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Journal article

MKID digital readout tuning with deep learning

Abstract:

Microwave Kinetic Inductance Detector (MKID) devices offer inherent spectral resolution, simultaneous read out of thousands of pixels, and photon-limited sensitivity at optical wavelengths. Before taking observations the readout power and frequency of each pixel must be individually tuned, and if the equilibrium state of the pixels change, then the readout must be retuned. This process has previously been performed through manual inspection, and typically takes one hour per 500 resonators (20...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1016/j.ascom.2018.03.001

Authors


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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Particle Physics
Role:
Author
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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
Role:
Author
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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
Role:
Author
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Funding agency for:
Dodkins, R
Grant:
ST/M50371X/1
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Funding agency for:
O'Brien, K
Grant:
ST/M003868/1
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Funding agency for:
Thatte, N
Grant:
ST/N002717/1
Publisher:
Elsevier Publisher's website
Journal:
Astronomy and Computing Journal website
Volume:
23
Pages:
60-71
Publication date:
2018-03-13
Acceptance date:
2018-03-03
DOI:
ISSN:
2213-1337
Source identifiers:
828228
Keywords:
Pubs id:
pubs:828228
UUID:
uuid:75d47ccc-a33d-4466-ae16-a0df21618df3
Local pid:
pubs:828228
Deposit date:
2018-03-07

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