Reconstruction of stereoscopic CTA events using deep learning with CTLearn

the CTA Consortium

研究成果: ジャーナルへの寄稿会議記事査読

2 被引用数 (Scopus)

抄録

The Cherenkov Telescope Array (CTA), conceived as an array of tens of imaging atmospheric Cherenkov telescopes (IACTs), is an international project for a next-generation ground-based gamma-ray observatory, aiming to improve on the sensitivity of current-generation instruments a factor of five to ten and provide energy coverage from 20 GeV to more than 300 TeV. Arrays of IACTs probe the very-high-energy gamma-ray sky. Their working principle consists of the simultaneous observation of air showers initiated by the interaction of very-high-energy gamma rays and cosmic rays with the atmosphere. Cherenkov photons induced by a given shower are focused onto the camera plane of the telescopes in the array, producing a multi-stereoscopic record of the event. This image contains the longitudinal development of the air shower, together with its spatial, temporal, and calorimetric information. The properties of the originating very-high-energy particle (type, energy, and incoming direction) can be inferred from those images by reconstructing the full event using machine learning techniques. In this contribution, we present a purely deep-learning driven, full-event reconstruction of simulated, stereoscopic IACT events using CTLearn. CTLearn is a package that includes modules for loading and manipulating IACT data and for running deep learning models, using pixel-wise camera data as input.

本文言語英語
論文番号730
ジャーナルProceedings of Science
395
出版ステータス出版済み - 2022/03/18
イベント37th International Cosmic Ray Conference, ICRC 2021 - Virtual, Berlin, ドイツ
継続期間: 2021/07/122021/07/23

ASJC Scopus 主題領域

  • 一般

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