Fabrication of Detector Arrays for the SPT-3G Receiver
The South Pole Telescope third-generation (SPT-3G) receiver was installed during the austral summer of 2016–2017. It is designed to measure the cosmic microwave background across three frequency bands centered at 95, 150, and 220 GHz. The SPT-3G receiver has ten focal plane modules, each with 269 pi...
Published in: | Journal of Low Temperature Physics |
---|---|
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Language: | unknown |
Published: |
2022
|
Subjects: | |
Online Access: | http://www.osti.gov/servlets/purl/1496029 https://www.osti.gov/biblio/1496029 https://doi.org/10.1007/s10909-018-1924-1 |
id |
ftosti:oai:osti.gov:1496029 |
---|---|
record_format |
openpolar |
spelling |
ftosti:oai:osti.gov:1496029 2023-07-30T04:06:52+02:00 Fabrication of Detector Arrays for the SPT-3G Receiver Posada, C. M. Ade, P. A. R. Ahmed, Z. Anderson, A. J. Austermann, J. E. Avva, J. S. Thakur, R. Basu 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. Divan, R. Dobbs, M. A. Dutcher, D. Everett, W. Foster, A. Gannon, R. N. Gilbert, A. Groh, J. C. Halverson, N. W. Harke-Hosemann, A. H. Harrington, N. L. Henning, J. W. Hilton, G. C. Holzapfel, W. L. 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. Michalik, D. Miller, C. S. Montgomery, J. Nadolski, A. Natoli, T. Nguyen, H. Noble, G. I. Novosad, V. Padin, S. Pan, Z. Pearson, J. Rahlin, A. Ruhl, J. E. Saunders, L. J. Sayre, J. T. Shirley, I. Shirokoff, E. Smecher, G. Sobrin, J. A. Stan, L. 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. 2022-05-25 application/pdf http://www.osti.gov/servlets/purl/1496029 https://www.osti.gov/biblio/1496029 https://doi.org/10.1007/s10909-018-1924-1 unknown http://www.osti.gov/servlets/purl/1496029 https://www.osti.gov/biblio/1496029 https://doi.org/10.1007/s10909-018-1924-1 doi:10.1007/s10909-018-1924-1 79 ASTRONOMY AND ASTROPHYSICS 46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY 2022 ftosti https://doi.org/10.1007/s10909-018-1924-1 2023-07-11T09:31:27Z The South Pole Telescope third-generation (SPT-3G) receiver was installed during the austral summer of 2016–2017. It is designed to measure the cosmic microwave background across three frequency bands centered at 95, 150, and 220 GHz. The SPT-3G receiver has ten focal plane modules, each with 269 pixels. Each pixel features a broadband sinuous antenna coupled to a niobium microstrip transmission line. In-line filters define the desired band-passes before the signal is coupled to six bolometers with Ti/Au/Ti/Au transition edge sensors (three bands×two polarizations). In total, the SPT-3G receiver is composed of 16,000 detectors, which are read out using a 68× frequency-domain multiplexing scheme. In this paper, we present the process employed in fabricating the detector arrays. Other/Unknown Material South pole SciTec Connect (Office of Scientific and Technical Information - OSTI, U.S. Department of Energy) Austral South Pole Journal of Low Temperature Physics 193 5-6 703 711 |
institution |
Open Polar |
collection |
SciTec Connect (Office of Scientific and Technical Information - OSTI, U.S. Department of Energy) |
op_collection_id |
ftosti |
language |
unknown |
topic |
79 ASTRONOMY AND ASTROPHYSICS 46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY |
spellingShingle |
79 ASTRONOMY AND ASTROPHYSICS 46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY Posada, C. M. Ade, P. A. R. Ahmed, Z. Anderson, A. J. Austermann, J. E. Avva, J. S. Thakur, R. Basu 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. Divan, R. Dobbs, M. A. Dutcher, D. Everett, W. Foster, A. Gannon, R. N. Gilbert, A. Groh, J. C. Halverson, N. W. Harke-Hosemann, A. H. Harrington, N. L. Henning, J. W. Hilton, G. C. Holzapfel, W. L. 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. Michalik, D. Miller, C. S. Montgomery, J. Nadolski, A. Natoli, T. Nguyen, H. Noble, G. I. Novosad, V. Padin, S. Pan, Z. Pearson, J. Rahlin, A. Ruhl, J. E. Saunders, L. J. Sayre, J. T. Shirley, I. Shirokoff, E. Smecher, G. Sobrin, J. A. Stan, L. 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. Fabrication of Detector Arrays for the SPT-3G Receiver |
