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Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Jee-Ho Kim

Graduate Students

Sub department

  • Astrophysics
jee-ho.kim@physics.ox.ac.uk
Denys Wilkinson Building, room 650
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Silicon-on-insulator membrane SIS mixers for Africa millimeter telescope Band 6+7 operation

National Radio Astronomy Observatory

Authors:

Jee-Ho Kim, Faouzi Boussaha, Christine Chaumont, Michele Piscitelli, Josiane Firminy, Etienne Eustache, Fabrice Stoppani, Andrey Baryshev, Boon Kok Tan

Abstract:

We present the design, simulation, fabrication, and initial characterization efforts toward a broadband superconductor-insulator-superconductor (SIS) mixer covering ALMA Bands 6 and 7 (211–373 GHz) on a single chip. The mixer employs a twin-junction SIS architecture integrated on a 10 µm-thick silicon-on-insulator (SOI) membrane substrate and is intended as a building block for future sideband-separating and dual-polarization receivers. To support the fabrication of these devices, front-side SIS circuit processing, SOI membrane release techniques, and gold beam-lead integration have been developed and refined. Initial device-release trials have successfully produced mixer chips with intact membranes and beam leads, while experimental setup for cryogenic mixer characterization has also been completed.
Details from ORA

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