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

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dc.creatorFowler, J. W.
dc.creatorNiemack, M. D.
dc.creatorDicker, S. R.
dc.creatorAboobaker, A. M.
dc.creatorAde, P. A. R.
dc.creatorBattistelli, E. S.
dc.creatorDevlin, M. J.
dc.creatorFisher, R. P.
dc.creatorHalpern, M.
dc.creatorHargrave, P. C.
dc.creatorHincks, A. D.
dc.creatorKaul, M.
dc.creatorKlein, J.
dc.creatorLau, J. M.
dc.creatorLimon, M.
dc.creatorMarriage, T. A.
dc.creatorMauskopf, P. D.
dc.creatorPage, L.
dc.creatorStaggs, S. T.
dc.creatorSwetz, D. S.
dc.creatorSwitzer, E. R.
dc.creatorThornton, R. J.
dc.creatorTucker, C. E.
dc.date2006-12-31
dc.date2007-02-02
dc.date.accessioned2026-07-07T11:20:55Z
dc.date.available2026-07-07T11:20:55Z
dc.descriptionThe 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.
dc.description23 pages. Accepted for publication in Applied Optics. Several minor clarifications added after peer review
dc.identifierhttps://arxiv.org/abs/astro-ph/0701020
dc.identifierhttp://arxiv.org/abs/astro-ph/0701020
dc.identifierAppl.Opt.46:3444-3454,2007
dc.identifierdoi:10.1364/AO.46.003444
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194111
dc.subjectAstrophysics
dc.titleOptical Design of the Atacama Cosmology Telescope and the Millimeter Bolometric Array Camera
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