Skip to main content
Home
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
Menu
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

650 GHz SIS mixer fabricated on silicon‐on‐insulator substrate

Electronics Letters Institution of Engineering and Technology (IET) 49:20 (2013) 1273-1275

Authors:

B‐K Tan, G Yassin, P Grimes, K Jacobs
More details from the publisher
More details

The James Clerk Maxwell Telescope Nearby Galaxies Legacy Survey IX: $^{12}$CO $J=3\to2$ Observations of NGC 2976 and NGC 3351

(2013)

Authors:

Boon-Kok Tan, J Leech, D Rigopoulou, BE Warren, CD Wilson, D Attewell, M Azimlu, GJ Bendo, HM Butner, E Brinks, P Chanial, DL Clements, V Heesen, F Israel, JH Knapen, HE Matthews, AMJ Mortier, Mühle, JR Sánchez-Gallego, RPJ Tilanus, A Usero, P van der Werf, M Zhu
More details from the publisher

A simple method to widen the IF bandwidth of a high frequency SIS mixer

24th International Symposium on Space Terahertz Technology (2013)

Authors:

Boon Tan, G Yassin, P Grimes

Abstract:

In this paper, we describe a simple method for widening the instantaneous frequency (IF) bandwidth of a high frequency superconductor-insulator-superconductor (SIS) mixer. This method requires only a standard PCB technology, without incurring any difficulties or complication in altering the tunnel junction fabrication. It involves the use of a simple multi-stage IF transformer to match the dynamic output impedance of the SIS mixer to a 50 Ω load over a wide IF bandwidth. We use an existing 650 GHz SIS mixer chip as an example to illustrate the methodology of the IF transformer design. In this example, we show how we widen the IF bandwidth of the mixer to operate over 4–12 GHz bandwidth using this simple impedance matching method.

Details from ORA

Easy to Fabricate Feeds for Astronomical Receivers

Institute of Electrical and Electronics Engineers (IEEE) (2013) 15-18

Authors:

Ghassan Yassin, Jamie Leech, Boon Kok Tan, Phichet Kittara
More details from the publisher
More details

Preliminary Measurement Results of a 650 GHz Planar Circuit Balanced SIS Mixer

IEEE Transactions on Terahertz Science and Technology Institute of Electrical and Electronics Engineers (IEEE) 3:1 (2013) 32-38

Authors:

Boon-Kok Tan, Ghassan Yassin, Paul Grimes, Karl Jacobs, Stafford Withington
More details from the publisher
More details

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 15
  • Page 16
  • Page 17
  • Page 18
  • Current page 19
  • Page 20
  • Page 21
  • Page 22
  • Page 23
  • …
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

University of Oxfrod logo Department Of Physics text logo
IOP Juno Champion logo Athena Swan Silver Award logo

© University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

Built by: Versantus

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Current students
  • Staff intranet