SPTpol: An instrument for CMB polarization

J. J. McMahon; K. A. Aird; B. A. Benson; L. E. Bleem; J. Britton; J. E. Carlstrom; C. L. Chang; H. S. Cho; T. Dehaan; T. M. Crawford; A. T. Crites; A. Datesman; M. A. Dobbs; W. Everett; N. W. Halverson; G. P. Holder; W. L. Holzapfel; D. Hmbes; K. D. Irwin; M. Joy; R. Keisler; T. M. Lanting; A. T. Lee; E. M. Leitch; A. Loehr; M. Lueker; J. Mehl; S. S. Meyer; J. J. Mohr; T. E. Montroy; M. D. Niemack; C. C. Ngeow; V. Novosad; S. Padin; T. Plagge; C. Pryke; C. Reichardt; J. E. Ruhl; K. K. Schaffer; L. Shaw; E. Shirokoff; H. G. Spieler; B. Stadler; A. A. Stark; Z. Staniszewski; K. Vanderlinde; J. D. Vieira; G. Wang; R. Wilhamson; V. Yefremenko; K. W. Yoon; O. Zhan; A. Zenteno

doi:10.1063/1.3292391

SPTpol: An instrument for CMB polarization

J. J. McMahon, K. A. Aird, B. A. Benson, L. E. Bleem, J. Britton, J. E. Carlstrom, C. L. Chang, H. S. Cho, T. Dehaan, T. M. Crawford, A. T. Crites, A. Datesman, M. A. Dobbs, W. Everett, N. W. Halverson, G. P. Holder, W. L. Holzapfel, D. Hmbes, K. D. Irwin, M. JoyR. Keisler, T. M. Lanting, A. T. Lee, E. M. Leitch, A. Loehr, M. Lueker, J. Mehl, S. S. Meyer, J. J. Mohr, T. E. Montroy, M. D. Niemack, C. C. Ngeow, V. Novosad, S. Padin, T. Plagge, C. Pryke, C. Reichardt, J. E. Ruhl, K. K. Schaffer, L. Shaw, E. Shirokoff, H. G. Spieler, B. Stadler, A. A. Stark, Z. Staniszewski, K. Vanderlinde, J. D. Vieira, G. Wang, R. Wilhamson, V. Yefremenko, K. W. Yoon, O. Zhan, A. Zenteno

Physics and Astronomy (Twin Cities)

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

56 Scopus citations

Abstract

SPTpol will consist of an 850 element polarization sensitive bolometric camera deployed to the South Pole Telescope in late 2011. This camera is optimized for measurement of the polarization of the cosmic microwave background with arcminute resolution. These measurements will be used to constrain neutrino masses and to constrain the amplitude of gravitational waves from inflation. The camera includes two detector architectures that observe in two different frequency bands. At 150 GHz, SPTpol will use 650 feedhorn-coupled TES polarimeters fabricated at NIST. At 90 GHz, it will use 200 absorber-coupled polarimeters developed at Argonne National Lab. The NIST pixels will be coupled to the telescope using a monolithic array of corrugated feeds and the Argonne devices will be coupled with individually machined contoured feeds. The entire focal plane will be readout using a digital frequency-domain multiplexer system. We provide an overview of the project, describe the detectors and discuss the design of this system.

Original language	English (US)
Title of host publication	Low Temperature Detectors LTD-13 - Proceedings of the 13th International Workshop
Pages	511-514
Number of pages	4
DOIs	https://doi.org/10.1063/1.3292391
State	Published - 2009
Event	13th International Workshop on Low Temperature Detectors, LTD-13 - Stanford, CA, United States Duration: Jul 20 2009 → Jul 24 2009

Publication series

Name	AIP Conference Proceedings
Volume	1185
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Other

Other	13th International Workshop on Low Temperature Detectors, LTD-13
Country/Territory	United States
City	Stanford, CA
Period	7/20/09 → 7/24/09

Keywords

Bolometers
Cosmic microwave background
Cosmology
Polarimetry
Transition-edge sensors

Publisher link

10.1063/1.3292391

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McMahon, J. J., Aird, K. A., Benson, B. A., Bleem, L. E., Britton, J., Carlstrom, J. E., Chang, C. L., Cho, H. S., Dehaan, T., Crawford, T. M., Crites, A. T., Datesman, A., Dobbs, M. A., Everett, W., Halverson, N. W., Holder, G. P., Holzapfel, W. L., Hmbes, D., Irwin, K. D., ... Zenteno, A. (2009). SPTpol: An instrument for CMB polarization. In Low Temperature Detectors LTD-13 - Proceedings of the 13th International Workshop (pp. 511-514). (AIP Conference Proceedings; Vol. 1185). https://doi.org/10.1063/1.3292391

