SPT-3G: A Multichroic Receiver for the South Pole Telescope

A. J. Anderson; P. A.R. Ade; Z. Ahmed; J. E. Austermann; J. S. Avva; P. S. Barry; R. Basu Thakur; A. N. Bender; B. A. Benson; L. E. Bleem; K. Byrum; J. E. Carlstrom; F. W. Carter; T. Cecil; C. L. Chang; H. M. Cho; J. F. Cliche; T. M. Crawford; A. Cukierman; E. V. Denison; T. de Haan; J. Ding; M. A. Dobbs; D. Dutcher; W. Everett; A. Foster; R. N. Gannon; A. Gilbert; J. C. Groh; N. W. Halverson; A. H. Harke-Hosemann; N. L. Harrington; J. W. Henning; G. C. Hilton; G. P. Holder; W. L. Holzapfel; N. Huang; K. D. Irwin; O. B. Jeong; M. Jonas; T. Khaire; L. Knox; A. M. Kofman; M. Korman; D. Kubik; S. Kuhlmann; N. Kuklev; C. L. Kuo; A. T. Lee; E. M. Leitch; A. E. Lowitz; S. S. Meyer; D. Michalik; J. Montgomery; A. Nadolski; T. Natoli; H. Nguyen; G. I. Noble; V. Novosad; S. Padin; Z. Pan; J. Pearson; C. M. Posada; A. Rahlin; C. L. Reichardt; J. E. Ruhl; L. J. Saunders; J. T. Sayre; I. Shirley; E. Shirokoff; G. Smecher; J. A. Sobrin; A. A. Stark; K. T. Story; A. Suzuki; Q. Y. Tang; K. L. Thompson; C. Tucker; L. R. Vale; K. Vanderlinde; J. D. Vieira; G. Wang; N. Whitehorn; V. Yefremenko; K. W. Yoon; M. R. Young

doi:10.1007/s10909-018-2007-z

SPT-3G: A Multichroic Receiver for the South Pole Telescope

A. J. Anderson, P. A.R. Ade, Z. Ahmed, J. E. Austermann, J. S. Avva, P. S. Barry, R. Basu Thakur, A. N. Bender, B. A. Benson, L. E. Bleem, K. Byrum, J. E. Carlstrom, F. W. Carter, T. Cecil, C. L. Chang, H. M. Cho, J. F. Cliche, T. M. Crawford, A. Cukierman, E. V. DenisonT. de Haan, J. Ding, M. A. Dobbs, D. Dutcher, W. Everett, A. Foster, R. N. Gannon, A. Gilbert, J. C. Groh, N. W. Halverson, A. H. Harke-Hosemann, N. L. Harrington, J. W. Henning, G. C. Hilton, G. P. Holder, W. L. Holzapfel, N. Huang, K. D. Irwin, O. B. Jeong, M. Jonas, T. Khaire, L. Knox, A. M. Kofman, M. Korman, D. Kubik, S. Kuhlmann, N. Kuklev, C. L. Kuo, A. T. Lee, E. M. Leitch, A. E. Lowitz, S. S. Meyer, D. Michalik, J. Montgomery, A. Nadolski, T. Natoli, H. Nguyen, G. I. Noble, V. Novosad, S. Padin, Z. Pan, J. Pearson, C. M. Posada, A. Rahlin, C. L. Reichardt, J. E. Ruhl, L. J. Saunders, J. T. Sayre, I. Shirley, E. Shirokoff, G. Smecher, J. A. Sobrin, A. A. Stark, K. T. Story, A. Suzuki, Q. Y. Tang, K. L. Thompson, C. Tucker, L. R. Vale, K. Vanderlinde, J. D. Vieira, G. Wang, N. Whitehorn, V. Yefremenko, K. W. Yoon, M. R. Young

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

Abstract

A new receiver for the South Pole Telescope, SPT-3G, was deployed in early 2017 to map the cosmic microwave background at 95, 150, and 220 GHz with ∼ 16,000 detectors, 10 times more than its predecessor SPTpol. The increase in detector count is made possible by lenslet-coupled trichroic polarization-sensitive pixels fabricated at Argonne National Laboratory, new 68× frequency-domain multiplexing readout electronics, and a higher-throughput optical design. The enhanced sensitivity of SPT-3G will enable a wide range of results including constraints on primordial B-mode polarization, measurements of gravitational lensing of the CMB, and a galaxy cluster survey. Here we present an overview of the instrument and its science objectives, highlighting its measured performance and plans for the upcoming 2018 observing season.

