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Extracting Gamma-Ray Information from Images with Convolutional Neural Network Methods on Simulated Cherenkov Telescope Array Data

机译:卷积神经网络在模拟切伦科夫望远镜阵列数据上的图像提取伽马射线信息

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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.
机译:切伦科夫望远镜阵列(CTA)将成为世界领先的地面伽玛射线天文台,使我们能够研究宇宙中非常高的能量现象。 CTA将产生数量级为PB的巨大数据集,而面临的挑战是寻找比现有数据集更好的替代数据分析方法。像深度学习技术一样,机器学习算法在该方向上给出了令人鼓舞的结果。特别地,图像上的卷积神经网络方法已被证明在模式识别中有效,并产生可以实现令人满意的预测的数据表示。我们测试了卷积神经网络的使用,以从具有高拒绝因子的背景图像中区分出信号,并从伽马射线事件中提供重建参数。在图像的人工数据集上对网络进行训练和评估。结果表明,用模拟数据训练的神经网络可用于提取伽马射线信息。这样的网络将帮助我们充分利用未来几十年内产生的大量实际数据。

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