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BICEP3 performance overview and planned Keck Array upgrade

Grayson, J. A. and Bock, J. J. and Filippini, J. P. and Hristov, V. V. and Hui, H. and Kefeli, S. and Lueker, M. and O'Brient, R. and Staniszewski, Z. K. and Steinbach, B. and Teply, G. P. (2016) BICEP3 performance overview and planned Keck Array upgrade. In: Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII. Proceedings of SPIE. No.9914. Society of Photo-Optical Instrumentation Engineers (SPIE) , Bellingham, WA, Art. No. 99140S. ISBN 978-1-5106-0207-6. http://resolver.caltech.edu/CaltechAUTHORS:20161114-153610613

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Abstract

Bicep3 is a 520mm aperture, compact two-lens refractor designed to observe the polarization of the cosmic microwave background (CMB) at 95 GHz. Its focal plane consists of modularized tiles of antenna-coupled transition edge sensors (TESs), similar to those used in Bicep2 and the Keck Array. The increased per-receiver optical throughput compared to Bicep2/Keck Array, due to both its faster f=1:7 optics and the larger aperture, more than doubles the combined mapping speed of the Bicep/Keck program. The Bicep3 receiver was recently upgraded to a full complement of 20 tiles of detectors (2560 TESs) and is now beginning its second year of observation (and first science season) at the South Pole. We report on its current performance and observing plans. Given its high per-receiver throughput while maintaining the advantages of a compact design, Bicep3- class receivers are ideally suited as building blocks for a 3rd-generation CMB experiment, consisting of multiple receivers spanning 35 GHz to 270 GHz with total detector count in the tens of thousands. We present plans for such an array, the new "BICEP Array" that will replace the Keck Array at the South Pole, including design optimization, frequency coverage, and deployment/observing strategies.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1117/12.2233894DOIArticle
http://proceedings.spiedigitallibrary.org/proceeding.aspx?articleid=2536906PublisherArticle
https://arxiv.org/abs/1607.04668arXivDiscussion Paper
Additional Information:© 2016 Society of Photo-Optical Instrumentation Engineers (SPIE). This work is supported by the National Science Foundation (grant nos. 1313158, 1313010, 1313062, 1313287, 1056465, 0960243), the SLAC Laboratory Directed Research and Development Fund, the Canada Foundation for Innovation, Science and Technology Facilities Council Consolidated Grant (ST/K000926/1), and the British Columbia Development Fund. The development of detector technology was supported by the JPL Research and Technology Development Fund and grants 06-ARPA206-0040, 10-SAT10-0017, and 12-SAT12-0031 from the NASA APRA and SAT programs. The development and testing of detector modules was supported by the Gordon and Betty Moore Foundation.
Funders:
Funding AgencyGrant Number
NSFPLR-1313158
NSFPLR-1313010
NSFPLR-1313062
NSFPLR-1313287
NSFAST-1056465
NSFPLR-0960243
Stanford Linear Accelerator CenterUNSPECIFIED
Canada Foundation for InnovationUNSPECIFIED
Science and Technology Facilities Council (STFC)ST/K000926/1
British Columbia Development FundUNSPECIFIED
JPL Research and Technology Development Fund06-ARPA206-0040
NASA10-SAT10-0017
NASA12-SAT12-0031
Gordon and Betty Moore FoundationUNSPECIFIED
Subject Keywords:Cosmic Microwave Background, Inflation, Gravitational Waves, Polarization, BICEP, Keck Array
Record Number:CaltechAUTHORS:20161114-153610613
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20161114-153610613
Official Citation:J. A. Grayson ; P. A. R. Ade ; Z. Ahmed ; K. D. Alexander ; M. Amiri ; D. Barkats ; S. J. Benton ; C. A. Bischoff ; J. J. Bock ; H. Boenish ; R. Bowens-Rubin ; I. Buder ; E. Bullock ; V. Buza ; J. Connors ; J. P. Filippini ; S. Fliescher ; M. Halpern ; S. Harrison ; G. C. Hilton ; V. V. Hristov ; H. Hui ; K. D. Irwin ; J. Kang ; K. S. Karkare ; E. Karpel ; S. Kefeli ; S. A. Kernasovskiy ; J. M. Kovac ; C. L. Kuo ; E. M. Leitch ; M. Lueker ; K. G. Megerian ; V. Monticue ; T. Namikawa ; C. B. Netterfield ; H. T. Nguyen ; R. O'Brient ; R. W. Ogburn ; C. Pryke ; C. D. Reintsema ; S. Richter ; R. Schwarz ; C. Sorenson ; C. D. Sheehy ; Z. K. Staniszewski ; B. Steinbach ; G. P. Teply ; K. L. Thompson ; J. E. Tolan ; C. Tucker ; A. D. Turner ; A. G. Vieregg ; A. Wandui ; A. C. Weber ; D. V. Wiebe ; J. Willmert ; W. L. K. Wu ; K. W. Yoon; BICEP3 performance overview and planned Keck Array upgrade. Proc. SPIE 9914, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII, 99140S (July 19, 2016); doi:10.1117/12.2233894.
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:72004
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:15 Nov 2016 21:40
Last Modified:14 Nov 2017 18:24

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