切伦科夫望远镜阵列 (CTA) 反射镜生产技术的现状
天体物理仪器与方法
2013-10-08 v1
摘要
切伦科夫望远镜阵列 (CTA) 是下一代甚高能伽马射线天文台，其灵敏度至少比现有仪器高 10 倍。CTA 将由数十台以阵列模式运行的成像大气切伦科夫望远镜 (IACTs) 组成，并分为三类尺寸：大型、中型和小型望远镜。总反射面积可能高达 10,000 平方米，需要前所未有的技术努力。反射镜的特性直接影响望远镜的性能，因此是提高和维持灵敏度的基本要素。本文回顾了针对不同类别望远镜的 CTA 望远镜反射镜用轻质、可靠且具成本效益的镜面单元的研发现状。
引用
@article{arxiv.1310.1713,
title = {Status of the technologies for the production of the Cherenkov Telescope Array (CTA) mirrors},
author = {G. Pareschi and T. Armstrong and H. Baba and J. Bähr and A. Bonardi and G. Bonnoli and P. Brun and R. Canestrari and P. Chadwick and M. Chikawa and P. -H. Carton and V. de Souza and J. Dipold and M. Doro and D. Durand and M. Dyrda and A. Förster and M. Garczarczyk and E. Giro and J. -F. Glicenstein and Y. Hanabata and M. Hayashida and M. Hrabovski and C. Jeanney and M. Kagaya and H. Katagiri and L. Lessio and D. Mandat and M. Mariotti and C. Medina and J. Michałowski and P. Micolon and D. Nakajima and J. Niemiec and A. Nozato and M. Palatka and M. Pech and B. Peyaud and G. Pühlhofer and M. Rataj and G. Rodeghiero and G. Rojas and J. Rousselle and R. Sakonaka and P. Schovanek and K. Seweryn and C. Schultz and S. Shu and F. Stinzing and M. Stodulski and M. Teshima and P. Travniczek and C. van Eldik and V. Vassiliev and Ł. Wiśniewski and A. Wörnlein and T. Yoshida},
journal= {arXiv preprint arXiv:1310.1713},
year = {2013}
}
备注
19 pages, SPIE Optics + Photonics 2013