Please use this identifier to cite or link to this item: https://dspace.iiti.ac.in/handle/123456789/17840
Title: Exploring machine learning regression models for advancing foreground mitigation and global 21cm signal parameter extraction
Authors: Tripathi, Anshuman
Datta, Abhirup
Issue Date: 2026
Publisher: Springer
Citation: Tripathi, A., Datta, A., & Kaur, G. (2026). Exploring machine learning regression models for advancing foreground mitigation and global 21cm signal parameter extraction. Journal of Astrophysics and Astronomy, 47(1). https://doi.org/10.1007/s12036-025-10117-0
Abstract: Extracting parameters from the global 21cm signal is crucial for understanding the early Universe. However, detecting the 21cm signal is challenging due to the brighter foreground and associated observational difficulties. In this study, we evaluate the performance of various machine-learning regression models to improve parameter extraction and foreground removal. This evaluation is essential for selecting the most suitable machine learning regression model based on computational efficiency and predictive accuracy. We compare four models: random forest regressor (RFR), Gaussian process regressor (GPR), support vector regressor (SVR), and artificial neural networks (ANNs). The comparison is based on metrics, such as the root mean square error (RMSE) and R2 scores. We examine their effectiveness across different dataset sizes and conditions, including scenarios with foreground contamination. Our results indicate that ANN consistently outperforms the other models, achieving the lowest RMSE and the highest R2 scores across multiple cases. While GPR also performs well, it is computationally intensive, requiring significant RAM and longer execution times. SVR struggles with large datasets due to its high computational costs, and RFR demonstrates the weakest accuracy among the models tested. We also found that employing principal component analysis (PCA) as a preprocessing step significantly enhances model performance, especially in the presence of foregrounds. © Indian Academy of Sciences 2026.
URI: https://dx.doi.org/10.1007/s12036-025-10117-0
https://dspace.iiti.ac.in:8080/jspui/handle/123456789/17840
ISSN: 0250-6335
Type of Material: Journal Article
Appears in Collections:Department of Astronomy, Astrophysics and Space Engineering

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