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Black Hole

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.

Dr. Boon Kok Tan

Senior Researcher

Research theme

  • Astronomy and astrophysics
  • Instrumentation

Sub department

  • Astrophysics

Research groups

  • Superconducting quantum detectors
boonkok.tan@physics.ox.ac.uk
Telephone: 01865 (2)73352
Denys Wilkinson Building, room 756
  • About
  • Publications

A new, simple method for fabricating high performance sub-mm focal plane arrays by direct machining using shaped drill bits

Authors:

JAMIE LEECH, GHASSAN YASSIN, Boon Kok TAN, Mike Tacon, Pichet Kittara, A Jiralucksanawong, S Wangsuya

Advances in Feed Horn Array Optics for Millimetre and Sub-Millimetre Receivers

Abstract:

Invited talk

An End-Fire SIS Mixer with Near Quantum-Limited Performance

Authors:

John Garrett, Boon-Kok Tan, Christine Chaumont, Faouzi Boussaha, Ghassan Yassin
More details from the publisher

An initial concept of a resonance phase matched junction-loaded travelling wave parametric tripler

Abstract:

In this paper, we investigate the possibility of utilising a tunnel-junction loaded transmission line as high efficiency parametric frequency multiplier. Through the interaction between the injected primary tone and the nonlinear medium, higher harmonic tones can be generated through wave-mixing process. Here, we aim to maximise the third harmonic wave generation. We first establish a theoretical framework outlining the mechanism for generating the third harmonic component from a single pump wave propagating in a nonlinear transmission line. We begin by demonstrating that strong third harmonic generation is possible with the resonance phase matching technique, albeit with an extremely narrow operational bandwidth. To broaden the bandwidth, we modify the dispersion engineering element of our circuit and show that broadband operation is achievable, while preventing unwanted harmonic tone growth. We extend this calculation from the microwave to the millimetre and sub-millimetre regimes and demonstrate that by adjusting the parameters of the junctions and the dispersion engineering circuits, we can achieve high conversion efficiency close to 1 THz.
Details from ORA

Astronomical Instrumentations for Millimetre and Sub-Millimetre Observations

Abstract:

Lecture for Graduate Students

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