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Detection chain and electronic readout of the QUBIC instrument

Abstract:
The Q and U Bolometric Interferometer for Cosmology (QUBIC) Technical Demonstrator (TD) aiming to shows the feasibility of the combination of interferometry and bolometric detection. The electronic readout system is based on an array of 128 NbSi Transition Edge Sensors cooled at 350mK readout with 128 SQUIDs at 1K controlled and amplified by an Application Specific Integrated Circuit at 40K. This readout design allows a 128:1 Time Domain Multiplexing. We report the design and the performance of the detection chain in this paper. The technological demonstrator unwent a campaign of test in the lab. Evaluation of the QUBIC bolometers and readout electronics includes the measurement of I-V curves, time constant and the Noise Equivalent Power. Currently the mean Noise Equivalent Power is ~ 2 x 10-16W= p √Hz
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1117/12.2561567

Authors


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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Oxford college:
St Cross College
Role:
Author
ORCID:
0000-0002-8132-4896


Publisher:
Society of Photo-Optical Instrumentation Engineers
Host title:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X
Journal:
Proceedings of SPIE More from this journal
Volume:
11453
Article number:
1145328
Publication date:
2020-12-13
Acceptance date:
2020-02-24
Event title:
SPIE Astronomical Telescopes + Instrumentation 2020
Event location:
Virtual event.
Event website:
https://spie.org/conferences-and-exhibitions/astronomical-telescopes-and-instrumentation/
Event start date:
2020-12-14
Event end date:
2020-12-18
DOI:
EISSN:
1996-756X
ISSN:
0277-786X
ISBN:
9781510636934


Language:
English
Keywords:
Pubs id:
1162828
Local pid:
pubs:1162828
Deposit date:
2021-09-09

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