Original language	English (US)
Pages (from-to)	1057-1065
Number of pages	9
Journal	Journal of Low Temperature Physics
Volume	193
Issue number	5-6
DOIs	https://doi.org/10.1007/s10909-018-2007-z
State	Published - Dec 1 2018

Keywords

CMB
Instrumentation
Polarimetry
SPT-3G

ASJC Scopus subject areas

Atomic and Molecular Physics, and Optics
Materials Science(all)
Condensed Matter Physics

Online availability

10.1007/s10909-018-2007-z

Library availability

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Anderson, A. J., Ade, P. A. R., Ahmed, Z., Austermann, J. E., Avva, J. S., Barry, P. S., Thakur, R. B., Bender, A. N., Benson, B. A., Bleem, L. E., Byrum, K., Carlstrom, J. E., Carter, F. W., Cecil, T., Chang, C. L., Cho, H. M., Cliche, J. F., Crawford, T. M., Cukierman, A., ... Young, M. R. (2018). SPT-3G: A Multichroic Receiver for the South Pole Telescope. Journal of Low Temperature Physics, 193(5-6), 1057-1065. https://doi.org/10.1007/s10909-018-2007-z

Anderson, AJ, Ade, PAR, Ahmed, Z, Austermann, JE, Avva, JS, Barry, PS, Thakur, RB, Bender, AN, Benson, BA, Bleem, LE, Byrum, K, Carlstrom, JE, Carter, FW, Cecil, T, Chang, CL, Cho, HM, Cliche, JF, Crawford, TM, Cukierman, A, Denison, EV, de Haan, T, Ding, J, Dobbs, MA, Dutcher, D, Everett, W, Foster, A, Gannon, RN, Gilbert, A, Groh, JC, Halverson, NW, Harke-Hosemann, AH, Harrington, NL, Henning, JW, Hilton, GC, Holder, GP, Holzapfel, WL, Huang, N, Irwin, KD, Jeong, OB, Jonas, M, Khaire, T, Knox, L, Kofman, AM, Korman, M, Kubik, D, Kuhlmann, S, Kuklev, N, Kuo, CL, Lee, AT, Leitch, EM, Lowitz, AE, Meyer, SS, Michalik, D, Montgomery, J, Nadolski, A, Natoli, T, Nguyen, H, Noble, GI, Novosad, V, Padin, S, Pan, Z, Pearson, J, Posada, CM, Rahlin, A, Reichardt, CL, Ruhl, JE, Saunders, LJ, Sayre, JT, Shirley, I, Shirokoff, E, Smecher, G, Sobrin, JA, Stark, AA, Story, KT, Suzuki, A, Tang, QY, Thompson, KL, Tucker, C, Vale, LR, Vanderlinde, K, Vieira, JD, Wang, G, Whitehorn, N, Yefremenko, V, Yoon, KW & Young, MR 2018, 'SPT-3G: A Multichroic Receiver for the South Pole Telescope', Journal of Low Temperature Physics, vol. 193, no. 5-6, pp. 1057-1065. https://doi.org/10.1007/s10909-018-2007-z

@article{b099912d47b441d28cc88d924db8dad1,

title = "SPT-3G: A Multichroic Receiver for the South Pole Telescope",

abstract = "A new receiver for the South Pole Telescope, SPT-3G, was deployed in early 2017 to map the cosmic microwave background at 95, 150, and 220 GHz with ∼ 16,000 detectors, 10 times more than its predecessor SPTpol. The increase in detector count is made possible by lenslet-coupled trichroic polarization-sensitive pixels fabricated at Argonne National Laboratory, new 68× frequency-domain multiplexing readout electronics, and a higher-throughput optical design. The enhanced sensitivity of SPT-3G will enable a wide range of results including constraints on primordial B-mode polarization, measurements of gravitational lensing of the CMB, and a galaxy cluster survey. Here we present an overview of the instrument and its science objectives, highlighting its measured performance and plans for the upcoming 2018 observing season.",

