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

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

2006-12-31

arxiv.org/abs/astro-ph/0701020v2

Appl.Opt.46:3444-3454,2007

Astronomy and Astrophysics

Astrophysics

23 pages. Accepted for publication in Applied Optics. Several minor clarifications added after peer review

Scientific paper

10.1364/AO.46.003444

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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