Status of the H.E.S.S. Experiment
Astrophysics
2019-08-14 v2
Abstract
The H.E.S.S. experiment (High Energy Stereoscopic System) is a new generation atmospheric Cherenkov detector measuring high-energy (>100 GeV) gamma radiation from the Universe. This paper briefly explains the imaging Cherenkov technique and describes the H.E.S.S. project and its current status.
Cite
@article{arxiv.astro-ph/0307287,
title = {Status of the H.E.S.S. Experiment},
author = {U. Schwanke},
journal= {arXiv preprint arXiv:astro-ph/0307287},
year = {2019}
}
Comments
3 pages, Latex, two eps figures, uses pic03.sty, to be published in the proceedings of the XXIII Physics in Collision conference (PIC03), PSN FRAP16