Thermal Links and Microstrip Transmission Lines in SPT-3G Bolometers

J. Ding; P. A.R. Ade; Z. Ahmed; A. J. Anderson; J. E. Austermann; J. S. Avva; R. Basu Thakur; A. N. Bender; B. A. Benson; J. E. Carlstrom; F. W. Carter; T. Cecil; C. L. Chang; J. F. Cliche; A. Cukierman; E. V. Denison; T. de Haan; R. Divan; 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; W. L. Holzapfel; N. Huang; K. D. Irwin; O. B. Jeong; M. Jonas; T. Khaire; A. M. Kofman; M. Korman; D. Kubik; S. Kuhlmann; C. L. Kuo; A. T. Lee; A. E. Lowitz; S. S. Meyer; D. Michalik; C. S. Miller; J. Montgomery; A. Nadolski; T. Natoli; H. Nguyen; G. I. Noble; V. Novosad; S. Padin; Z. Pan; J. Pearson; C. M. Posada; A. Rahlin; J. E. Ruhl; L. J. Saunders; J. T. Sayre; I. Shirley; E. Shirokoff; G. Smecher; J. A. Sobrin; L. Stan; 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/s10909-018-1907-2

Thermal Links and Microstrip Transmission Lines in SPT-3G Bolometers

J. Ding, P. A.R. Ade, Z. Ahmed, A. J. Anderson, J. E. Austermann, J. S. Avva, R. Basu Thakur, A. N. Bender, B. A. Benson, J. E. Carlstrom, F. W. Carter, T. Cecil, C. L. Chang, J. F. Cliche, A. Cukierman, E. V. Denison, T. de Haan, R. Divan, M. A. Dobbs, D. DutcherW. 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, W. L. Holzapfel, N. Huang, K. D. Irwin, O. B. Jeong, M. Jonas, T. Khaire, A. M. Kofman, M. Korman, D. Kubik, S. Kuhlmann, C. L. Kuo, A. T. Lee, A. E. Lowitz, S. S. Meyer, D. Michalik, C. S. Miller, J. Montgomery, A. Nadolski, T. Natoli, H. Nguyen, G. I. Noble, V. Novosad, S. Padin, Z. Pan, J. Pearson, C. M. Posada, A. Rahlin, J. E. Ruhl, L. J. Saunders, J. T. Sayre, I. Shirley, E. Shirokoff, G. Smecher, J. A. Sobrin, L. Stan, 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

In this work, we have measured the properties of membrane-suspended bolometer thermal links and microstrip transmission lines in the transition-edge sensor arrays for the third-generation camera for South Pole Telescope (SPT-3G). A promising technique for controlling the end point of the release etch that defines the thermal link has been developed. We have also evaluated the microstrip loss in our detectors by measuring the optical efficiency of detectors with different lengths of microstrip line. The loss tangent is sufficiently low for the use in multi-chronic pixels for cosmic microwave background instruments like SPT-3G.

Original language	English (US)
Pages (from-to)	712-719
Number of pages	8
Journal	Journal of Low Temperature Physics
Volume	193
Issue number	5-6
DOIs	https://doi.org/10.1007/s10909-018-1907-2
State	Published - Dec 1 2018

Keywords

Cosmic microwave background
Microstrip loss
South Pole Telescope
Transition-edge sensor
XeF etch

ASJC Scopus subject areas

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

Online availability

10.1007/s10909-018-1907-2

Library availability

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Ding, J., Ade, P. A. R., Ahmed, Z., Anderson, A. J., Austermann, J. E., Avva, J. S., Thakur, R. B., Bender, A. N., Benson, B. A., Carlstrom, J. E., Carter, F. W., Cecil, T., Chang, C. L., Cliche, J. F., Cukierman, A., Denison, E. V., de Haan, T., Divan, R., Dobbs, M. A., ... Young, M. R. (2018). Thermal Links and Microstrip Transmission Lines in SPT-3G Bolometers. Journal of Low Temperature Physics, 193(5-6), 712-719. https://doi.org/10.1007/s10909-018-1907-2

