mlsanityData to 14 Oct 2026

Reproducing Bayesian Posterior Distributions for Exoplanet Atmospheric Parameter Retrievals with a Machine Learning Surrogate Model

arXiv 2310.10521 ↗First posted 16 Oct 2023astro-ph.EP astro-ph.IM cs.LGcited by 3

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Abstract (arXiv)

We describe a machine-learning-based surrogate model for reproducing the Bayesian posterior distributions for exoplanet atmospheric parameters derived from transmission spectra of transiting planets with typical retrieval software such as TauRex. The model is trained on ground truth distributions for seven parameters: the planet radius, the atmospheric temperature, and the mixing ratios for five common absorbers: H2O, CH4, NH3, CO and CO2. The model performance is enhanced by domain-inspired preprocessing of the features and the use of semi-supervised learning in order to leverage the large amount of unlabelled training data available. The model was among the winning solutions in the 2023 Ariel Machine Learning Data Challenge.

Key facts. Cited by 3 papers in the map (data through 14 Oct 2026). Builds on 5 of its 17 references that are in the map. First posted on arXiv 16 Oct 2023.

Builds on

5 of 17 references.

References · 5

  1. 2014Adam: A Method for Stochastic Optimizationcited by 37,240
  2. 2019PyTorch: An Imperative Style, High-Performance Deep Learning Librarycited by 20,305
  3. 2021Analytical Modelling of Exoplanet Transit Specroscopy with Dimensional Analysis and Symbolic Regressioncited by 18
  4. 2020Lessons Learned from the 1st ARIEL Machine Learning Challenge: Correcting Transiting Exoplanet Light Curves for Stellar Spotscited by 5
  5. 2022Unsupervised Machine Learning for Exploratory Data Analysis of Exoplanet Transmission Spectracited by 3

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Cited by year (2026 to 14 Oct)

Citing papers per year: 2023: 1; 2024: 0; 2025: 0; 2026: 2.

3 papers.