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Design and Assembly of SPT-3G Cold Readout Hardware
The third-generation upgrade to the receiver on the South Pole Telescope, SPT-3G, was installed at the South Pole during the 2016–2017 austral summer to measure the polarization of the cosmic microwave background. Increasing the number of detectors by a factor of 10 to ~16,000 required the multiplex...
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Published in: | Journal of low temperature physics 2018-05, Vol.193 (3-4) |
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creator | Avva, J. S. Ade, P. A. R. Ahmed, Z. Anderson, A. J. Austermann, J. E. Thakur, R. Basu Barron, D. 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. Ding, J. Dobbs, M. A. Dutcher, D. Elleflot, T. Everett, W. Foster, A. Gannon, R. N. Gilbert, A. Groh, J. C. Halverson, N. W. Harke-Hosemann, A. H. Harrington, N. L. Hasegawa, M. Hattori, K. Henning, J. W. Hilton, G. C. Holzapfel, W. L. Hori, Y. Huang, N. Irwin, K. D. Jeong, O. B. Jonas, M. Khaire, T. Kofman, A. M. Korman, M. Kubik, D. Kuhlmann, S. Kuo, C. L. Lee, A. T. Lowitz, A. E. Meyer, S. S. Montgomery, J. Nadolski, A. Natoli, T. Nguyen, H. Nishino, H. Noble, G. I. Novosad, V. Padin, S. Pan, Z. Pearson, J. Posada, C. M. Rahlin, A. Rotermund, K. Ruhl, J. E. Saunders, L. J. Sayre, J. T. Shirley, I. Shirokoff, E. Smecher, G. Sobrin, J. A. Stark, A. A. Story, K. T. Suzuki, A. Tang, Q. Y. Thompson, K. L. Tucker, C. Vale, L. R. Vanderlinde, K. Vieira, J. D. Wang, G. Whitehorn, N. Yefremenko, V. Yoon, K. W. Young, M. R. |
description | The third-generation upgrade to the receiver on the South Pole Telescope, SPT-3G, was installed at the South Pole during the 2016–2017 austral summer to measure the polarization of the cosmic microwave background. Increasing the number of detectors by a factor of 10 to ~16,000 required the multiplexing factor to increase to 68 and the bandwidth of the frequency-division readout electronics to span 1.6–5.2 MHz. This increase necessitates low-thermal conductance, low-inductance cryogenic wiring. Our cold readout system consists of planar thin-film aluminum inductive–capacitive resonators, wired in series with the detectors, summed together, and connected to 4K SQUIDs by 10-μm -thick niobium–titanium (NbTi) broadside-coupled striplines. Here, we present an overview of the cold readout electronics for SPT-3G, including assembly details and characterization of electrical and thermal properties of the system. We report, for the NbTi striplines, values of R≤10-4Ω , L=21±1 nH , and C=1.47±.02 nF . Additionally, the striplines’ thermal conductivity is described by kA=6.0±0.3 T0.92±0.04 μW mm K-1 . Finally, we provide projections for cross talk induced by parasitic impedances from the stripline and find that the median value of percentage cross talk from leakage current is 0.22 and 0.09% from wiring impedance. |
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V. ; de Haan, T. ; Ding, J. ; Dobbs, M. A. ; Dutcher, D. ; Elleflot, T. ; Everett, W. ; Foster, A. ; Gannon, R. N. ; Gilbert, A. ; Groh, J. C. ; Halverson, N. W. ; Harke-Hosemann, A. H. ; Harrington, N. L. ; Hasegawa, M. ; Hattori, K. ; Henning, J. W. ; Hilton, G. C. ; Holzapfel, W. L. ; Hori, Y. ; Huang, N. ; Irwin, K. D. ; Jeong, O. B. ; Jonas, M. ; Khaire, T. ; Kofman, A. M. ; Korman, M. ; Kubik, D. ; Kuhlmann, S. ; Kuo, C. L. ; Lee, A. T. ; Lowitz, A. E. ; Meyer, S. S. ; Montgomery, J. ; Nadolski, A. ; Natoli, T. ; Nguyen, H. ; Nishino, H. ; Noble, G. I. ; Novosad, V. ; Padin, S. ; Pan, Z. ; Pearson, J. ; Posada, C. M. ; Rahlin, A. ; Rotermund, K. ; Ruhl, J. E. ; Saunders, L. J. ; Sayre, J. T. ; Shirley, I. ; Shirokoff, E. ; Smecher, G. ; Sobrin, J. A. ; Stark, A. A. ; Story, K. T. ; Suzuki, A. ; Tang, Q. Y. ; Thompson, K. L. ; Tucker, C. ; Vale, L. R. ; Vanderlinde, K. ; Vieira, J. D. ; Wang, G. ; Whitehorn, N. ; Yefremenko, V. ; Yoon, K. W. ; Young, M. R.