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Proceedings Paper

Preliminary design of the wavefront front sensor for CCAT
Author(s): David Naylor; Brad Gom; Mélanie Leclerc; Mathieu Legros; Stephen Padin; Eugene Serabyn
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Paper Abstract

CCAT1 is a submillimeter telescope currently under development that will be located at an altitude of 5600 meters in the Andes mountains of northern Chile. The atmospheric transmission at this site will allow CCAT to achieve high sensitivity over a wide field of view and a broad wavelength range to provide an unprecedented capability for deep, large area multicolor submillimeter surveys. In order to achieve high aperture efficiencies out to frequencies of ~ 1 THz, the 162 individual panels that form the 25 meter aperture of CCAT must be aligned to a tolerance of a few microns rms. The design of a wavefront sensor to achieve this goal is presented.

Paper Details

Date Published: 23 July 2014
PDF: 7 pages
Proc. SPIE 9153, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII, 915326 (23 July 2014); doi: 10.1117/12.2055372
Show Author Affiliations
David Naylor, Univ. of Lethbridge (Canada)
Brad Gom, Blue Sky Spectroscopy Inc. (Canada)
Mélanie Leclerc, INO (Canada)
Mathieu Legros, INO (Canada)
Stephen Padin, California Institute of Technology (United States)
Eugene Serabyn, Jet Propulsion Lab. (United States)


Published in SPIE Proceedings Vol. 9153:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII
Wayne S. Holland; Jonas Zmuidzinas, Editor(s)

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