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DeepTTV: Deep Learning Prediction of Hidden Exoplanet From Transit Timing Variations
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abstract
Transit timing variation (TTV) provides rich information about the mass and orbital properties of exoplanets, which are often obtained by solving an inverse problem via Markov Chain Monte Carlo (MCMC). In this paper, we design a new data-driven approach, which potentially can be applied to problems that are hard to traditional MCMC methods, such as the case with only one planet transiting. Specifically, we use a deep learning approach to predict the parameters of non-transit companion for the single transit system with transit information (i.e., TTV, and Transit Duration Variation (TDV)) as input. Thanks to a newly constructed \textit{Transformer}-based architecture that can extract long-range interactions from TTV sequential data, this previously difficult task can now be accomplished with high accuracy, with an overall fractional error of $\sim$2\% on mass and eccentricity.
Forward citations
Cited by 2 Pith papers
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Estimating Orbital Parameters of Direct Imaging Exoplanet Using Neural Network
Warm-starting parallel-tempered MCMC with flow-matching posterior proposals infers β Pictoris b's orbit about 78-365× faster than conventional samplers with comparable posteriors, though the comparison is not fully ap...
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Three-Dimensional Orbital Architectures and Detectability of Adjacent Companions to Hot Jupiters
Stellar spin-down can knock outer companions to hot Jupiters out of the transiting plane, biasing transit surveys against them, while inner companions remain detectable.
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