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The paper discusses the challenges of reconstructing the emission source location of ultra-high energy cosmic rays (UHECR) using radio-detection methods, highlighting issues related to the convergence of minimization algorithms and the ill-posed nature of the problem. It presents a simple method to improve the estimation of the source location while addressing the biases and degeneracies encountered in traditional approaches. The study emphasizes the importance of understanding the objective function used i

Author

rebii ahmed

Language

EN