# Signal recognition and background suppression by matched filters and   neural networks for Tunka-Rex

**Authors:** D. Shipilov, P. A. Bezyazeekov, N. M. Budnev, D. Chernykh, O. Fedorov,, O. A. Gress, A. Haungs, R. Hiller, T. Huege, Y. Kazarina, M. Kleifges, E. E., Korosteleva, D. Kostunin, L. A. Kuzmichev, V. Lenok, N. Lubsandorzhiev, T., Marshalkina, R. Monkhoev, E. Osipova, A. Pakhorukov, L. Pankov, V. V. Prosin,, F. G. Schr\"oder, A. Zagorodnikov

arXiv: 1812.03347 · 2019-10-23

## TL;DR

This paper enhances cosmic-ray air-shower radio signal detection by combining matched filtering with neural network autoencoders to improve background suppression and lower detection thresholds.

## Contribution

It introduces a novel approach integrating matched filtering and neural network autoencoders for improved signal reconstruction in cosmic-ray radio detection.

## Key findings

- Matched filtering reduces detection threshold and increases purity.
- Autoencoders effectively denoise signals beyond traditional methods.
- Neural networks show promise for lowering detection thresholds.

## Abstract

The Tunka Radio Extension (Tunka-Rex) is a digital antenna array, which measures the radio emission of the cosmic-ray air-showers in the frequency band of 30-80 MHz. Tunka-Rex is co-located with TAIGA experiment in Siberia and consists of 63 antennas, 57 of them are in a densely instrumented area of about 1 km\textsuperscript{2}. In the present work we discuss the improvements of the signal reconstruction applied for the Tunka-Rex. At the first stage we implemented matched filtering using averaged signals as template. The simulation study has shown that matched filtering allows one to decrease the threshold of signal detection and increase its purity. However, the maximum performance of matched filtering is achievable only in case of white noise, while in reality the noise is not fully random due to different reasons. To recognize hidden features of the noise and treat them, we decided to use convolutional neural network with autoencoder architecture. Taking the recorded trace as an input, the autoencoder returns denoised trace, i.e. removes all signal-unrelated amplitudes. We present the comparison between standard method of signal reconstruction, matched filtering and autoencoder, and discuss the prospects of application of neural networks for lowering the threshold of digital antenna arrays for cosmic-ray detection.

## Full text

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## Figures

3 figures with captions in the complete paper: https://tomesphere.com/paper/1812.03347/full.md

## References

5 references — full list in the complete paper: https://tomesphere.com/paper/1812.03347/full.md

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Source: https://tomesphere.com/paper/1812.03347