Calibration of the CAT Telescope
天体物理学
2019-08-14 v1
摘要
Due to the lack of test-beams in ground-based gamma-ray astronomy, detector calibration has been a major challenge in this field. However, with the use of Cherenkov ring-images due to cosmic-ray muons and of strong gamma-ray signals, the CAT telescope could be rather well monitored and understood. Here we present a few oustanding aspects of this work.
引用
@article{arxiv.astro-ph/9910518,
title = {Calibration of the CAT Telescope},
author = {Frederic Piron},
journal= {arXiv preprint arXiv:astro-ph/9910518},
year = {2019}
}
备注
5 pages, 5 figures. To appear in the proceedings of the GeV-TeV Gamma Ray Astrophysics Workshop "Towards a Major Atmospheric Cherenkov Detector VI", Snowbird, Utah, August 13-16, 1999