McMahon, JJ, Aird, KA, Benson, BA, Bleem, LE, Britton, J, Carlstrom, JE, Chang, CL, Cho, HS, Dehaan, T, Crawford, TM, Crites, AT, Datesman, A, Dobbs, MA, Everett, W, Halverson, NW, Holder, GP, Holzapfel, WL, Hmbes, D, Irwin, KD, Joy, M, Keisler, R, Lanting, TM, Lee, AT, Leitch, EM, Loehr, A, Lueker, M, Mehl, J, Meyer, SS, Mohr, JJ, Montroy, TE, Niemack, MD, Ngeow, CC, Novosad, V, Padin, S, Plagge, T, Pryke, C, Reichardt, C, Ruhl, JE, Schaffer, KK, Shaw, L, Shirokoff, E, Spieler, HG, Stadler, B, Stark, AA, Staniszewski, Z, Vanderlinde, K, Vieira, JD, Wang, G, Wilhamson, R, Yefremenko, V, Yoon, KW, Zhan, O & Zenteno, A 2009, SPTpol: An instrument for CMB polarization. in Low Temperature Detectors LTD-13 - Proceedings of the 13th International Workshop. AIP Conference Proceedings, vol. 1185, pp. 511-514, 13th International Workshop on Low Temperature Detectors, LTD-13, Stanford, CA, United States, 7/20/09. https://doi.org/10.1063/1.3292391

@inproceedings{6cdcd2ef42f948979c6224014b61bbec,

title = "SPTpol: An instrument for CMB polarization",

abstract = "SPTpol will consist of an 850 element polarization sensitive bolometric camera deployed to the South Pole Telescope in late 2011. This camera is optimized for measurement of the polarization of the cosmic microwave background with arcminute resolution. These measurements will be used to constrain neutrino masses and to constrain the amplitude of gravitational waves from inflation. The camera includes two detector architectures that observe in two different frequency bands. At 150 GHz, SPTpol will use 650 feedhorn-coupled TES polarimeters fabricated at NIST. At 90 GHz, it will use 200 absorber-coupled polarimeters developed at Argonne National Lab. The NIST pixels will be coupled to the telescope using a monolithic array of corrugated feeds and the Argonne devices will be coupled with individually machined contoured feeds. The entire focal plane will be readout using a digital frequency-domain multiplexer system. We provide an overview of the project, describe the detectors and discuss the design of this system.",

keywords = "Bolometers, Cosmic microwave background, Cosmology, Polarimetry, Transition-edge sensors",

author = "McMahon, {J. J.} and Aird, {K. A.} and Benson, {B. A.} and Bleem, {L. E.} and J. Britton and Carlstrom, {J. E.} and Chang, {C. L.} and Cho, {H. S.} and T. Dehaan and Crawford, {T. M.} and Crites, {A. T.} and A. Datesman and Dobbs, {M. A.} and W. Everett and Halverson, {N. W.} and Holder, {G. P.} and Holzapfel, {W. L.} and D. Hmbes and Irwin, {K. D.} and M. Joy and R. Keisler and Lanting, {T. M.} and Lee, {A. T.} and Leitch, {E. M.} and A. Loehr and M. Lueker and J. Mehl and Meyer, {S. S.} and Mohr, {J. J.} and Montroy, {T. E.} and Niemack, {M. D.} and Ngeow, {C. C.} and V. Novosad and S. Padin and T. Plagge and C. Pryke and C. Reichardt and Ruhl, {J. E.} and Schaffer, {K. K.} and L. Shaw and E. Shirokoff and Spieler, {H. G.} and B. Stadler and Stark, {A. A.} and Z. Staniszewski and K. Vanderlinde and Vieira, {J. D.} and G. Wang and R. Wilhamson and V. Yefremenko and Yoon, {K. W.} and O. Zhan and A. Zenteno",

year = "2009",

doi = "10.1063/1.3292391",

language = "English (US)",

isbn = "9780735407510",

series = "AIP Conference Proceedings",

pages = "511--514",

booktitle = "Low Temperature Detectors LTD-13 - Proceedings of the 13th International Workshop",

note = "13th International Workshop on Low Temperature Detectors, LTD-13 ; Conference date: 20-07-2009 Through 24-07-2009",

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TY - GEN

T1 - SPTpol

T2 - 13th International Workshop on Low Temperature Detectors, LTD-13

AU - McMahon, J. J.