keywords = "CMB, Instrumentation, Polarimetry, SPT-3G",

author = "Anderson, {A. J.} and Ade, {P. A.R.} and Z. Ahmed and Austermann, {J. E.} and Avva, {J. S.} and Barry, {P. S.} and Thakur, {R. Basu} and Bender, {A. N.} and Benson, {B. A.} and Bleem, {L. E.} and K. Byrum and Carlstrom, {J. E.} and Carter, {F. W.} and T. Cecil and Chang, {C. L.} and Cho, {H. M.} and Cliche, {J. F.} and Crawford, {T. M.} and A. Cukierman and Denison, {E. V.} and {de Haan}, T. and J. Ding and Dobbs, {M. A.} and D. Dutcher and W. Everett and A. Foster and Gannon, {R. N.} and A. Gilbert and Groh, {J. C.} and Halverson, {N. W.} and Harke-Hosemann, {A. H.} and Harrington, {N. L.} and Henning, {J. W.} and Hilton, {G. C.} and Holder, {G. P.} and Holzapfel, {W. L.} and N. Huang and Irwin, {K. D.} and Jeong, {O. B.} and M. Jonas and T. Khaire and L. Knox and Kofman, {A. M.} and M. Korman and D. Kubik and S. Kuhlmann and N. Kuklev and Kuo, {C. L.} and Lee, {A. T.} and Leitch, {E. M.} and Lowitz, {A. E.} and Meyer, {S. S.} and D. Michalik and J. Montgomery and A. Nadolski and T. Natoli and H. Nguyen and Noble, {G. I.} and V. Novosad and S. Padin and Z. Pan and J. Pearson and Posada, {C. M.} and A. Rahlin and Reichardt, {C. L.} and Ruhl, {J. E.} and Saunders, {L. J.} and Sayre, {J. T.} and I. Shirley and E. Shirokoff and G. Smecher and Sobrin, {J. A.} and Stark, {A. A.} and Story, {K. T.} and A. Suzuki and Tang, {Q. Y.} and Thompson, {K. L.} and C. Tucker and Vale, {L. R.} and K. Vanderlinde and Vieira, {J. D.} and G. Wang and N. Whitehorn and V. Yefremenko and Yoon, {K. W.} and Young, {M. R.}",

note = "Funding Information: Acknowledgements The South Pole Telescope is supported by the National Science Foundation (NSF) through Grant PLR-1248097. Partial support is also provided by the NSF Physics Frontier Center Grant Funding Information: PHY-1125897 to the Kavli Institute of Cosmological Physics at the University of Chicago, and the Kavli Foundation and the Gordon and Betty Moore Foundation Grant GBMF 947. Work at Argonne National Laboratory, including Laboratory Directed Research and Development support and Use of the Center for Nanoscale Materials, a US Department of Energy, Office of Science (DOE-OS) user facility, was supported under Contract No. DE-AC02-06CH11357. We acknowledge R. Divan, L. Stan, C.S. Miller, and V. Kutepova for supporting our work in the Argonne Center for Nanoscale Materials. Work at Fermi National Accelerator Laboratory, a DOE-OS, HEP User Facility managed by the Fermi Research Alliance, LLC, was supported under Contract No. DE-AC02-07CH11359. NWH acknowledges support from NSF CAREER Grant AST-0956135. The McGill authors acknowledge funding from the Natural Sciences and Engineering Research Council of Canada, Canadian Institute for Advanced Research, and Canada Research Chairs program. Funding Information: The South Pole Telescope is supported by the National Science Foundation (NSF) through Grant PLR-1248097. Partial support is also provided by the NSF Physics Frontier Center Grant PHY-1125897 to the Kavli Institute of Cosmological Physics at the University of Chicago, and the Kavli Foundation and the Gordon and Betty Moore Foundation Grant GBMF 947. Work at Argonne National Laboratory, including Laboratory Directed Research and Development support and Use of the Center for Nanoscale Materials, a US Department of Energy, Office of Science (DOE-OS) user facility, was supported under Contract No. DE-AC02-06CH11357. We acknowledge R. Divan, L. Stan, C.S. Miller, and V. Kutepova for supporting our work in the Argonne Center for Nanoscale Materials. Work at Fermi National Accelerator Laboratory, a DOE-OS, HEP User Facility managed by the Fermi Research Alliance, LLC, was supported under Contract No. DE-AC02-07CH11359. NWH acknowledges support from NSF CAREER Grant AST-0956135. The McGill authors acknowledge funding from the Natural Sciences and Engineering Research Council of Canada, Canadian Institute for Advanced Research, and Canada Research Chairs program. Publisher Copyright: {\textcopyright} 2018, This is a U.S. government work and its text is not subject to copyright protection in the United States; however, its text may be subject to foreign copyright protection.",

