Optical design of the atacama cosmology telescope and the millimeter bolometric array camera

被引：164
|
作者：
Fowler, J. W.
Niemack, M. D.
Dicker, S. R.
Aboobaker, A. M.
Ade, P. A. R.
Battistelli, E. S.
Devlin, M. J.
Fisher, R. P.
Halpern, M.
Hargrave, P. C.
Hincks, A. D.
Kaul, M.
Klein, J.
Lau, J. M.
Limon, M.
Marriage, T. A.
Mauskopf, P. D.
Page, L.
Staggs, S. T.
Swetz, D. S.
Switzer, E. R.
Thornton, R. J.
Tucker, C. E.
机构：
[1] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA
[2] Univ Penn, David Rittenhouse Lab, Dept Phys & Astron, Philadelphia, PA 19104 USA
[3] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, Wales
[4] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
来源：
APPLIED OPTICS | 2007年 / 46卷 / 17期
基金：
美国国家科学基金会;
关键词：
D O I：
10.1364/AO.46.003444
中图分类号：
O43 [光学];
学科分类号：
070207 ; 0803 ;
摘要：
The Atacama Cosmology Telescope is a 6 m telescope designed to map the cosmic microwave background simultaneously at 145, 215, and 280 GHz with arcminute resolution. Each frequency will have a 32 by 32 element focal plane array of transition edge sensor bolometers. The telescope and the cold reimaging optics are optimized for millimeter-wave observations with these sensitive detectors. The design of each is described. (C) 2007 Optical Society of America.
引用
收藏
页码：3444 / 3454
页数：11
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