Automated Exoplanet Transit Detection from Stellar Light Curves

28 Apr 2026 (modified: 29 Apr 2026)THU 2026 Spring ANM SubmissionEveryoneRevisionsBibTeXCC BY 4.0
Keywords: Time Series Intelligence, Transit Photometry
Abstract: The discovery of exoplanets is a crucial frontier in modern astrophysics. It expands our understanding of planetary formation, contextualizes the uniqueness of our own solar system, and drives the search for potentially habitable worlds. Just as ancient explorers like Herodotus gathered knowledge about islands of habitability outside the known world, modern astronomers seek out habitable zones beyond our local cosmic neighborhood. Until recent years, the field relied heavily on classical approaches and manual interpretation of potential exoplanet candidates. These methods are labor-intensive, subject to human error, and often struggle to isolate weak signals hidden in noise. The recent introduction of Machine Learning has driven significant progress, leading to the automated discovery of many new potential exoplanets. In this course project, we aim to contribute to this intersection of Planetary Science and ML by bringing state-of-the-art Time-Series Intelligence techniques into the existing framework of exoplanet discovery. Specifically, we plan to focus on the automated search for smaller exoplanets with weak or non-periodic transit signals, which are currently difficult for existing architectures to recognize.
Submission Number: 8
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