AU - Aird, K. A.

AU - Benson, B. A.

AU - Bleem, L. E.

AU - Britton, J.

AU - Carlstrom, J. E.

AU - Chang, C. L.

AU - Cho, H. S.

AU - Dehaan, T.

AU - Crawford, T. M.

AU - Crites, A. T.

AU - Datesman, A.

AU - Dobbs, M. A.

AU - Everett, W.

AU - Halverson, N. W.

AU - Holder, G. P.

AU - Holzapfel, W. L.

AU - Hmbes, D.

AU - Irwin, K. D.

AU - Joy, M.

AU - Keisler, R.

AU - Lanting, T. M.

AU - Lee, A. T.

AU - Leitch, E. M.

AU - Loehr, A.

AU - Lueker, M.

AU - Mehl, J.

AU - Meyer, S. S.

AU - Mohr, J. J.

AU - Montroy, T. E.

AU - Niemack, M. D.

AU - Ngeow, C. C.

AU - Novosad, V.

AU - Padin, S.

AU - Plagge, T.

AU - Pryke, C.

AU - Reichardt, C.

AU - Ruhl, J. E.

AU - Schaffer, K. K.

AU - Shaw, L.

AU - Shirokoff, E.

AU - Spieler, H. G.

AU - Stadler, B.

AU - Stark, A. A.

AU - Staniszewski, Z.

AU - Vanderlinde, K.

AU - Vieira, J. D.

AU - Wang, G.

AU - Wilhamson, R.

AU - Yefremenko, V.

AU - Yoon, K. W.

AU - Zhan, O.

AU - Zenteno, A.

PY - 2009

Y1 - 2009

N2 - SPTpol will consist of an 850 element polarization sensitive bolometric camera deployed to the South Pole Telescope in late 2011. This camera is optimized for measurement of the polarization of the cosmic microwave background with arcminute resolution. These measurements will be used to constrain neutrino masses and to constrain the amplitude of gravitational waves from inflation. The camera includes two detector architectures that observe in two different frequency bands. At 150 GHz, SPTpol will use 650 feedhorn-coupled TES polarimeters fabricated at NIST. At 90 GHz, it will use 200 absorber-coupled polarimeters developed at Argonne National Lab. The NIST pixels will be coupled to the telescope using a monolithic array of corrugated feeds and the Argonne devices will be coupled with individually machined contoured feeds. The entire focal plane will be readout using a digital frequency-domain multiplexer system. We provide an overview of the project, describe the detectors and discuss the design of this system.

AB - SPTpol will consist of an 850 element polarization sensitive bolometric camera deployed to the South Pole Telescope in late 2011. This camera is optimized for measurement of the polarization of the cosmic microwave background with arcminute resolution. These measurements will be used to constrain neutrino masses and to constrain the amplitude of gravitational waves from inflation. The camera includes two detector architectures that observe in two different frequency bands. At 150 GHz, SPTpol will use 650 feedhorn-coupled TES polarimeters fabricated at NIST. At 90 GHz, it will use 200 absorber-coupled polarimeters developed at Argonne National Lab. The NIST pixels will be coupled to the telescope using a monolithic array of corrugated feeds and the Argonne devices will be coupled with individually machined contoured feeds. The entire focal plane will be readout using a digital frequency-domain multiplexer system. We provide an overview of the project, describe the detectors and discuss the design of this system.

KW - Bolometers

KW - Cosmic microwave background

KW - Cosmology

KW - Polarimetry

KW - Transition-edge sensors

UR - http://www.scopus.com/inward/record.url?scp=74349084222&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=74349084222&partnerID=8YFLogxK

U2 - 10.1063/1.3292391

DO - 10.1063/1.3292391

M3 - Conference contribution

AN - SCOPUS:74349084222

SN - 9780735407510

T3 - AIP Conference Proceedings

SP - 511

EP - 514

BT - Low Temperature Detectors LTD-13 - Proceedings of the 13th International Workshop

Y2 - 20 July 2009 through 24 July 2009

ER -

SPTpol: An instrument for CMB polarization

Abstract

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Keywords

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