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A 230 GHz Finline SIS receiver with wide IF bandwidth

Abstract:
We have developed anSIS receiver with a wide intermediate-frequency (IF) bandwidth.This is important for reducing image integration time and simultaneously measuring multiple spectral lines. The receiver is a finline mixer-based design, which allows for ultra-wide radio-frequency (RF) bandwidth and has lower mechanical requirements compared to radial stub designs. Simulations of this receiver showed quantum limited noise in the RF frequency range of 140 to 260 GHzand from DC to 10GHz in the IF spectrum.We measured the noise temperature by comparing the receiver's response to hot and cold loads. The best noise temperature was 37.9 K at 231.0 GHz, and all of the results were below 100 K from 213 to 257 GHz (the bandwidth of our local-oscillator). We measured the IF bandwidth using a spectrum analyser, and found good results from around 3-10 GHz. The lower frequency was restricted by our IF amplifier's bandwidth but the higher frequency limit was lower than we expected from simulations. We believe that this discrepancywas due to the inductance of the bondwires that we used to connect the mixer chip to the IF board. We are currently investigating techniques to reduce and compensate for this inductance.
Publication status:
Published
Peer review status:
Peer reviewed

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
Role:
Author


Publisher:
International Symposium on Space Terahertz Technology
Host title:
27th International Symposium on Space Terahertz Technology, ISSTT 2016
Journal:
27th International Symposium on Space Terahertz Technology (ISSTT 2016) More from this journal
Publication date:
2017-01-01
Acceptance date:
2016-06-30


Pubs id:
pubs:705532
UUID:
uuid:f7a6a53e-5a49-4104-944a-9e0edddf222b
Local pid:
pubs:705532
Source identifiers:
705532
Deposit date:
2018-02-07

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