Antenna-coupled TES bolometers used in BICEP2, Keck Array, and SPIDER

Ade, P. A.  R.; Aikin, R. W.; Amiri, M.; Barkats, D.; Benton, S. J.; Bischoff, C. A.; Bock, J. J.; Bonetti, J. A.; Brevik, J. A.; Buder, I.; Bullock, E.; Chattopadhyay, G.; Davis, G.; Day, P. K.; Dowell, C. D.; Duband, L.; Filippini, J. P.; Fliescher, S.; Golwala, S. R.; Halpern, M.; Hasselfield, M.; Hildebrandt, S. R.; Hilton, G. C.; Hristov, V.; Hui, H.; Irwin, K. D.; Jones, W. C.; Karkare, K. S.; Kaufman, J. P.; Keating, B. G.; Kefeli, S.; Kernasovskiy, S. A.; Kovac, J. M.; Kuo, C. L.; LeDuc, H. G.; Leitch, E. M.; Llombart, N.; Lueker, M.; Mason, P.; Megerian, K.; Moncelsi, L.; Netterfield, C. B.; Nguyen, H. T.; O’Brient, R.; IV, R. W.  Ogburn; Orlando, A.; Pryke, C.; Rahlin, A. S.; Reintsema, C. D.; Richter, S.; Runyan, M. C.; Schwarz, R.; Sheehy, C. D.; Staniszewski, Z. K.; Sudiwala, R. V.; Teply, G. P.; Tolan, J. E.; Trangsrud, A.; Tucker, R. S.; Turner, A. D.; Vieregg, A. G.; Weber, A.; Wiebe, D. V.; Wilson, P.; Wong, C. L.; Yoon, K. W.; Zmuidzinas, J.

doi:10.1088/0004-637X/812/2/176

Title: Antenna-coupled TES bolometers used in BICEP2, Keck Array, and SPIDER

Journal Article · Tue Oct 20 00:00:00 EDT 2015 · The Astrophysical Journal (Online)

DOI:https://doi.org/10.1088/0004-637X/812/2/176· OSTI ID:1263390

Ade, P. A. R.; Aikin, R. W.; Amiri, M.; Barkats, D.; Benton, S. J.; Bischoff, C. A.; Bock, J. J.; Bonetti, J. A.; Brevik, J. A.; Buder, I.; Bullock, E.; Chattopadhyay, G.; Davis, G.; Day, P. K.; Dowell, C. D.; Duband, L.; Filippini, J. P.; Fliescher, S.; Golwala, S. R.; Halpern, M. more »

We have developed antenna-coupled transition-edge sensor bolometers for a wide range of cosmic microwave background (CMB) polarimetry experiments, including Bicep2, Keck Array, and the balloon borne Spider. These detectors have reached maturity and this paper reports on their design principles, overall performance, and key challenges associated with design and production. Our detector arrays repeatedly produce spectral bands with 20%–30% bandwidth at 95, 150, or 230 GHz. The integrated antenna arrays synthesize symmetric co-aligned beams with controlled side-lobe levels. Cross-polarized response on boresight is typically $$\sim 0.5\%$$, consistent with cross-talk in our multiplexed readout system. End-to-end optical efficiencies in our cameras are routinely 35% or higher, with per detector sensitivities of NET ~ 300 $$\mu {{\rm{K}}}_{\mathrm{CMB}}\sqrt{{\rm{s}}}$$. Thanks to the scalability of this design, we have deployed 2560 detectors as 1280 matched pairs in Keck Array with a combined instantaneous sensitivity of $$\sim 9\;\mu {{\rm{K}}}_{\mathrm{CMB}}\sqrt{{\rm{s}}}$$, as measured directly from CMB maps in the 2013 season. Furthermore, similar arrays have recently flown in the Spider instrument, and development of this technology is ongoing.

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Research Organization:: SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

Contributing Organization:: Bicep2, Keck Array, and Spider Collaborations

Grant/Contract Number:: AC02-76SF00515

OSTI ID:: 1263390

Report Number(s):: SLAC-PUB-16648; arXiv:1502.00619

Journal Information:: The Astrophysical Journal (Online), Vol. 812, Issue 2; ISSN 1538-4357

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 54 works

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79 ASTRONOMY AND ASTROPHYSICS
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instrumentation: detectors
instrumentation: polarimeters
methods: laboratory: solid-state
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Title: Antenna-coupled TES bolometers used in BICEP2, Keck Array, and SPIDER

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