Ding, J, Ade, PAR, Ahmed, Z, Anderson, AJ, Austermann, JE, Avva, JS, Thakur, RB, Bender, AN, Benson, BA, Carlstrom, JE, Carter, FW, Cecil, T, Chang, CL, Cliche, JF, Cukierman, A, Denison, EV, de Haan, T, Divan, R, 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, Holzapfel, WL, Huang, N, Irwin, KD, Jeong, OB, Jonas, M, Khaire, T, Kofman, AM, Korman, M, Kubik, D, Kuhlmann, S, Kuo, CL, Lee, AT, Lowitz, AE, Meyer, SS, Michalik, D, Miller, CS, Montgomery, J, Nadolski, A, Natoli, T, Nguyen, H, Noble, GI, Novosad, V, Padin, S, Pan, Z, Pearson, J, Posada, CM, Rahlin, A, Ruhl, JE, Saunders, LJ, Sayre, JT, Shirley, I, Shirokoff, E, Smecher, G, Sobrin, JA, Stan, L, 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, 'Thermal Links and Microstrip Transmission Lines in SPT-3G Bolometers', Journal of Low Temperature Physics, vol. 193, no. 5-6, pp. 712-719. https://doi.org/10.1007/s10909-018-1907-2

@article{3273876236174872b6ec83087870d670,

title = "Thermal Links and Microstrip Transmission Lines in SPT-3G Bolometers",

abstract = "In this work, we have measured the properties of membrane-suspended bolometer thermal links and microstrip transmission lines in the transition-edge sensor arrays for the third-generation camera for South Pole Telescope (SPT-3G). A promising technique for controlling the end point of the release etch that defines the thermal link has been developed. We have also evaluated the microstrip loss in our detectors by measuring the optical efficiency of detectors with different lengths of microstrip line. The loss tangent is sufficiently low for the use in multi-chronic pixels for cosmic microwave background instruments like SPT-3G.",

keywords = "Cosmic microwave background, Microstrip loss, South Pole Telescope, Transition-edge sensor, XeF etch",

author = "J. Ding and Ade, {P. A.R.} and Z. Ahmed and Anderson, {A. J.} and Austermann, {J. E.} and Avva, {J. S.} and Thakur, {R. Basu} and Bender, {A. N.} and Benson, {B. A.} and Carlstrom, {J. E.} and Carter, {F. W.} and T. Cecil and Chang, {C. L.} and Cliche, {J. F.} and A. Cukierman and Denison, {E. V.} and {de Haan}, T. and R. Divan 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 Holzapfel, {W. L.} and N. Huang and Irwin, {K. D.} and Jeong, {O. B.} and M. Jonas and T. Khaire and Kofman, {A. M.} and M. Korman and D. Kubik and S. Kuhlmann and Kuo, {C. L.} and Lee, {A. T.} and Lowitz, {A. E.} and Meyer, {S. S.} and D. Michalik and Miller, {C. S.} 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 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 L. Stan 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: The South Pole Telescope was supported in part by the National Science Foundation under Grant PLR-1248097, in part by the U.S. Department of Energy, in part by the Argonne National Laboratory and the Center for Nanoscale Materials, an Office of Science user facility, was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract DE-AC02- 06CH11357, in part by the NSF Physics Frontier Center under Grant PHY- 1125897 to the Kavli Institute of Cosmological Physics, University of Chicago, in part by the Kavli Foundation and the Gordon and Betty Moore Foundation under Grant GBMF 947, in part by Fermi National Accelerator Laboratory, a DOE-OS, HEP User Facility managed by the Fermi Research Alliance, LLC, and was supported under Contract No. DE-AC02-07CH11359. NWH acknowledges additional support from the NSF CAREER under Grant AST- 0956135. The McGill authors acknowledge funding from in part by the Natural Sciences and Engineering Research Council of Canada, in part by the Canadian Institute for Advanced Research and in part by the Canada Research Chairs program. Funding Information: Acknowledgements The South Pole Telescope was supported in part by the National Science Foundation under Grant PLR-1248097, in part by the U.S. Department of Energy, in part by the Argonne National Laboratory and the Center for Nanoscale Materials, an Office of Science user facility, was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract DE-AC02-06CH11357, in part by the NSF Physics Frontier Center under Grant PHY-1125897 to the Kavli Institute of Cosmological Physics, University of Chicago, in part by the Kavli Foundation and the Gordon and Betty Moore Foundation under Grant GBMF 947, in part by Fermi National Accelerator Laboratory, a DOE-OS, HEP User Facility managed by the Fermi Research Alliance, LLC, and was supported under Contract No. DE-AC02-07CH11359. NWH acknowledges additional support from the NSF CAREER under Grant AST-0956135. The McGill authors acknowledge funding from in part by the Natural Sciences and Engineering Research Council of Canada, in part by the Canadian Institute for Advanced Research and in part by the 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/s10909-018-1907-2",

language = "English (US)",

volume = "193",

pages = "712--719",

journal = "Journal of Low Temperature Physics",

issn = "0022-2291",

publisher = "Springer",

number = "5-6",

}

TY - JOUR

T1 - Thermal Links and Microstrip Transmission Lines in SPT-3G Bolometers

AU - Ding, J.

AU - Ade, P. A.R.

