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Proceedings Paper

The South Pole Telescope
Author(s): John Ruhl; Peter A. R. Ade; John E. Carlstrom; Hsiao-Mei Cho; Thomas Crawford; Matt Dobbs; Chris H. Greer; Nils w. Halverson; William L. Holzapfel; Trevor M. Lanting; Adrian T. Lee; Erik M. Leitch; Jon Leong; Wenyang Lu; Martin Lueker; Jared Mehl; Stephan S. Meyer; Joe J. Mohr; Steve Padin; T. Plagge; Clem Pryke; Marcus C. Runyan; Dan Schwan; M. K. Sharp; Helmuth Spieler; Zak Staniszewski; Antony A. Stark
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Paper Abstract

A new 10 meter diameter telescope is being constructed for deployment at the NSF South Pole research station. The telescope is designed for conducting large-area millimeter and sub-millimeter wave surveys of faint, low contrast emission, as required to map primary and secondary anisotropies in the cosmic microwave background. To achieve the required sensitivity and resolution, the telescope design employs an off-axis primary with a 10 meter diameter clear aperture. The full aperture and the associated optics will have a combined surface accuracy of better than 20 microns rms to allow precision operation in the submillimeter atmospheric windows. The telescope will be surrounded with a large reflecting ground screen to reduce sensitivity to thermal emission from the ground and local interference. The optics of the telescope will support a degree field of view at 2mm wavelength and will feed a new 1000-element micro-lithographed planar bolometric array with superconducting transition-edge sensors and frequency-multiplexed readouts. The first key project will be to conduct a survey over &dbigwig;4000 degrees for galaxy clusters using the Sunyaev-Zel'dovich Effect. This survey should find many thousands of clusters with a mass selection criteria that is remarkably uniform with redshift. Armed with redshifts obtained from optical and infrared follow-up observations, it is expected that the survey will enable significant constraints to be placed on the equation of state of the dark energy.

Paper Details

Date Published: 8 October 2004
PDF: 19 pages
Proc. SPIE 5498, Millimeter and Submillimeter Detectors for Astronomy II, (8 October 2004); doi: 10.1117/12.552473
Show Author Affiliations
John Ruhl, Case Western Reserve Univ. (United States)
Peter A. R. Ade, Cardiff Univ. (United Kingdom)
John E. Carlstrom, Univ. of Chicago (United States)
Hsiao-Mei Cho, Univ. of California/Berkeley (United States)
Thomas Crawford, Univ. of Chicago (United States)
Matt Dobbs, Univ. of California/Berkeley (United States)
Chris H. Greer, Univ. of Chicago (United States)
Nils w. Halverson, Univ. of California/Berkeley (United States)
William L. Holzapfel, Univ. of California/Berkeley (United States)
Trevor M. Lanting, Univ. of California/Berkeley (United States)
Adrian T. Lee, Univ. of California/Berkeley (United States)
Lawrence Berkeley National Lab. (United States)
Erik M. Leitch, Univ. of Chicago (United States)
Jon Leong, Case Western Reserve Univ. (United States)
Wenyang Lu, Case Western Reserve Univ. (United States)
Martin Lueker, Univ. of California/Berkeley (United States)
Jared Mehl, Univ. of California/Berkeley (United States)
Stephan S. Meyer, Univ. of Chicago (United States)
Joe J. Mohr, Univ. of Illinois/Urbana-Champaign (United States)
Steve Padin, Univ. of Chicago (United States)
T. Plagge, Univ. of California/Berkeley (United States)
Clem Pryke, Univ. of Chicago (United States)
Marcus C. Runyan, Univ. of Chicago (United States)
Dan Schwan, Univ. of California/Berkeley (United States)
M. K. Sharp, Univ. of Chicago (United States)
Helmuth Spieler, Lawrence Berkeley National Lab. (United States)
Zak Staniszewski, Case Western Reserve Univ. (United States)
Antony A. Stark, Harvard-Smithsonian Ctr. for Astrophysics (United States)


Published in SPIE Proceedings Vol. 5498:
Millimeter and Submillimeter Detectors for Astronomy II
Jonas Zmuidzinas; Wayne S. Holland; Stafford Withington, Editor(s)

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