Reducción de ruido por medio de autoencoders: caso de estudio con la señal GW150914
To address severe signal-to-noise ratio (SNR) degradation of low-amplitude astrophysical signals—such as gravitational waves—in the presence of strong, multi-source noise, this paper proposes an end-to-end nonlinear denoising method based on a deep autoencoder. The model jointly optimizes architecture and parameters using mixed data comprising real gravitational-wave events (e.g., GW150914) and synthetic noise, enabling adaptive extraction of weak signal features and effective noise suppression. Experiments demonstrate a substantial average SNR improvement of 38% over target signals, outperforming conventional filtering and shallow learning approaches. Crucially, this work provides the first systematic validation of autoencoders for denoising real astrophysical time-series data, establishing their effectiveness, robustness, and scalability. The method eliminates the need for prior noise modeling and is readily embeddable into real-time gravitational-wave analysis pipelines, offering a novel, data-driven paradigm for gravitational-wave detection.