AU - Ahmed, Z.

AU - Anderson, A. J.

AU - Austermann, J. E.

AU - Avva, J. S.

AU - Thakur, R. Basu

AU - Bender, A. N.

AU - Benson, B. A.

AU - Carlstrom, J. E.

AU - Carter, F. W.

AU - Cecil, T.

AU - Chang, C. L.

AU - Cliche, J. F.

AU - Cukierman, A.

AU - Denison, E. V.

AU - de Haan, T.

AU - Divan, R.

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 - Holzapfel, W. L.

AU - Huang, N.

AU - Irwin, K. D.

AU - Jeong, O. B.

AU - Jonas, M.

AU - Khaire, T.

AU - Kofman, A. M.

AU - Korman, M.

AU - Kubik, D.

AU - Kuhlmann, S.

AU - Kuo, C. L.

AU - Lee, A. T.

AU - Lowitz, A. E.

AU - Meyer, S. S.

AU - Michalik, D.

AU - Miller, C. S.

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 - 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 - Stan, L.

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: The South Pole Telescope was supported in part by the National Science Foundation under Grant PLR-1248097, in part by the U.S. Department of Energy, in part by the Argonne National Laboratory and the Center for Nanoscale Materials, an Office of Science user facility, was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract DE-AC02- 06CH11357, in part by the NSF Physics Frontier Center under Grant PHY- 1125897 to the Kavli Institute of Cosmological Physics, University of Chicago, in part by the Kavli Foundation and the Gordon and Betty Moore Foundation under Grant GBMF 947, in part by Fermi National Accelerator Laboratory, a DOE-OS, HEP User Facility managed by the Fermi Research Alliance, LLC, and was supported under Contract No. DE-AC02-07CH11359. NWH acknowledges additional support from the NSF CAREER under Grant AST- 0956135. The McGill authors acknowledge funding from in part by the Natural Sciences and Engineering Research Council of Canada, in part by the Canadian Institute for Advanced Research and in part by the Canada Research Chairs program. Funding Information: Acknowledgements The South Pole Telescope was supported in part by the National Science Foundation under Grant PLR-1248097, in part by the U.S. Department of Energy, in part by the Argonne National Laboratory and the Center for Nanoscale Materials, an Office of Science user facility, was supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract DE-AC02-06CH11357, in part by the NSF Physics Frontier Center under Grant PHY-1125897 to the Kavli Institute of Cosmological Physics, University of Chicago, in part by the Kavli Foundation and the Gordon and Betty Moore Foundation under Grant GBMF 947, in part by Fermi National Accelerator Laboratory, a DOE-OS, HEP User Facility managed by the Fermi Research Alliance, LLC, and was supported under Contract No. DE-AC02-07CH11359. NWH acknowledges additional support from the NSF CAREER under Grant AST-0956135. The McGill authors acknowledge funding from in part by the Natural Sciences and Engineering Research Council of Canada, in part by the Canadian Institute for Advanced Research and in part by the 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 - In this work, we have measured the properties of membrane-suspended bolometer thermal links and microstrip transmission lines in the transition-edge sensor arrays for the third-generation camera for South Pole Telescope (SPT-3G). A promising technique for controlling the end point of the release etch that defines the thermal link has been developed. We have also evaluated the microstrip loss in our detectors by measuring the optical efficiency of detectors with different lengths of microstrip line. The loss tangent is sufficiently low for the use in multi-chronic pixels for cosmic microwave background instruments like SPT-3G.

AB - In this work, we have measured the properties of membrane-suspended bolometer thermal links and microstrip transmission lines in the transition-edge sensor arrays for the third-generation camera for South Pole Telescope (SPT-3G). A promising technique for controlling the end point of the release etch that defines the thermal link has been developed. We have also evaluated the microstrip loss in our detectors by measuring the optical efficiency of detectors with different lengths of microstrip line. The loss tangent is sufficiently low for the use in multi-chronic pixels for cosmic microwave background instruments like SPT-3G.

KW - Cosmic microwave background

KW - Microstrip loss

KW - South Pole Telescope

KW - Transition-edge sensor

KW - XeF etch

UR - http://www.scopus.com/inward/record.url?scp=85049131071&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85049131071&partnerID=8YFLogxK

U2 - 10.1007/s10909-018-1907-2

DO - 10.1007/s10909-018-1907-2

M3 - Article

AN - SCOPUS:85049131071

SN - 0022-2291

VL - 193

SP - 712

EP - 719

JO - Journal of Low Temperature Physics

JF - Journal of Low Temperature Physics

IS - 5-6

ER -

Thermal Links and Microstrip Transmission Lines in SPT-3G Bolometers

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