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.

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收藏

页码：3444 / 3454

页数：11

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