Eventdisplay reconstruction and analysis pipeline for ground-based imaging atmospheric Cherenkov Telescopes
Published September 19, 2024 | Version v5.13.3
Software Open

Eventdisplay: An Analysis and Reconstruction Package for Ground-based Gamma-ray Astronomy

Creators

  • 1. DESY
  • 2. Department of Physics and Astronomy and the Bartol Research Institute, University of Delaware, Newark, DE 19716, USA

Description

Eventdisplay is a reconstruction and analysis pipeline for data of Imaging Atmospheric Cherenkov Telescopes (IACT). It has been primarily developed for VERITAS and CTA analysis.

Code, analysis files and scripts can be find in the Eventdisplay GitHub Organisation. Docker images are available from the Eventdisplay container registry.

In case Eventdisplay is used in a research project, please cite the following publication:

Maier, G.; Holder, J., Eventdisplay: An Analysis and Reconstruction Package for Ground-based Gamma-ray Astronomy, 35th International Cosmic Ray Conference. 10-20 July, 2017. Bexco, Busan, Korea, Proceedings of Science, Vol. 301. Online at [https://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=301], id.747 arXiv:1708.04048

This release changes the NSB levels in the docker run scripts to half and full for the different moon illumination settings.

What's Changed

  • Apply new naming for half-mooon observations by @GernotMaier in https://github.com/Eventdisplay/Eventdisplay/pull/165

Full Changelog: https://github.com/Eventdisplay/Eventdisplay/compare/v5.13.2...v5.13.3

Notes

If you use this software, please cite it using these metadata.

Files

Eventdisplay/Eventdisplay-v5.13.3.zip

Files (1.5 MB)

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Additional details

Related works

Is supplement to
Software: https://github.com/Eventdisplay/Eventdisplay/tree/v5.13.3 (URL)