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Title: Fabrication of Detector Arrays for the SPT-3G Receiver

Abstract

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.

Authors:
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Publication Date:
Research Org.:
SLAC National Accelerator Lab., Menlo Park, CA (United States); Argonne National Lab. (ANL), Argonne, IL (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Sponsoring Org.:
National Science Foundation (NSF); Gordon and Betty Moore Foundation (GBMF); USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
Contributing Org.:
SPT Team; SPT
OSTI Identifier:
1490485
Alternate Identifier(s):
OSTI ID: 1496029
Report Number(s):
FERMILAB-PUB-18-739-AE
Journal ID: ISSN 0022-2291; PII: 1924
Grant/Contract Number:  
PLR-1248097; AC02-76SF00515; AC02-06CH11357; PHY-1125897; GBMF 947; AC02-07CH11359; AST-0906135; AST- 1402161
Resource Type:
Accepted Manuscript
Journal Name:
Journal of Low Temperature Physics
Additional Journal Information:
Journal Volume: 193; Journal Issue: 5-6; Journal ID: ISSN 0022-2291
Publisher:
Springer
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Bolometers; Cosmic microwave background; TES detectors; Multichroic sensors; SPT-3G; 46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY

Citation Formats

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., and Young, M. R. Fabrication of Detector Arrays for the SPT-3G Receiver. United States: N. p., 2018. Web. doi:10.1007/s10909-018-1924-1.
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. United States. doi:10.1007/s10909-018-1924-1.
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., and Young, M. R. Tue . "Fabrication of Detector Arrays for the SPT-3G Receiver". United States. doi:10.1007/s10909-018-1924-1. https://www.osti.gov/servlets/purl/1490485.
@article{osti_1490485,
title = {Fabrication of Detector Arrays for the SPT-3G Receiver},
author = {Posada, C. M. and Ade, P. A. R. and Ahmed, Z. 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 Cecil, T. and Chang, C. L. and Cliche, J. F. and Cukierman, A. and Denison, E. V. and de Haan, T. and Ding, J. and Divan, R. and Dobbs, M. A. and Dutcher, D. and Everett, W. and Foster, A. and Gannon, R. N. and Gilbert, A. 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 Huang, N. and Irwin, K. D. and Jeong, O. B. and Jonas, M. and Khaire, T. and Kofman, A. M. and Korman, M. and Kubik, D. and Kuhlmann, S. and Kuo, C. L. and Lee, A. T. and Lowitz, A. E. and Meyer, S. S. and Michalik, D. and Miller, C. S. and Montgomery, J. and Nadolski, A. and Natoli, T. and Nguyen, H. and Noble, G. I. and Novosad, V. and Padin, S. and Pan, Z. and Pearson, J. and Rahlin, A. and Ruhl, J. E. and Saunders, L. J. and Sayre, J. T. and Shirley, I. and Shirokoff, E. and Smecher, G. and Sobrin, J. A. and Stan, L. and Stark, A. A. and Story, K. T. and Suzuki, A. and Tang, Q. Y. and Thompson, K. L. and Tucker, C. and Vale, L. R. and Vanderlinde, K. and Vieira, J. D. and Wang, G. and Whitehorn, N. and Yefremenko, V. and Yoon, K. W. and Young, M. R.},
abstractNote = {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.},
doi = {10.1007/s10909-018-1924-1},
journal = {Journal of Low Temperature Physics},
number = 5-6,
volume = 193,
place = {United States},
year = {2018},
month = {5}
}

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Thermal Links and Microstrip Transmission Lines in SPT-3G Bolometers
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Tuning SPT-3G Transition-Edge-Sensor Electrical Properties with a Four-Layer Ti–Au–Ti–Au Thin-Film Stack
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    Works referencing / citing this record:

    Thermal Links and Microstrip Transmission Lines in SPT-3G Bolometers
    journal, June 2018


    SPT-3G: A Multichroic Receiver for the South Pole Telescope
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    • Anderson, A. J.; Ade, P. A. R.; Ahmed, Z.
    • Journal of Low Temperature Physics, Vol. 193, Issue 5-6
    • DOI: 10.1007/s10909-018-2007-z