Antenna-coupled TES bolometer arrays for BICEP2/Keck and SPIDER
BICEP2/Keck and SPIDER are cosmic microwave background (CMB) polarimeters targeting the B-mode polarization induced by primordial gravitational waves from inflation. They will be using planar arrays of polarization sensitive antenna-coupled TES bolometers, operating at frequencies between 90 GHz and...
Published in: | SPIE Proceedings, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V |
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Online Access: | http://hdl.handle.net/2429/37250 https://doi.org/10.1117/12.857914 |
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ftunivbritcolcir:oai:circle.library.ubc.ca:2429/37250 2023-05-15T18:22:55+02:00 Antenna-coupled TES bolometer arrays for BICEP2/Keck and SPIDER Amiri, Mandana Burger, Bryce Halpern, Mark Hasselfield, Matthew 2010 http://hdl.handle.net/2429/37250 https://doi.org/10.1117/12.857914 eng eng Society of Photo-Optical Instrumentation Engineers (SPIE) Attribution-NonCommercial-NoDerivatives 4.0 International http://creativecommons.org/licenses/by-nc-nd/4.0/ Halpern, Mark CC-BY-NC-ND Text Conference Paper 2010 ftunivbritcolcir https://doi.org/10.1117/12.857914 2019-10-15T18:05:48Z BICEP2/Keck and SPIDER are cosmic microwave background (CMB) polarimeters targeting the B-mode polarization induced by primordial gravitational waves from inflation. They will be using planar arrays of polarization sensitive antenna-coupled TES bolometers, operating at frequencies between 90 GHz and 220 GHz. At 150 GHz each array consists of 64 polarimeters and four of these arrays are assembled together to make a focal plane, for a total of 256 dual-polarization elements (512 TES sensors). The detector arrays are integrated with a time-domain SQUID multiplexer developed at NIST and read out using the multi-channel electronics (MCE) developed at the University of British Columbia. Following our progress in improving detector parameters uniformity across the arrays and fabrication yield, our main effort has focused on improving detector arrays optical and noise performances, in order to produce science grade focal planes achieving target sensitivities. We report on changes in detector design implemented to optimize such performances and following focal plane arrays characterization. BICEP2 has deployed a first 150 GHz science grade focal plane to the South Pole in December 2009 Copyright 2010 Society of Photo-Optical Instrumentation Engineers. One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited. Science, Faculty of Physics and Astronomy, Department of Reviewed Faculty Conference Object South pole University of British Columbia: cIRcle - UBC's Information Repository South Pole SPIE Proceedings, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V 7741 77410H |
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University of British Columbia: cIRcle - UBC's Information Repository |
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English |
description |
BICEP2/Keck and SPIDER are cosmic microwave background (CMB) polarimeters targeting the B-mode polarization induced by primordial gravitational waves from inflation. They will be using planar arrays of polarization sensitive antenna-coupled TES bolometers, operating at frequencies between 90 GHz and 220 GHz. At 150 GHz each array consists of 64 polarimeters and four of these arrays are assembled together to make a focal plane, for a total of 256 dual-polarization elements (512 TES sensors). The detector arrays are integrated with a time-domain SQUID multiplexer developed at NIST and read out using the multi-channel electronics (MCE) developed at the University of British Columbia. Following our progress in improving detector parameters uniformity across the arrays and fabrication yield, our main effort has focused on improving detector arrays optical and noise performances, in order to produce science grade focal planes achieving target sensitivities. We report on changes in detector design implemented to optimize such performances and following focal plane arrays characterization. BICEP2 has deployed a first 150 GHz science grade focal plane to the South Pole in December 2009 Copyright 2010 Society of Photo-Optical Instrumentation Engineers. One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited. Science, Faculty of Physics and Astronomy, Department of Reviewed Faculty |
format |
Conference Object |
author |
Amiri, Mandana Burger, Bryce Halpern, Mark Hasselfield, Matthew |
spellingShingle |
Amiri, Mandana Burger, Bryce Halpern, Mark Hasselfield, Matthew Antenna-coupled TES bolometer arrays for BICEP2/Keck and SPIDER |
author_facet |
Amiri, Mandana Burger, Bryce Halpern, Mark Hasselfield, Matthew |
author_sort |
Amiri, Mandana |
title |
Antenna-coupled TES bolometer arrays for BICEP2/Keck and SPIDER |
title_short |
Antenna-coupled TES bolometer arrays for BICEP2/Keck and SPIDER |
title_full |
Antenna-coupled TES bolometer arrays for BICEP2/Keck and SPIDER |
title_fullStr |
Antenna-coupled TES bolometer arrays for BICEP2/Keck and SPIDER |
title_full_unstemmed |
Antenna-coupled TES bolometer arrays for BICEP2/Keck and SPIDER |
title_sort |
antenna-coupled tes bolometer arrays for bicep2/keck and spider |
publisher |
Society of Photo-Optical Instrumentation Engineers (SPIE) |
publishDate |
2010 |
url |
http://hdl.handle.net/2429/37250 https://doi.org/10.1117/12.857914 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_rights |
Attribution-NonCommercial-NoDerivatives 4.0 International http://creativecommons.org/licenses/by-nc-nd/4.0/ Halpern, Mark |
op_rightsnorm |
CC-BY-NC-ND |
op_doi |
https://doi.org/10.1117/12.857914 |
container_title |
SPIE Proceedings, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V |
container_volume |
7741 |
container_start_page |
77410H |
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1766202334099013632 |