year = "2018",

month = dec,

day = "1",

doi = "10.1007/s10909-018-2007-z",

language = "English (US)",

volume = "193",

pages = "1057--1065",

journal = "Journal of Low Temperature Physics",

issn = "0022-2291",

publisher = "Springer",

number = "5-6",

}

TY - JOUR

T1 - SPT-3G

T2 - A Multichroic Receiver for the South Pole Telescope

AU - Anderson, A. J.

AU - Ade, P. A.R.

AU - Ahmed, Z.

AU - Austermann, J. E.

AU - Avva, J. S.

AU - Barry, P. S.

AU - Thakur, R. Basu

AU - Bender, A. N.

AU - Benson, B. A.

AU - Bleem, L. E.

AU - Byrum, K.

AU - Carlstrom, J. E.

AU - Carter, F. W.

AU - Cecil, T.

AU - Chang, C. L.

AU - Cho, H. M.

AU - Cliche, J. F.

AU - Crawford, T. M.

AU - Cukierman, A.

AU - Denison, E. V.

AU - de Haan, T.

AU - Ding, J.

AU - Dobbs, M. A.

AU - Dutcher, D.

AU - Everett, W.

AU - Foster, A.

AU - Gannon, R. N.

AU - Gilbert, A.

AU - Groh, J. C.

AU - Halverson, N. W.

AU - Harke-Hosemann, A. H.

AU - Harrington, N. L.

AU - Henning, J. W.

AU - Hilton, G. C.

AU - Holder, G. P.

AU - Holzapfel, W. L.

AU - Huang, N.

AU - Irwin, K. D.

AU - Jeong, O. B.

AU - Jonas, M.

AU - Khaire, T.

AU - Knox, L.

AU - Kofman, A. M.

AU - Korman, M.

AU - Kubik, D.

AU - Kuhlmann, S.

AU - Kuklev, N.

AU - Kuo, C. L.

AU - Lee, A. T.

AU - Leitch, E. M.

AU - Lowitz, A. E.

AU - Meyer, S. S.

AU - Michalik, D.

AU - Montgomery, J.

AU - Nadolski, A.

AU - Natoli, T.

AU - Nguyen, H.

AU - Noble, G. I.

AU - Novosad, V.

AU - Padin, S.

AU - Pan, Z.

AU - Pearson, J.

AU - Posada, C. M.

AU - Rahlin, A.

AU - Reichardt, C. L.

AU - Ruhl, J. E.

AU - Saunders, L. J.

AU - Sayre, J. T.

AU - Shirley, I.

AU - Shirokoff, E.

AU - Smecher, G.

AU - Sobrin, J. A.

AU - Stark, A. A.

AU - Story, K. T.

AU - Suzuki, A.

AU - Tang, Q. Y.

AU - Thompson, K. L.

AU - Tucker, C.

AU - Vale, L. R.

AU - Vanderlinde, K.

AU - Vieira, J. D.

AU - Wang, G.

AU - Whitehorn, N.

AU - Yefremenko, V.

AU - Yoon, K. W.

AU - Young, M. R.

