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Optical Design of the Atacama Cosmology Telescope and the Millimeter Bolometric Array Camera

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arxiv astro-ph/0701020 v2 pith:W3MBYBPI submitted 2006-12-31 astro-ph

J. W. Fowler , M. D. Niemack , S. R. Dicker , A. M. Aboobaker , P. A. R. Ade , E. S. Battistelli , M. J. Devlin , R. P. Fisher
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M. Halpern P. C. Hargrave A. D. Hincks M. Kaul J. Klein J. M. Lau M. Limon T. A. Marriage P. D. Mauskopf L. Page S. T. Staggs D. S. Swetz E. R. Switzer R. J. Thornton C. E. Tucker
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keywords telescopearrayatacamacosmologydesignarcminutebackgroundbolometers
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The Atacama Cosmology Telescope is a 6-meter telescope designed to map the Cosmic Microwave Background simultaneously at 145 GHz, 215 GHz, and 280 GHz with arcminute resolution. Each frequency will have a 32 by 32 element focal plane array of TES bolometers. This paper describes the design of the telescope and the cold reimaging optics, which is optimized for millimeter-wave observations with these sensitive detectors.

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