South Pole Telescope optics

S. Padin, Z. Staniszewski, R. Keisler, M. Joy, A. A. Stark, P. A.R. Ade, K. A. Aird, B. A. Benson, L. E. Bleem, J. E. Carlstrom, C. L. Chang, T. M. Crawford, A. T. Crites, M. A. Dobbs, N. W. Halverson, S. Heimsath, R. E. Hills, W. L. Holzapfel, C. Lawrie, A. T. LeeE. M. Leitch, J. Leong, W. Lu, M. Lueker, J. J. McMahon, S. S. Meyer, J. J. Mohr, T. E. Montroy, T. Plagge, C. Pryke, J. E. Ruhl, K. K. Schaffer, E. Shirokoff, H. G. Spieler, J. D. Vieira

Research output: Contribution to journalArticlepeer-review

66 Scopus citations

Abstract

The South Pole Telescope is a 10 m diameter, wide-field, offset Gregorian telescope with a 966-pixel, millimeter-wave, bolometer array receiver. The telescope has an unusual optical system with a cold stop around the secondary. The design emphasizes low scattering and low background loading. All the optical components except the primary are cold, and the entire beam from prime focus to the detectors is surrounded by cold absorber.

Original languageEnglish (US)
Pages (from-to)4418-4428
Number of pages11
JournalApplied Optics
Volume47
Issue number24
DOIs
StatePublished - Aug 20 2008

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