91探花

Skip to main content
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding 91探花
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
  • Support
91探花
Black Hole

Lensing of space time around a black hole. At 91探花 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 High Performance 700 GHz Feed Horn

Journal of Infrared, Millimeter, and Terahertz Waves Springer Nature 33:1 (2012) 1-5

Authors:

Boon-Kok Tan, Jamie Leech, Ghassan Yassin, Phichet Kittara, Mike Tacon, Sujint Wangsuya, Christopher Groppi

Experimental Investigation of a Low-Cost, High Performance Focal-Plane Horn Array

IEEE Transactions on Terahertz Science and Technology Institute of Electrical and Electronics Engineers (IEEE) 2:1 (2012) 61-70

Authors:

Jamie Leech, Boon Kok Tan, Ghassan Yassin, Phichet Kittara, Sujint Wangsuya

Josephson pair tunnelling influence on the performance of an SIS mixer near its superconducting gap

International Journal of Terahertz Science and Technology Terahertz Science and Technology 4:3 (2011) 123-127

Authors:

Boon Tan, G Yassin

Abstract:

We report the investigation of the influence of Josephson pair tunnelling on the sensitivity of an SIS mixer near the superconducting gap of niobium. Hot and cold load measurements were carried out from 600 GHz to 700 GHz, without completely supressing the Josephson effect. We have noticed that when measurements were made at bias points near the first Shapiro step, significantly higher values of Y-factor could be obtained with magnetic field strengths that made the Shapiro step sharper, rather then those that supressed the step. This resulted in a significant improvement in noise temperature of the mixer at those bias points. This observation is important for SIS mixers operating at frequencies near or above gap frequency (蠅gap) because the warping of the second negative photon step to the positive display side, narrowing down the bias voltage interval in which measurement of the Y-factor at the first photon step could be done.

The influence of Josephson Pair Tunnelling on the Sensitivity of an SIS mixer Near the Superconducting Gap

4th UK/Europe Chine Workshop on Millimetre Waves and Terahertz Technologies University of Strathclyde (2011)

Authors:

Boon Tan, G Yassin

Abstract:

We report the investigation of the influence of Josephson pair tunnelling on the sensitivity of an SIS mixer near the superconducting gap of niobium. Hot and cold load measurements were carried out from 600 GHz to 700 GHz, without completely supressing the Josephson effect. We have noticed that when measurements were made at bias points near the first Shapiro step, significantly higher values of Y-factor could be obtained with magnetic field strengths that made the Shapiro step sharper, rather then those that supressed the step. This resulted in a significant improvement in noise temperature of the mixer at those bias points. This observation is important for SIS mixers operating at frequencies near or above gap frequency (蠅gap) because the warping of the second negative photon step to the positive display side, narrowing down the bias voltage interval in which measurement of the Y-factor at the first photon step could be done.

Multiple flare-angle horn feeds for sub-mm astronomy and cosmic microwave background experiments

Astronomy & Astrophysics EDP Sciences 532 (2011) a61

Authors:

J Leech, BK Tan, G Yassin, P Kittara, S Wangsuya, J Treuttel, M Henry, ML Oldfield, PG Huggard

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 18
  • Page 19
  • Page 20
  • Page 21
  • Current page 22
  • Page 23
  • Page 24
  • Page 25
  • Page 26
  • …
  • Next page Next
  • Last page Last

Footer 91探花

  • 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,

91探花,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

Department Of Physics text logo

漏 91探花 - Department of Physics

Cookies | Privacy policy | Accessibility statement

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Giving to Physics