniel Angerhausen, Sascha P. Quanz, Bernhard, Sch\"olkopf

TL;DR
This paper introduces flow matching posterior estimation (FMPE) for atmospheric retrieval of exoplanets, enhancing reliability, flexibility, and speed over traditional methods, with noise level conditioning and importance sampling for verification.
Contribution
The paper proposes FMPE as a new, scalable ML approach for atmospheric retrieval, incorporating noise conditioning and importance sampling for verification and model comparison.
Findings
FMPE trains three times faster than NPE.
Both FMPE and NPE perform comparably to nested sampling across noise levels.
Importance sampling effectively verifies results and estimates Bayesian evidence.
Abstract
Inferring atmospheric properties of exoplanets from observed spectra is key to understanding their formation, evolution, and habitability. Since traditional Bayesian approaches to atmospheric retrieval (e.g., nested sampling) are computationally expensive, a growing number of machine learning (ML) methods such as neural posterior estimation (NPE) have been proposed. We seek to make ML-based atmospheric retrieval (1) more reliable and accurate with verified results, and (2) more flexible with respect to the underlying neural networks and the choice of the assumed noise models. First, we adopt flow matching posterior estimation (FMPE) as a new ML approach to atmospheric retrieval. FMPE maintains many advantages of NPE, but provides greater architectural flexibility and scalability. Second, we use importance sampling (IS) to verify and correct ML results, and to compute an estimate of the…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Inertial Sensor and Navigation
