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

Jan, 2007
22 pages
Published in:
  • Appl.Opt. 46 (2007) 3444-3454
e-Print:

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Abstract: (arXiv)
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.
Note:
  • 23 pages. Accepted for publication in Applied Optics. Several minor clarifications added after peer review
  • optics: geometrical
  • mirror: surface
  • design
  • cosmic background radiation
  • performance