Fabrication of large dual-polarized multichroic TES bolometer arrays for CMB measurements with the SPT-3G camera
This paper presents the procedures used by Argonne National Laboratory to fabricate large arrays of multichroic transition-edge sensor (TES) bolometers for cosmic microwave background (CMB) measurements. These detectors will be assembled into the focal plane for the SPT-3G camera, the third generati...
Published in: | Superconductor Science and Technology |
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Online Access: | http://www.osti.gov/servlets/purl/1594616 https://www.osti.gov/biblio/1594616 https://doi.org/10.1088/0953-2048/28/9/094002 |
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ftosti:oai:osti.gov:1594616 2023-07-30T04:06:54+02:00 Fabrication of large dual-polarized multichroic TES bolometer arrays for CMB measurements with the SPT-3G camera Posada, C. M. Ade, P. A. R. Ahmed, Z. Arnold, K. Austermann, J. E. Bender, A. N. Bleem, L. E. Benson, B. A. Byrum, K. Carlstrom, J. E. Chang, C. L. Cho, H. M. Ciocys, S. T. Cliche, J. F. Crawford, T. M. Cukierman, A. Czaplewski, D. Ding, J. Divan, R. de Haan, T. Dobbs, M. A. Dutcher, D. Everett, W. Gilbert, A. Halverson, N. W. Harrington, N. L. Hattori, K. Henning, J. W. Hilton, G. C. Holzapfel, W. L. Hubmayr, J. Irwin, K. D. Jeong, O. Keisler, R. Kubik, D. Kuo, C. L. Lee, A. T. Leitch, E. M. Lendinez, S. Meyer, S. S. Miller, C. S. Montgomery, J. Myers, M. Nadolski, A. Natoli, T. Nguyen, H. Novosad, V. Padin, S. Pan, Z. Pearson, J. Ruhl, J. E. Saliwanchik, B. R. Smecher, G. Sayre, J. T. Shirokoff, E. Stan, L. Stark, A. A. Sobrin, J. Story, K. Suzuki, A. Thompson, K. L. Tucker, C. Vanderlinde, K. Vieira, J. D. Wang, G. Whitehorn, N. Yefremenko, V. Yoon, K. W. Ziegler, K. E. 2022-12-15 application/pdf http://www.osti.gov/servlets/purl/1594616 https://www.osti.gov/biblio/1594616 https://doi.org/10.1088/0953-2048/28/9/094002 unknown http://www.osti.gov/servlets/purl/1594616 https://www.osti.gov/biblio/1594616 https://doi.org/10.1088/0953-2048/28/9/094002 doi:10.1088/0953-2048/28/9/094002 79 ASTRONOMY AND ASTROPHYSICS 46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY 2022 ftosti https://doi.org/10.1088/0953-2048/28/9/094002 2023-07-11T09:39:19Z This paper presents the procedures used by Argonne National Laboratory to fabricate large arrays of multichroic transition-edge sensor (TES) bolometers for cosmic microwave background (CMB) measurements. These detectors will be assembled into the focal plane for the SPT-3G camera, the third generation CMB camera to be installed in the South Pole Telescope. The complete SPT-3G camera will have approximately 2690 pixels, for a total of 16,140 TES bolometric detectors. Each pixel is comprised of a broad-band sinuous antenna coupled to a Nb microstrip line. In-line filters are used to define the different band-passes before the millimeter-wavelength signal is fed to the respective Ti/Au TES bolometers. There are six TES bolometer detectors per pixel, which allow for measurements of three band-passes (95 GHz, 150 GHz and 220 GHz) and two polarizations. The steps involved in the monolithic fabrication of these detector arrays are presented here in detail. Patterns are defined using a combination of stepper and contact lithography. The misalignment between layers is kept below 200 nm. The overall fabrication involves a total of 16 processes, including reactive and magnetron sputtering, reactive ion etching, inductively coupled plasma etching and chemical etching. Other/Unknown Material South pole SciTec Connect (Office of Scientific and Technical Information - OSTI, U.S. Department of Energy) South Pole Superconductor Science and Technology 28 9 094002 |
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SciTec Connect (Office of Scientific and Technical Information - OSTI, U.S. Department of Energy) |
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language |
unknown |
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79 ASTRONOMY AND ASTROPHYSICS 46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY |
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79 ASTRONOMY AND ASTROPHYSICS 46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY Posada, C. M. Ade, P. A. R. Ahmed, Z. Arnold, K. Austermann, J. E. Bender, A. N. Bleem, L. E. Benson, B. A. Byrum, K. Carlstrom, J. E. Chang, C. L. Cho, H. M. Ciocys, S. T. Cliche, J. F. Crawford, T. M. Cukierman, A. Czaplewski, D. Ding, J. Divan, R. de Haan, T. Dobbs, M. A. Dutcher, D. Everett, W. Gilbert, A. Halverson, N. W. Harrington, N. L. Hattori, K. Henning, J. W. Hilton, G. C. Holzapfel, W. L. Hubmayr, J. Irwin, K. D. Jeong, O. Keisler, R. Kubik, D. Kuo, C. L. Lee, A. T. Leitch, E. M. Lendinez, S. Meyer, S. S. Miller, C. S. Montgomery, J. Myers, M. Nadolski, A. Natoli, T. Nguyen, H. Novosad, V. Padin, S. Pan, Z. Pearson, J. Ruhl, J. E. Saliwanchik, B. R. Smecher, G. Sayre, J. T. Shirokoff, E. Stan, L. Stark, A. A. Sobrin, J. Story, K. Suzuki, A. Thompson, K. L. Tucker, C. Vanderlinde, K. Vieira, J. D. Wang, G. Whitehorn, N. Yefremenko, V. Yoon, K. W. Ziegler, K. E. Fabrication of large dual-polarized multichroic TES bolometer arrays for CMB measurements with the SPT-3G camera |
