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Proceedings Paper

Development and characterization of the readout system for POLARBEAR-2
Author(s): D. Barron; P. A. R. Ade; Y. Akiba; C. Aleman; K. Arnold; M. Atlas; A. Bender; J. Borrill; S. Chapman; Y. Chinone; A. Cukierman; M. Dobbs; T. Elleflot; J. Errard; G. Fabbian; G. Feng; A. Gilbert; N. W. Halverson; M. Hasegawa; K. Hattori; M. Hazumi; W. L. Holzapfel; Y. Hori; Y. Inoue; G. C. Jaehnig; N. Katayama; B. Keating; Z. Kermish; R. Keskitalo; T. Kisner; M. Le Jeune; A. T. Lee; F. Matsuda; T. Matsumura; H. Morii; M. J. Myers; M. Navroli; H. Nishino; T. Okamura; J. Peloton; G. Rebeiz; C. L. Reichardt; P. L. Richards; C. Ross; M. Sholl; P. Siritanasak; G. Smecher; N. Stebor; B. Steinbach; R. Stompor; A. Suzuki; J. Suzuki; S. Takada; T. Takakura; T. Tomaru; B. Wilson; H. Yamaguchi; O. Zahn
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Paper Abstract

POLARBEAR-2 is a next-generation receiver for precision measurements of polarization of the cosmic microwave background, scheduled to deploy in 2015. It will feature a large focal plane, cooled to 250 milliKelvin, with 7,588 polarization-sensitive antenna-coupled transition edge sensor bolometers, read-out with frequency domain multiplexing with 32 bolometers on a single SQUID amplifier. We will present results from testing and characterization of new readout components, integrating these components into a scaled-down readout system for validation of the design and technology.

Paper Details

Date Published: 23 July 2014
PDF: 8 pages
Proc. SPIE 9153, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII, 915335 (23 July 2014); doi: 10.1117/12.2055611
Show Author Affiliations
D. Barron, Univ. of California, San Diego (United States)
P. A. R. Ade, Cardiff Univ. (United Kingdom)
Y. Akiba, The Graduate Univ. for Advanced Studies (Japan)
C. Aleman, Univ. of California, San Diego (United States)
K. Arnold, Univ. of California, San Diego (United States)
M. Atlas, Univ. of California, San Diego (United States)
A. Bender, McGill Univ. (Canada)
J. Borrill, Lawrence Berkeley National Lab. (United States)
Univ. of California, Berkeley (United States)
S. Chapman, Dalhousie Univ. (Canada)
Y. Chinone, High Energy Accelerator Research Organization, KEK (Japan)
Univ. of California, Berkeley (United States)
A. Cukierman, Univ. of California, Berkeley (United States)
M. Dobbs, McGill Univ. (Canada)
T. Elleflot, Univ. of California, San Diego (United States)
J. Errard, Univ. of California, Berkeley (United States)
Lawrence Berkeley National Lab. (United States)
G. Fabbian, AstroParticle et Cosmologie, CNRS, Univ. Paris Diderot (France)
Observatoire de Paris, IRFU-CEA (France)
International School for Advanced Studies (Italy)
G. Feng, Univ. of California, San Diego (United States)
A. Gilbert, McGill Univ. (Canada)
N. W. Halverson, Univ. of Colorado at Boulder (United States)
M. Hasegawa, High Energy Accelerator Research Organization, KEK (Japan)
The Graduate Univ. for Advanced Studies (Japan)
K. Hattori, High Energy Accelerator Research Organization, KEK (Japan)
M. Hazumi, High Energy Accelerator Research Organization, KEK (Japan)
The Graduate Univ. for Advanced Studies (Japan)
Kavli Institute for the Physics and Mathematics of the Universe, The Univ. of Tokyo (Japan)
W. L. Holzapfel, Univ. of California, Berkeley (United States)
Y. Hori, High Energy Accelerator Research Organization, KEK (Japan)
Y. Inoue, The Graduate Univ. for Advanced Studies (Japan)
G. C. Jaehnig, Univ. of Colorado at Boulder (United States)
N. Katayama, Kavli Institute for the Physics and Mathematics, The Univ. of Tokyo (Japan)
B. Keating, Univ. of California, San Diego (United States)
Z. Kermish, Princeton Univ. (United States)
R. Keskitalo, Lawrence Berkeley National Lab. (United States)
T. Kisner, Lawrence Berkeley National Lab. (United States)
Space Sciences Lab., Univ. of California, Berkeley (United States)
M. Le Jeune, AstroParticle et Cosmologie, CNRS, Univ. Paris Diderot (France)
Observatoire de Paris, IRFU-CEA (France)
A. T. Lee, Univ. of California, Berkeley (United States)
Lawrence Berkeley National Lab. (United States)
F. Matsuda, Univ. of California, San Diego (United States)
T. Matsumura, Japan Aerospace Exploration Agency (Japan)
H. Morii, High Energy Accelerator Research Organization, KEK (Japan)
M. J. Myers, Univ. of California, Berkeley (United States)
M. Navroli, Univ. of California, San Diego (United States)
H. Nishino, Kavli Institute for the Physics and Mathematics of the Universe, The Univ. of Tokyo (Japan)
T. Okamura, High Energy Accelerator Research Organization, KEK (Japan)
J. Peloton, AstroParticle et Cosmologie, CNRS, Univ. Paris Diderot (France)
Observatoire de Paris, IRFU-CEA (France)
G. Rebeiz, Univ. of California, San Diego (United States)
C. L. Reichardt, Univ. of California, Berkeley (United States)
P. L. Richards, Univ. of California, Berkeley (United States)
C. Ross, Dalhousie Univ. (Canada)
M. Sholl, Lawrence Berkeley National Lab. (United States)
P. Siritanasak, Univ. of California, San Diego (United States)
G. Smecher, Three-Speed Logic, Inc. (Canada)
N. Stebor, Univ. of California, San Diego (United States)
B. Steinbach, Univ. of California, Berkeley (United States)
R. Stompor, AstroParticle et Cosmologie, CNRS, Univ. Paris Diderot (France)
Observatoire de Paris, IRFU-CEA (France)
A. Suzuki, Univ. of California, Berkeley (United States)
J. Suzuki, High Energy Accelerator Research Organization, KEK (Japan)
S. Takada, National Institute for Fusion Science (Japan)
T. Takakura, Osaka Univ. (Japan)
High Energy Accelerator Research Organization KEK (Japan)
T. Tomaru, High Energy Accelerator Research Organization, KEK (Japan)
B. Wilson, Univ. of California, San Diego (United States)
H. Yamaguchi, High Energy Accelerator Research Organization, KEK (Japan)
O. Zahn, Lawrence Berkeley National Lab. (United States)


Published in SPIE Proceedings Vol. 9153:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII
Wayne S. Holland; Jonas Zmuidzinas, Editor(s)

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