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DC Field | Value | Language |
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dc.contributor.author | Darcy Barron | en_US |
dc.contributor.author | Kayla Mitchell | en_US |
dc.contributor.author | John Groh | en_US |
dc.contributor.author | Kam Arnold | en_US |
dc.contributor.author | Tucker Elleflot | en_US |
dc.contributor.author | Logan Howe | en_US |
dc.contributor.author | Jen Ito | en_US |
dc.contributor.author | Adrian T. Lee | en_US |
dc.contributor.author | Lindsay N. Lowry | en_US |
dc.contributor.author | Adam Anderson | en_US |
dc.contributor.author | Jessica Avva | en_US |
dc.contributor.author | Tylor Adkins | en_US |
dc.contributor.author | Carlo Baccigalupi | en_US |
dc.contributor.author | Kolen Cheung | en_US |
dc.contributor.author | Yuji Chinone | en_US |
dc.contributor.author | Oliver Jeong | en_US |
dc.contributor.author | Nobu Katayama | en_US |
dc.contributor.author | Brian Keating | en_US |
dc.contributor.author | Joshua Montgomery | en_US |
dc.contributor.author | Haruki Nishino | en_US |
dc.contributor.author | Christopher Raum | en_US |
dc.contributor.author | Praween Siritanasak | en_US |
dc.contributor.author | Aritoki Suzuki | en_US |
dc.contributor.author | Sayuri Takatori | en_US |
dc.contributor.author | Calvin Tsai | en_US |
dc.contributor.author | Benjamin Westbrook | en_US |
dc.contributor.author | Yuyang Zhou | en_US |
dc.date.accessioned | 2022-10-16T07:11:26Z | - |
dc.date.available | 2022-10-16T07:11:26Z | - |
dc.date.issued | 2021-08-01 | en_US |
dc.identifier.issn | 15582515 | en_US |
dc.identifier.issn | 10518223 | en_US |
dc.identifier.other | 2-s2.0-85103294306 | en_US |
dc.identifier.other | 10.1109/TASC.2021.3067190 | en_US |
dc.identifier.uri | https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85103294306&origin=inward | en_US |
dc.identifier.uri | http://cmuir.cmu.ac.th/jspui/handle/6653943832/76528 | - |
dc.description.abstract | Polarbear/Simons Array is a cosmic microwave background (CMB) polarization experiment, with science goals including a deep search for CMB B-mode polarization created by inflationary gravitational waves, and characterization of the CMB B-mode signal from gravitational lensing. When completed, Simons Array will have over 20,000 superconducting transition-edge sensor bolometers, cooled to 300 mK with closed-cycle cryogenics. This significant increase in detectors and sensitivity is enabled by advancements in frequency multiplexed readout. The detectors are read out with DfMux digital frequency-domain multiplexing, with 40 channels read out by each SQUID array, with frequency channels between 1 and 5 MHz defined by an inductor and capacitor in series with each detector. After the system was completed and characterized for Polarbear-2a, modifications were made that further improved performance for Polarbear-2b. We present the characterization of the integrated cryogenic readout system for Polarbear-2a and Polarbear-2b, and comparison of properties including stray impedance and frequency scatter. | en_US |
dc.subject | Engineering | en_US |
dc.subject | Materials Science | en_US |
dc.subject | Physics and Astronomy | en_US |
dc.title | Integrated Electrical Properties of the Frequency Multiplexed Cryogenic Readout System for Polarbear/Simons Array | en_US |
dc.type | Journal | en_US |
article.title.sourcetitle | IEEE Transactions on Applied Superconductivity | en_US |
article.volume | 31 | en_US |
article.stream.affiliations | Department of Physics | en_US |
article.stream.affiliations | Istituto Nazionale di Fisica Nucleare, Sezione di Trieste | en_US |
article.stream.affiliations | Research Center for the Early Universe | en_US |
article.stream.affiliations | The University of New Mexico | en_US |
article.stream.affiliations | The University of Tokyo | en_US |
article.stream.affiliations | University of California, Berkeley | en_US |
article.stream.affiliations | National Institute of Standards and Technology | en_US |
article.stream.affiliations | The Graduate University for Advanced Studies | en_US |
article.stream.affiliations | Harvard-Smithsonian Center for Astrophysics | en_US |
article.stream.affiliations | Fermi National Accelerator Laboratory | en_US |
article.stream.affiliations | Scuola Internazionale Superiore di Studi Avanzati | en_US |
article.stream.affiliations | Lawrence Berkeley National Laboratory | en_US |
article.stream.affiliations | High Energy Accelerator Research Organization, Tsukuba | en_US |
article.stream.affiliations | Université McGill | en_US |
article.stream.affiliations | Chiang Mai University | en_US |
article.stream.affiliations | Institute for Fundamental Physics of the Universe (IFPU) | en_US |
Appears in Collections: | CMUL: Journal Articles |
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