topic_facet |
79 ASTRONOMY AND ASTROPHYSICS 46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY |
description |
This paper presents the procedures used by Argonne National Laboratory to fabricate large arrays of multichroic transition-edge sensor (TES) bolometers for cosmic microwave background (CMB) measurements. These detectors will be assembled into the focal plane for the SPT-3G camera, the third generation CMB camera to be installed in the South Pole Telescope. The complete SPT-3G camera will have approximately 2690 pixels, for a total of 16,140 TES bolometric detectors. Each pixel is comprised of a broad-band sinuous antenna coupled to a Nb microstrip line. In-line filters are used to define the different band-passes before the millimeter-wavelength signal is fed to the respective Ti/Au TES bolometers. There are six TES bolometer detectors per pixel, which allow for measurements of three band-passes (95 GHz, 150 GHz and 220 GHz) and two polarizations. The steps involved in the monolithic fabrication of these detector arrays are presented here in detail. Patterns are defined using a combination of stepper and contact lithography. The misalignment between layers is kept below 200 nm. The overall fabrication involves a total of 16 processes, including reactive and magnetron sputtering, reactive ion etching, inductively coupled plasma etching and chemical etching. |
author |
Posada, C. M. Ade, P. A. R. Ahmed, Z. Arnold, K. Austermann, J. E. Bender, A. N. Bleem, L. E. Benson, B. A. Byrum, K. Carlstrom, J. E. Chang, C. L. Cho, H. M. Ciocys, S. T. Cliche, J. F. Crawford, T. M. Cukierman, A. Czaplewski, D. Ding, J. Divan, R. de Haan, T. Dobbs, M. A. Dutcher, D. Everett, W. Gilbert, A. Halverson, N. W. Harrington, N. L. Hattori, K. Henning, J. W. Hilton, G. C. Holzapfel, W. L. Hubmayr, J. Irwin, K. D. Jeong, O. Keisler, R. Kubik, D. Kuo, C. L. Lee, A. T. Leitch, E. M. Lendinez, S. Meyer, S. S. Miller, C. S. Montgomery, J. Myers, M. Nadolski, A. Natoli, T. Nguyen, H. Novosad, V. Padin, S. Pan, Z. Pearson, J. Ruhl, J. E. Saliwanchik, B. R. Smecher, G. Sayre, J. T. Shirokoff, E. Stan, L. Stark, A. A. Sobrin, J. Story, K. Suzuki, A. Thompson, K. L. Tucker, C. Vanderlinde, K. Vieira, J. D. Wang, G. Whitehorn, N. Yefremenko, V. Yoon, K. W. Ziegler, K. E. |
author_facet |
Posada, C. M. Ade, P. A. R. Ahmed, Z. Arnold, K. Austermann, J. E. Bender, A. N. Bleem, L. E. Benson, B. A. Byrum, K. Carlstrom, J. E. Chang, C. L. Cho, H. M. Ciocys, S. T. Cliche, J. F. Crawford, T. M. Cukierman, A. Czaplewski, D. Ding, J. Divan, R. de Haan, T. Dobbs, M. A. Dutcher, D. Everett, W. Gilbert, A. Halverson, N. W. Harrington, N. L. Hattori, K. Henning, J. W. Hilton, G. C. Holzapfel, W. L. Hubmayr, J. Irwin, K. D. Jeong, O. Keisler, R. Kubik, D. Kuo, C. L. Lee, A. T. Leitch, E. M. Lendinez, S. Meyer, S. S. Miller, C. S. Montgomery, J. Myers, M. Nadolski, A. Natoli, T. Nguyen, H. Novosad, V. Padin, S. Pan, Z. Pearson, J. Ruhl, J. E. Saliwanchik, B. R. Smecher, G. Sayre, J. T. Shirokoff, E. Stan, L. Stark, A. A. Sobrin, J. Story, K. Suzuki, A. Thompson, K. L. Tucker, C. Vanderlinde, K. Vieira, J. D. Wang, G. Whitehorn, N. Yefremenko, V. Yoon, K. W. Ziegler, K. E. |
author_sort |
Posada, C. M. |
title |
Fabrication of large dual-polarized multichroic TES bolometer arrays for CMB measurements with the SPT-3G camera |
title_short |
Fabrication of large dual-polarized multichroic TES bolometer arrays for CMB measurements with the SPT-3G camera |
title_full |
Fabrication of large dual-polarized multichroic TES bolometer arrays for CMB measurements with the SPT-3G camera |
title_fullStr |
Fabrication of large dual-polarized multichroic TES bolometer arrays for CMB measurements with the SPT-3G camera |
title_full_unstemmed |
Fabrication of large dual-polarized multichroic TES bolometer arrays for CMB measurements with the SPT-3G camera |
title_sort |
fabrication of large dual-polarized multichroic tes bolometer arrays for cmb measurements with the spt-3g camera |
publishDate |
2022 |
url |
http://www.osti.gov/servlets/purl/1594616 https://www.osti.gov/biblio/1594616 https://doi.org/10.1088/0953-2048/28/9/094002 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
http://www.osti.gov/servlets/purl/1594616 https://www.osti.gov/biblio/1594616 https://doi.org/10.1088/0953-2048/28/9/094002 doi:10.1088/0953-2048/28/9/094002 |
op_doi |
https://doi.org/10.1088/0953-2048/28/9/094002 |
container_title |
Superconductor Science and Technology |
container_volume |
28 |
container_issue |
9 |
container_start_page |
094002 |
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1772819856506224640 |