Revised LOFAR upper limits on the 21-cm signal power spectrum at $\mathbf{z\approx9.1}$ using Machine Learning and Gaussian Process Regression
Anshuman Acharya, Florent Mertens, Benedetta Ciardi, Raghunath Ghara,, L\'eon V. E. Koopmans, Saleem Zaroubi

TL;DR
This paper introduces a machine learning-enhanced Gaussian Process Regression method to improve foreground mitigation in LOFAR data, leading to revised upper limits on the high-redshift 21-cm signal power spectrum at z≈9.1.
Contribution
The study applies a novel VAE-based covariance kernel within GPR to reduce signal loss and systematically improve upper limit estimates for the 21-cm power spectrum.
Findings
Revised 2-sigma upper limit of Δ²₁₋₂ < (25)^2 mK² at k=0.075 h Mpc⁻¹.
VAE-based kernel shows smaller correlation with excess noise.
GPR approach effectively models LOFAR data for 21-cm signal constraints.
Abstract
The use of Gaussian Process Regression (GPR) for foregrounds mitigation in data collected by the LOw-Frequency ARray (LOFAR) to measure the high-redshift 21-cm signal power spectrum has been shown to have issues of signal loss when the 21-cm signal covariance is misestimated. To address this problem, we have recently introduced covariance kernels obtained by using a Machine Learning based Variational Auto-Encoder (VAE) algorithm in combination with simulations of the 21-cm signal. In this work, we apply this framework to 141 hours ( nights) of LOFAR data at , and report revised upper limits of the 21-cm signal power spectrum. Overall, we agree with past results reporting a 2- upper limit of at . Further, the VAE-based kernel has a smaller correlation with the systematic excess noise, and the…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Superconducting and THz Device Technology
