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. Lee; E. 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

doi:10.1364/AO.47.004418

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

Physics and Astronomy (Twin Cities)

Research output: Contribution to journal › Article › peer-review

63 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 language	English (US)
Pages (from-to)	4418-4428
Number of pages	11
Journal	Applied Optics
Volume	47
Issue number	24
DOIs	https://doi.org/10.1364/AO.47.004418
State	Published - Aug 20 2008

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Padin, S., Staniszewski, Z., Keisler, R., Joy, M., Stark, A. A., Ade, P. A. R., Aird, K. A., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Crawford, T. M., Crites, A. T., Dobbs, M. A., Halverson, N. W., Heimsath, S., Hills, R. E., Holzapfel, W. L., Lawrie, C., ... Vieira, J. D. (2008). South Pole Telescope optics. Applied Optics, 47(24), 4418-4428. https://doi.org/10.1364/AO.47.004418

Padin, S, Staniszewski, Z, Keisler, R, Joy, M, Stark, AA, Ade, PAR, Aird, KA, Benson, BA, Bleem, LE, Carlstrom, JE, Chang, CL, Crawford, TM, Crites, AT, Dobbs, MA, Halverson, NW, Heimsath, S, Hills, RE, Holzapfel, WL, Lawrie, C, Lee, AT, Leitch, EM, Leong, J, Lu, W, Lueker, M, McMahon, JJ, Meyer, SS, Mohr, JJ, Montroy, TE, Plagge, T, Pryke, C, Ruhl, JE, Schaffer, KK, Shirokoff, E, Spieler, HG & Vieira, JD 2008, 'South Pole Telescope optics', Applied Optics, vol. 47, no. 24, pp. 4418-4428. https://doi.org/10.1364/AO.47.004418

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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.",

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

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doi = "10.1364/AO.47.004418",

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AU - Padin, S.

AU - Staniszewski, Z.

AU - Keisler, R.

AU - Joy, M.

AU - Stark, A. A.

AU - Ade, P. A.R.

AU - Aird, K. A.

AU - Benson, B. A.

AU - Bleem, L. E.

AU - Carlstrom, J. E.

AU - Chang, C. L.

AU - Crawford, T. M.

AU - Crites, A. T.

AU - Dobbs, M. A.

AU - Halverson, N. W.

AU - Heimsath, S.

AU - Hills, R. E.

AU - Holzapfel, W. L.

AU - Lawrie, C.

AU - Lee, A. T.

AU - Leitch, E. M.

AU - Leong, J.

AU - Lu, W.

AU - Lueker, M.

AU - McMahon, J. J.

AU - Meyer, S. S.

AU - Mohr, J. J.

AU - Montroy, T. E.

AU - Plagge, T.

AU - Pryke, C.

AU - Ruhl, J. E.

AU - Schaffer, K. K.

AU - Shirokoff, E.

AU - Spieler, H. G.

AU - Vieira, J. D.

PY - 2008/8/20

Y1 - 2008/8/20

N2 - 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.

AB - 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.

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South Pole Telescope optics

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