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cs.LG updates on arXiv.org

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Estimating Orbital Parameters of Direct Imaging Exoplanet...
[Submitted on 20 Oct 2025 (v1), last revised 25 Jun 2026 (this v · 2026-06-26 · via cs.LG updates on arXiv.org

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Abstract:In this work, we propose a flow-matching Markov chain Monte Carlo (FM-MCMC) algorithm for estimating the orbital parameters of exoplanetary systems, especially for those only one exoplanet is involved. Compared to traditional methods that rely on random sampling within the Bayesian framework, our approach first leverages flow matching posterior estimation (FMPE) to efficiently constrain the prior range of physical parameters, and then employs MCMC to accurately infer the posterior distribution. For example, in the orbital parameter inference of beta Pictoris b, our model achieved a substantial speed-up while maintaining comparable accuracy-running 77.8 times faster than Parallel Tempered MCMC (PTMCMC) and 365.4 times faster than nested sampling. Moreover, our FM-MCMC method also attained the highest average log-likelihood among all approaches, demonstrating its superior sampling efficiency and accuracy. This highlights the scalability and efficiency of our approach, making it well-suited for processing the massive datasets expected from future exoplanet surveys. Beyond astrophysics, our methodology establishes a versatile paradigm for synergizing deep generative models with traditional sampling, which can be adopted to tackle complex inference problems in other fields, such as cosmology, biomedical imaging, and particle physics.

Submission history

From: Bo Liang [view email]
[v1] Mon, 20 Oct 2025 11:46:55 UTC (1,533 KB)
[v2] Fri, 7 Nov 2025 13:42:16 UTC (1,520 KB)
[v3] Thu, 25 Jun 2026 04:00:58 UTC (1,089 KB)