Abstract

The Cherenkov Telescope Array (CTA) will be the world's leading ground-based gamma-ray observatory allowing us to study very high energy phenomena in the Universe. CTA will produce huge data sets, of the order of petabytes, and the challenge is to find better alternative data analysis methods to the already existing ones. Machine learning algorithms, like deep learning techniques, give encouraging results in this direction. In particular, convolutional neural network methods on images have proven to be effective in pattern recognition and produce data representations which can achieve satisfactory predictions. We test the use of convolutional neural networks to discriminate signal from background images with high rejections factors and to provide reconstruction parameters from gamma-ray events. The networks are trained and evaluated on artificial data sets of images. The results show that neural networks trained with simulated data can be useful to extract gamma-ray information. Such networks would help us to make the best use of large quantities of real data coming in the next decades.

Highlights

  • The ground-based observation of the very high energy gamma-ray sky (Egamma > 100 GeV ) has greatly progressed during the last 40 years through the use of imaging atmospheric Cherenkov telescopes (IACTs)

  • Convolutional neural network methods on images have proven to be effective in pattern recognition and produce data representations which can achieve satisfactory predictions

  • These telescopes aim to detect the air shower produced by the interaction of a primary cosmic gamma ray in the Earth’s atmosphere

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Summary

Introduction

The ground-based observation of the very high energy gamma-ray sky (Egamma > 100 GeV ) has greatly progressed during the last 40 years through the use of imaging atmospheric Cherenkov telescopes (IACTs) These telescopes aim to detect the air shower produced by the interaction of a primary cosmic gamma ray in the Earth’s atmosphere. The Southern Hemisphere observatory has a total of 99 telescopes of three different sizes with an area of 4.5 km and the Northern Hemisphere observatory has a total of 19 telescopes with an area of 0.6 km2 These telescopes will provide a large amount of images that encode primary particle information and it is essential to develop efficient statistical tools to best extract such information.

Monte Carlo Simulation and Preselection
Convolutional Neural Networks for Simulated Cherenkov Telescope Array Data
Findings
Summary and Conclusion
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