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BICEP3 focal plane design and detector performance

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arxiv 1607.06861 v1 pith:DOXL533F submitted 2016-07-22 astro-ph.IM

H. Hui , P. A. R. Ade , Z. Ahmed , K. D. Alexander , M. Amiri , D. Barkats , S. J. Benton , C. A. Bischoff
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J. J. Bock H. Boenish R. Bowens-Rubin I. Buder E. Bullock V. Buza J. Connors J. P. Filippini S. Fliescher J. A. Grayson M. Halpern S. Harrison G. C. Hilton V. V. Hristov 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 IV C. Pryke C. D. Reintsema S. Richter R. Schwarz C. Sorensen 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
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keywords bicep3performancedesigndetectorfocalplanetelescopeaperture
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abstract

BICEP3, the latest telescope in the BICEP/Keck program, started science observations in March 2016. It is a 550mm aperture refractive telescope observing the polarization of the cosmic microwave background at 95 GHz. We show the focal plane design and detector performance, including spectral response, optical efficiency and preliminary sensitivity of the upgraded BICEP3. We demonstrate 9.72$\mu$K$\sqrt{\textrm{s}}$ noise performance of the BICEP3 receiver.

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Cited by 1 Pith paper

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    astro-ph.IM 2026-06 accept novelty 3.0 of 10

    A new 296-detector 90 GHz TES bolometer array for CLASS achieves uniform properties, 16 μK√s NET, 0.37 optical efficiency, and a 41% mapping speed boost after addressing blue-leak radiation.

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