N1 - Funding Information: Acknowledgements The South Pole Telescope is supported by the National Science Foundation (NSF) through Grant PLR-1248097. Partial support is also provided by the NSF Physics Frontier Center Grant Funding Information: PHY-1125897 to the Kavli Institute of Cosmological Physics at the University of Chicago, and the Kavli Foundation and the Gordon and Betty Moore Foundation Grant GBMF 947. Work at Argonne National Laboratory, including Laboratory Directed Research and Development support and Use of the Center for Nanoscale Materials, a US Department of Energy, Office of Science (DOE-OS) user facility, was supported under Contract No. DE-AC02-06CH11357. We acknowledge R. Divan, L. Stan, C.S. Miller, and V. Kutepova for supporting our work in the Argonne Center for Nanoscale Materials. Work at Fermi National Accelerator Laboratory, a DOE-OS, HEP User Facility managed by the Fermi Research Alliance, LLC, was supported under Contract No. DE-AC02-07CH11359. NWH acknowledges support from NSF CAREER Grant AST-0956135. The McGill authors acknowledge funding from the Natural Sciences and Engineering Research Council of Canada, Canadian Institute for Advanced Research, and Canada Research Chairs program. Funding Information: The South Pole Telescope is supported by the National Science Foundation (NSF) through Grant PLR-1248097. Partial support is also provided by the NSF Physics Frontier Center Grant PHY-1125897 to the Kavli Institute of Cosmological Physics at the University of Chicago, and the Kavli Foundation and the Gordon and Betty Moore Foundation Grant GBMF 947. Work at Argonne National Laboratory, including Laboratory Directed Research and Development support and Use of the Center for Nanoscale Materials, a US Department of Energy, Office of Science (DOE-OS) user facility, was supported under Contract No. DE-AC02-06CH11357. We acknowledge R. Divan, L. Stan, C.S. Miller, and V. Kutepova for supporting our work in the Argonne Center for Nanoscale Materials. Work at Fermi National Accelerator Laboratory, a DOE-OS, HEP User Facility managed by the Fermi Research Alliance, LLC, was supported under Contract No. DE-AC02-07CH11359. NWH acknowledges support from NSF CAREER Grant AST-0956135. The McGill authors acknowledge funding from the Natural Sciences and Engineering Research Council of Canada, Canadian Institute for Advanced Research, and Canada Research Chairs program. Publisher Copyright: © 2018, This is a U.S. government work and its text is not subject to copyright protection in the United States; however, its text may be subject to foreign copyright protection.

PY - 2018/12/1

Y1 - 2018/12/1

N2 - A new receiver for the South Pole Telescope, SPT-3G, was deployed in early 2017 to map the cosmic microwave background at 95, 150, and 220 GHz with ∼ 16,000 detectors, 10 times more than its predecessor SPTpol. The increase in detector count is made possible by lenslet-coupled trichroic polarization-sensitive pixels fabricated at Argonne National Laboratory, new 68× frequency-domain multiplexing readout electronics, and a higher-throughput optical design. The enhanced sensitivity of SPT-3G will enable a wide range of results including constraints on primordial B-mode polarization, measurements of gravitational lensing of the CMB, and a galaxy cluster survey. Here we present an overview of the instrument and its science objectives, highlighting its measured performance and plans for the upcoming 2018 observing season.

AB - A new receiver for the South Pole Telescope, SPT-3G, was deployed in early 2017 to map the cosmic microwave background at 95, 150, and 220 GHz with ∼ 16,000 detectors, 10 times more than its predecessor SPTpol. The increase in detector count is made possible by lenslet-coupled trichroic polarization-sensitive pixels fabricated at Argonne National Laboratory, new 68× frequency-domain multiplexing readout electronics, and a higher-throughput optical design. The enhanced sensitivity of SPT-3G will enable a wide range of results including constraints on primordial B-mode polarization, measurements of gravitational lensing of the CMB, and a galaxy cluster survey. Here we present an overview of the instrument and its science objectives, highlighting its measured performance and plans for the upcoming 2018 observing season.

KW - CMB

KW - Instrumentation

KW - Polarimetry

KW - SPT-3G

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EP - 1065

JO - Journal of Low Temperature Physics

JF - Journal of Low Temperature Physics

IS - 5-6

ER -

SPT-3G: A Multichroic Receiver for the South Pole Telescope

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