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Computing Transiting Exoplanet Parameters with 1D Convolutional Neural Networks
Feb. 22, 2024, 5:42 a.m. | Santiago Iglesias \'Alvarez, Enrique D\'iez Alonso, Mar\'ia Luisa S\'anchez Rodr\'iguez, Javier Rodr\'iguez Rodr\'iguez, Sa\'ul P\'erez Fern\'andez, F
cs.LG updates on arXiv.org arxiv.org
Abstract: The transit method allows the detection and characterization of planetary systems by analyzing stellar light curves. Convolutional neural networks appear to offer a viable solution for automating these analyses. In this research, two 1D convolutional neural network models, which work with simulated light curves in which transit-like signals were injected, are presented. One model operates on complete light curves and estimates the orbital period, and the other one operates on phase-folded light curves and estimates …
abstract arxiv astro-ph.ep astro-ph.im computing convolutional neural network convolutional neural networks cs.lg detection exoplanet light network networks neural network neural networks parameters research solution systems transit type work
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