Reconstructing Atmospheric Parameters of Exoplanets Using Deep Learning
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Abstract (arXiv)
Exploring exoplanets has transformed our understanding of the universe by revealing many planetary systems that defy our current understanding. To study their atmospheres, spectroscopic observations are used to infer essential atmospheric properties that are not directly measurable. Estimating atmospheric parameters that best fit the observed spectrum within a specified atmospheric model is a complex problem that is difficult to model. In this paper, we present a multi-target probabilistic regression approach that combines deep learning and inverse modeling techniques within a multimodal architecture to extract atmospheric parameters from exoplanets. Our methodology overcomes computational limitations and outperforms previous approaches, enabling efficient analysis of exoplanetary atmospheres. This research contributes to advancements in the field of exoplanet research and offers valuable insights for future studies.
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References · 4
- 2017Advances in Variational Inferencecited by 236
- 2020Peeking inside the Black Box: Interpreting Deep Learning Models for Exoplanet Atmospheric Retrievalscited by 9
- 2022Convolutional neural networks as an alternative to Bayesian retrievalscited by 5
- 2020PyLightcurve-torch: a transit modelling package for deep learning applications in PyTorchcited by 2
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