1. Department of Physics, University of Hamburg, Luruper Chaussee 149, 22761 Hamburg, Germany;2. School of Chemistry & Physics, University of Adelaide, Adelaide 5005, SA, Australia
Abstract:
Night sky brightness is a major source of noise both for Cherenkov telescopes as well as for wide-angle Cherenkov detectors. Therefore, it is important to know the level of night sky brightness at potential sites for future experiments.