</creator><creatorcontrib>Avva, J. S. ; Ade, P. A. R. ; Ahmed, Z. ; Anderson, A. J. ; Austermann, J. E. ; Thakur, R. Basu ; Barron, D. ; 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. ; Ding, J. ; Dobbs, M. A. ; Dutcher, D. ; Elleflot, T. ; Everett, W. ; Foster, A. ; Gannon, R. N. ; Gilbert, A. ; Groh, J. C. ; Halverson, N. W. ; Harke-Hosemann, A. H. ; Harrington, N. L. ; Hasegawa, M. ; Hattori, K. ; Henning, J. W. ; Hilton, G. C. ; Holzapfel, W. L. ; Hori, Y. ; Huang, N. ; Irwin, K. D. ; Jeong, O. B. ; Jonas, M. ; Khaire, T. ; Kofman, A. M. ; Korman, M. ; Kubik, D. ; Kuhlmann, S. ; Kuo, C. L. ; Lee, A. T. ; Lowitz, A. E. ; Meyer, S. S. ; Montgomery, J. ; Nadolski, A. ; Natoli, T. ; Nguyen, H. ; Nishino, H. ; Noble, G. I. ; Novosad, V. ; Padin, S. ; Pan, Z. ; Pearson, J. ; Posada, C. M. ; Rahlin, A. ; Rotermund, K. ; Ruhl, J. E. ; Saunders, L. J. ; Sayre, J. T. ; Shirley, I. ; Shirokoff, E. ; Smecher, G. ; Sobrin, J. A. ; Stark, A. A. ; Story, K. T. ; Suzuki, A. ; Tang, Q. Y. ; Thompson, K. L. ; Tucker, C. ; Vale, L. R. ; Vanderlinde, K. ; Vieira, J. D. ; Wang, G. ; Whitehorn, N. ; Yefremenko, V. ; Yoon, K. W. ; Young, M. R. ; SLAC National Accelerator Lab., Menlo Park, CA (United States)</creatorcontrib><description>The third-generation upgrade to the receiver on the South Pole Telescope, SPT-3G, was installed at the South Pole during the 2016–2017 austral summer to measure the polarization of the cosmic microwave background. Increasing the number of detectors by a factor of 10 to ~16,000 required the multiplexing factor to increase to 68 and the bandwidth of the frequency-division readout electronics to span 1.6–5.2 MHz. This increase necessitates low-thermal conductance, low-inductance cryogenic wiring. Our cold readout system consists of planar thin-film aluminum inductive–capacitive resonators, wired in series with the detectors, summed together, and connected to 4K SQUIDs by 10-μm -thick niobium–titanium (NbTi) broadside-coupled striplines. Here, we present an overview of the cold readout electronics for SPT-3G, including assembly details and characterization of electrical and thermal properties of the system. We report, for the NbTi striplines, values of R≤10-4Ω , L=21±1 nH , and C=1.47±.02 nF . Additionally, the striplines’ thermal conductivity is described by kA=6.0±0.3 T0.92±0.04 μW mm K-1 . 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R.</creatorcontrib><creatorcontrib>SLAC National Accelerator Lab., Menlo Park, CA (United States)</creatorcontrib><title>Design and Assembly of SPT-3G Cold Readout Hardware</title><title>Journal of low temperature physics</title><description>The third-generation upgrade to the receiver on the South Pole Telescope, SPT-3G, was installed at the South Pole during the 2016–2017 austral summer to measure the polarization of the cosmic microwave background. Increasing the number of detectors by a factor of 10 to ~16,000 required the multiplexing factor to increase to 68 and the bandwidth of the frequency-division readout electronics to span 1.6–5.2 MHz. This increase necessitates low-thermal