topic_facet |
79 ASTRONOMY AND ASTROPHYSICS 46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY |
description |
The South Pole Telescope third-generation (SPT-3G) receiver was installed during the austral summer of 2016–2017. It is designed to measure the cosmic microwave background across three frequency bands centered at 95, 150, and 220 GHz. The SPT-3G receiver has ten focal plane modules, each with 269 pixels. Each pixel features a broadband sinuous antenna coupled to a niobium microstrip transmission line. In-line filters define the desired band-passes before the signal is coupled to six bolometers with Ti/Au/Ti/Au transition edge sensors (three bands×two polarizations). In total, the SPT-3G receiver is composed of 16,000 detectors, which are read out using a 68× frequency-domain multiplexing scheme. In this paper, we present the process employed in fabricating the detector arrays. |
author |
Posada, C. M. Ade, P. A. R. Ahmed, Z. Anderson, A. J. Austermann, J. E. Avva, J. S. Thakur, R. Basu 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. Divan, R. Dobbs, M. A. Dutcher, D. Everett, W. Foster, A. Gannon, R. N. Gilbert, A. Groh, J. C. Halverson, N. W. Harke-Hosemann, A. H. Harrington, N. L. Henning, J. W. Hilton, G. C. Holzapfel, W. L. 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. Michalik, D. Miller, C. S. Montgomery, J. Nadolski, A. Natoli, T. Nguyen, H. Noble, G. I. Novosad, V. Padin, S. Pan, Z. Pearson, J. Rahlin, A. Ruhl, J. E. Saunders, L. J. Sayre, J. T. Shirley, I. Shirokoff, E. Smecher, G. Sobrin, J. A. Stan, L. 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. |
author_facet |
Posada, C. M. Ade, P. A. R. Ahmed, Z. Anderson, A. J. Austermann, J. E. Avva, J. S. Thakur, R. Basu 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. Divan, R. Dobbs, M. A. Dutcher, D. Everett, W. Foster, A. Gannon, R. N. Gilbert, A. Groh, J. C. Halverson, N. W. Harke-Hosemann, A. H. Harrington, N. L. Henning, J. W. Hilton, G. C. Holzapfel, W. L. 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. Michalik, D. Miller, C. S. Montgomery, J. Nadolski, A. Natoli, T. Nguyen, H. Noble, G. I. Novosad, V. Padin, S. Pan, Z. Pearson, J. Rahlin, A. Ruhl, J. E. Saunders, L. J. Sayre, J. T. Shirley, I. Shirokoff, E. Smecher, G. Sobrin, J. A. Stan, L. 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. |
author_sort |
Posada, C. M. |
title |
Fabrication of Detector Arrays for the SPT-3G Receiver |
title_short |
Fabrication of Detector Arrays for the SPT-3G Receiver |
title_full |
Fabrication of Detector Arrays for the SPT-3G Receiver |
title_fullStr |
Fabrication of Detector Arrays for the SPT-3G Receiver |
title_full_unstemmed |
Fabrication of Detector Arrays for the SPT-3G Receiver |
title_sort |
fabrication of detector arrays for the spt-3g receiver |
publishDate |
2022 |
url |
http://www.osti.gov/servlets/purl/1496029 https://www.osti.gov/biblio/1496029 https://doi.org/10.1007/s10909-018-1924-1 |
geographic |
Austral South Pole |
geographic_facet |
Austral South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
http://www.osti.gov/servlets/purl/1496029 https://www.osti.gov/biblio/1496029 https://doi.org/10.1007/s10909-018-1924-1 doi:10.1007/s10909-018-1924-1 |
op_doi |
https://doi.org/10.1007/s10909-018-1924-1 |
container_title |
Journal of Low Temperature Physics |
container_volume |
193 |
container_issue |
5-6 |
container_start_page |
703 |
op_container_end_page |
711 |
_version_ |
1772819826397413376 |