Atacama Cosmology Telescope 与 Millimeter Bolometric Array 相机的光学设计
天体物理学
2008-11-26 v2
摘要
Atacama Cosmology Telescope 是一台设计用于在 145 GHz、215 GHz 和 280 GHz 三个频率上以弧分钟分辨率绘制宇宙微波背景辐射的 6 米望远镜。每个频率都将配备 32 乘 32 元素的焦平面 TES bolometer阵列。本文描述了望远镜及其冷却再成像光学的设计，这些光学针对具有这些灵敏探测器的毫米波观测进行了优化。
引用
@article{arxiv.astro-ph/0701020,
title = {Optical Design of the Atacama Cosmology Telescope and the Millimeter Bolometric Array Camera},
author = {J. W. Fowler and M. D. Niemack and S. R. Dicker and A. M. Aboobaker and P. A. R. Ade and E. S. Battistelli and M. J. Devlin and R. P. Fisher and M. Halpern and P. C. Hargrave and A. D. Hincks and M. Kaul and J. Klein and J. M. Lau and M. Limon and T. A. Marriage and P. D. Mauskopf and L. Page and S. T. Staggs and D. S. Swetz and E. R. Switzer and R. J. Thornton and C. E. Tucker},
journal= {arXiv preprint arXiv:astro-ph/0701020},
year = {2008}
}
备注
23 pages. Accepted for publication in Applied Optics. Several minor clarifications added after peer review