conductance, low-inductance cryogenic wiring. Our cold readout system consists of planar thin-film aluminum inductive–capacitive resonators, wired in series with the detectors, summed together, and connected to 4K SQUIDs by 10-μm -thick niobium–titanium (NbTi) broadside-coupled striplines. Here, we present an overview of the cold readout electronics for SPT-3G, including assembly details and characterization of electrical and thermal properties of the system. We report, for the NbTi striplines, values of R≤10-4Ω , L=21±1 nH , and C=1.47±.02 nF . Additionally, the striplines’ thermal conductivity is described by kA=6.0±0.3 T0.92±0.04 μW mm K-1 . Finally, we provide projections for cross talk induced by parasitic impedances from the stripline and find that the median value of percentage cross talk from leakage current is 0.22 and 0.09% from wiring impedance.</description><subject>ASTRONOMY AND ASTROPHYSICS</subject><subject>Cosmic microwave background</subject><subject>Frequency-division multiplexing</subject><subject>SPT-3G</subject><issn>0022-2291</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><recordid>eNpjYeA0MDAy0jUysjTkYOAqLs4yMDCwtDAz5mQwdkktzkzPU0jMS1FwLC5OzU3KqVTIT1MIDgjRNXZXcM7PSVEISk1MyS8tUfBILEopTyxK5WFgTUvMKU7lhdLcDEpuriHOHrr5xSWZ8cXJmSWpyRnJ-Xl5qckl8YYmlgYmFobGRCkCAJ8iMgo</recordid><startdate>20180524</startdate><enddate>20180524</enddate><creator>Avva, J. S.</creator><creator>Ade, P. A. R.</creator><creator>Ahmed, Z.</creator><creator>Anderson, A. J.</creator><creator>Austermann, J. E.</creator><creator>Thakur, R. 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N. ; Gilbert, A. ; Groh, J. C. ; Halverson, N. W. ; Harke-Hosemann, A. H. ; Harrington, N. L. ; Hasegawa, M. ; Hattori, K. ; Henning, J. W. ; Hilton, G. C. ; Holzapfel, W. L. ; Hori, Y. ; Huang, N. ; Irwin, K. D. ; Jeong, O. B. ; Jonas, M. ; Khaire, T. ; Kofman, A. M. ; Korman, M. ; Kubik, D. ; Kuhlmann, S. ; Kuo, C. L. ; Lee, A. T. ; Lowitz, A. E. ; Meyer, S. S. ; Montgomery, J. ; Nadolski, A. ; Natoli, T. ; Nguyen, H. ; Nishino, H. ; Noble, G. I. ; Novosad, V. ; Padin, S. ; Pan, Z. ; Pearson, J. ; Posada, C. M. ; Rahlin, A. ; Rotermund, K. ; Ruhl, J. E. ; Saunders, L. J. ; Sayre, J. T. ; Shirley, I. ; Shirokoff, E. ; Smecher, G. ; Sobrin, J. A. ; Stark, A. A. ; Story, K. T. ; Suzuki, A. ; Tang, Q. Y. ; Thompson, K. L. ; Tucker, C. ; Vale, L. R. ; Vanderlinde, K. ; Vieira, J. D. ; Wang, G. ; Whitehorn, N. ; Yefremenko, V. ; Yoon, K. W. ; Young, M. 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R.</creatorcontrib><creatorcontrib>Vanderlinde, K.</creatorcontrib><creatorcontrib>Vieira, J. D.</creatorcontrib><creatorcontrib>Wang, G.</creatorcontrib><creatorcontrib>Whitehorn, N.</creatorcontrib><creatorcontrib>Yefremenko, V.</creatorcontrib><creatorcontrib>Yoon, K. W.</creatorcontrib><creatorcontrib>Young, M. R.</creatorcontrib><creatorcontrib>SLAC National Accelerator Lab., Menlo Park, CA (United States)</creatorcontrib><collection>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><jtitle>Journal of low temperature physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Avva, J. S.</au><au>Ade, P. A. R.</au><au>Ahmed, Z.</au><au>Anderson, A. J.</au><au>Austermann, J. E.</au><au>Thakur, R. Basu</au><au>Barron, D.</au><au>Bender, A. N.</au><au>Benson, B. A.</au><au>Carlstrom, J. E.</au><au>Carter, F. W.</au><au>Cecil, T.</au><au>Chang, C. L.</au><au>Cliche, J. F.</au><au>Cukierman, A.</au><au>Denison, E. V.</au><au>de Haan, T.</au><au>Ding, J.</au><au>Dobbs, M. A.</au><au>Dutcher, D.