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Antenna-coupled TES Bolometer Arrays for BICEP2/Keck and SPIDER

Orlando, A. and Aikin, R. W. and Bock, J. J. and Brevik, J. A. and Filippini, J. P. and Golwala, S. R. and Lange, A. E. and Ogburn, R. W. and Runyan, M. C. and Sudiwala, R. and Teply, G. and Trangsrud, A. R. (2010) Antenna-coupled TES Bolometer Arrays for BICEP2/Keck and SPIDER. In: Millimeter, submillimeter, and far-infrared detectors and instrumentation for astronomy V. Proceedings of SPIE. No.7741. Society of Photo-optical Instrumentation Engineers (SPIE) , Bellingham, WA, Art. No. 77410H. ISBN 978-0-81948-231-0. https://resolver.caltech.edu/CaltechAUTHORS:20110315-094044621

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Abstract

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.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1117/12.857914DOIArticle
http://proceedings.spiedigitallibrary.org/proceeding.aspx?articleid=751864PublisherArticle
ORCID:
AuthorORCID
Bock, J. J.0000-0002-5710-5212
Filippini, J. P.0000-0001-8217-6832
Golwala, S. R.0000-0002-1098-7174
Additional Information:© 2010 SPIE. We would like to thank the Gordon and Betty Moore Foundation, the National Aeronautics and Space Administration, the JPL Research and Technology Development Fund and the W.M. Keck Foundation. We also acknowledge NASA Postdoctoral Program support for Zak Staniszewski.
Funders:
Funding AgencyGrant Number
Gordon and Betty Moore FoundationUNSPECIFIED
NASA Postdoctoral ProgramUNSPECIFIED
JPL Research and Technology Development FundUNSPECIFIED
W. M. Keck FoundationUNSPECIFIED
Series Name:Proceedings of SPIE
Issue or Number:7741
Record Number:CaltechAUTHORS:20110315-094044621
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20110315-094044621
Official Citation:A. Orlando ; R. W. Aikin ; M. Amiri ; J. J. Bock ; J. A. Bonetti ; J. A. Brevik ; B. Burger ; G. Chattopadthyay ; P. K. Day ; J. P. Filippini ; S. R. Golwala ; M. Halpern ; M. Hasselfield ; G. C. Hilton ; K. D. Irwin ; M. Kenyon ; J. M. Kovac ; C. L. Kuo ; A. E. Lange ; H. G. LeDuc ; N. Llombart ; H. T. Nguyen ; R. W. Ogburn ; C. D. Reintsema ; M. C. Runyan ; Z. Staniszewski ; R. Sudiwala ; G. Teply ; A. R. Trangsrud ; A. D. Turner and P. Wilson "Antenna-coupled TES bolometer arrays for BICEP2/Keck and SPIDER", Proc. SPIE 7741, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V, 77410H (July 15, 2010); doi:10.1117/12.857914; http://dx.doi.org/10.1117/12.857914
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:22893
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:16 Mar 2011 22:36
Last Modified:10 Dec 2019 21:49

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