Application of deep learning methods to analysis of imaging atmospheric Cherenkov telescopes data

Ground based γ-ray observations with Imaging Atmospheric Cherenkov Telescopes (IACTs) play a significant role in the discovery of very high energy (E > 100 GeV) γ-ray emitters. The analysis of IACT data demands a highly efficient background rejection technique, as well as methods to accurately de...

Full description

Saved in:
Bibliographic Details
Published inAstroparticle physics Vol. 105; pp. 44 - 53
Main Authors Shilon, I., Kraus, M., Büchele, M., Egberts, K., Fischer, T., Holch, T.L., Lohse, T., Schwanke, U., Steppa, C., Funk, S.
Format Journal Article
LanguageEnglish
Published Elsevier B.V 01.02.2019
Subjects
Online AccessGet full text

Cover

Loading…
More Information
Summary:Ground based γ-ray observations with Imaging Atmospheric Cherenkov Telescopes (IACTs) play a significant role in the discovery of very high energy (E > 100 GeV) γ-ray emitters. The analysis of IACT data demands a highly efficient background rejection technique, as well as methods to accurately determine the position of its source in the sky and the energy of the recorded γ-ray. We present results for background rejection and signal direction reconstruction from first studies of a novel data analysis scheme for IACT measurements. The new analysis is based on a set of Convolutional Neural Networks (CNNs) applied to images from the four H.E.S.S. phase-I telescopes. As the H.E.S.S. cameras pixels are arranged in a hexagonal array, we demonstrate two ways to use such image data to train CNNs: by resampling the images to a square grid and by applying modified convolution kernels that conserve the hexagonal grid properties. The networks were trained on sets of Monte-Carlo simulated events and tested on both simulations and measured data from the H.E.S.S. array. A comparison between the CNN analysis to current state-of-the-art algorithms reveals a clear improvement in background rejection performance. When applied to H.E.S.S. observation data, the CNN direction reconstruction performs at a similar level as traditional methods. These results serve as a proof-of-concept for the application of CNNs to the analysis of events recorded by IACTs.
ISSN:0927-6505
1873-2852
DOI:10.1016/j.astropartphys.2018.10.003