</au><au>Elleflot, T.</au><au>Everett, W.</au><au>Foster, A.</au><au>Gannon, R. N.</au><au>Gilbert, A.</au><au>Groh, J. C.</au><au>Halverson, N. W.</au><au>Harke-Hosemann, A. H.</au><au>Harrington, N. L.</au><au>Hasegawa, M.</au><au>Hattori, K.</au><au>Henning, J. W.</au><au>Hilton, G. C.</au><au>Holzapfel, W. L.</au><au>Hori, Y.</au><au>Huang, N.</au><au>Irwin, K. D.</au><au>Jeong, O. B.</au><au>Jonas, M.</au><au>Khaire, T.</au><au>Kofman, A. M.</au><au>Korman, M.</au><au>Kubik, D.</au><au>Kuhlmann, S.</au><au>Kuo, C. L.</au><au>Lee, A. T.</au><au>Lowitz, A. E.</au><au>Meyer, S. S.</au><au>Montgomery, J.</au><au>Nadolski, A.</au><au>Natoli, T.</au><au>Nguyen, H.</au><au>Nishino, H.</au><au>Noble, G. I.</au><au>Novosad, V.</au><au>Padin, S.</au><au>Pan, Z.</au><au>Pearson, J.</au><au>Posada, C. M.</au><au>Rahlin, A.</au><au>Rotermund, K.</au><au>Ruhl, J. E.</au><au>Saunders, L. J.</au><au>Sayre, J. T.</au><au>Shirley, I.</au><au>Shirokoff, E.</au><au>Smecher, G.</au><au>Sobrin, J. A.</au><au>Stark, A. A.</au><au>Story, K. T.</au><au>Suzuki, A.</au><au>Tang, Q. Y.</au><au>Thompson, K. L.</au><au>Tucker, C.</au><au>Vale, L. R.</au><au>Vanderlinde, K.</au><au>Vieira, J. D.</au><au>Wang, G.</au><au>Whitehorn, N.</au><au>Yefremenko, V.</au><au>Yoon, K. W.</au><au>Young, M. R.</au><aucorp>SLAC National Accelerator Lab., Menlo Park, CA (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Design and Assembly of SPT-3G Cold Readout Hardware</atitle><jtitle>Journal of low temperature physics</jtitle><date>2018-05-24</date><risdate>2018</risdate><volume>193</volume><issue>3-4</issue><issn>0022-2291</issn><abstract>The third-generation upgrade to the receiver on the South Pole Telescope, SPT-3G, was installed at the South Pole during the 2016–2017 austral summer to measure the polarization of the cosmic microwave background. Increasing the number of detectors by a factor of 10 to ~16,000 required the multiplexing factor to increase to 68 and the bandwidth of the frequency-division readout electronics to span 1.6–5.2 MHz. This increase necessitates low-thermal conductance, low-inductance cryogenic wiring. Our cold readout system consists of planar thin-film aluminum inductive–capacitive resonators, wired in series with the detectors, summed together, and connected to 4K SQUIDs by 10-μm -thick niobium–titanium (NbTi) broadside-coupled striplines. Here, we present an overview of the cold readout electronics for SPT-3G, including assembly details and characterization of electrical and thermal properties of the system. We report, for the NbTi striplines, values of R≤10-4Ω , L=21±1 nH , and C=1.47±.02 nF . Additionally, the striplines’ thermal conductivity is described by kA=6.0±0.3 T0.92±0.04 μW mm K-1 . Finally, we provide projections for cross talk induced by parasitic impedances from the stripline and find that the median value of percentage cross talk from leakage current is 0.22 and 0.09% from wiring impedance.</abstract><cop>United States</cop><pub>Plenum Press</pub><orcidid>https://orcid.org/0000000323750229</orcidid><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0022-2291 |
ispartof | Journal of low temperature physics, 2018-05, Vol.193 (3-4) |
issn | 0022-2291 |
language | eng |
recordid | cdi_osti_scitechconnect_1490481 |
source | Springer Nature |
subjects | ASTRONOMY AND ASTROPHYSICS Cosmic microwave background Frequency-division multiplexing SPT-3G |
title | Design and Assembly of SPT-3G Cold Readout Hardware |
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