Prototype Tests for the CELESTE Solar Array Gamma--Ray Telescope
天体物理学
2009-10-30 v1
摘要
The CELESTE experiment will be an Atmospheric Cherenkov detector designed to bridge the gap in energy sensitivity between current satellite and ground-based gamma-ray telescopes, 20 to 300 GeV. We present test results made at the former solar power plant, Themis, in the French Pyrenees. The tests confirm the viability of using a central tower heliostat array for Cherenkov wavefront sampling.
关键词
引用
@article{arxiv.astro-ph/9803198,
title = {Prototype Tests for the CELESTE Solar Array Gamma--Ray Telescope},
author = {B. Giebels and R. Bazer-Bachi and H. Bergeret and A. Cordier and G. Debiais and M. De Naurois and J. P. Dezalay and D. Dumora and P. Eschstruth and P. Espigat and B. Fabre and P. Fleury and C. Ghesquière and N. Herault and I. Malet and B. Merkel and C. Meynadier and M. Palatka and E. Paré and J. Procureur and M. Punch and J. Québert and K. Ragan and L. Rob and P. Schovanek and D. A. Smith and J. Vrana},
journal= {arXiv preprint arXiv:astro-ph/9803198},
year = {2009}
}
备注
LaTeX2e,30 pages including 14 figures, accepted for publication by Nuclear Instruments & Methods Section A