English

Reconstruction of stereoscopic CTA events using deep learning with CTLearn

Instrumentation and Methods for Astrophysics 2021-09-14 v1 High Energy Astrophysical Phenomena

Abstract

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.

Keywords

Cite

@article{arxiv.2109.05809,
  title  = {Reconstruction of stereoscopic CTA events using deep learning with CTLearn},
  author = {Tjark Miener and Daniel Nieto and Aryeh Brill and Samuel Spencer and Jose Luis Contreras},
  journal= {arXiv preprint arXiv:2109.05809},
  year   = {2021}
}

Comments

15 pages, 3 figures, Proceedings of the ICRC 2021 PoS(ICRC2021) 730

R2 v1 2026-06-24T05:54:31.545Z