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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

The JCMT Nearby Galaxies Legacy Survey III: Comparisons of cold dust, polycyclic aromatic hydrocarbons, molecular gas, and atomic gas in NGC 2403

(2009)

Authors:

GJ Bendo, CD Wilson, BE Warren, E Brinks, HM Butner, P Chanial, DL Clements, S Courteau, J Irwin, FP Israel, JH Knapen, J Leech, HE Matthews, S Muehle, G Petitpas, S Serjeant, BK Tan, RPJ Tilanus, A Usero, M Vaccari, P van der Werf, C Vlahakis, T Wiegert, M Zhu
More details from the publisher

Digitalized Mirror Array and Its Application in Large Telescope: Principle and Case Studies

Communications in Theoretical Physics IOP Publishing 52:4 (2009) 750-760

Authors:

Chen Ying-Tian, Zhang Yang, Hu Sen, Ho Tso-Hsiu, Boon Ham Lim, Chen Sin Lim, Kok Keong Chong, Boon Kok Tan
More details from the publisher

Measurement of electron-phonon interaction time of niobium using heating effect in SIS tunnel junction

20th International Symposium on Space Terahertz Technology National Radio Astronomy Observatory (2009) 275-277

Authors:

Boon Tan, G Yassin, P Kittara, J Leech

Abstract:

The heating of SIS tunnel junctions by local oscillator (LO) power and bias voltage is well known and has been reported previously. In this paper, we present a novel method for recovering the heating parameters from the experimental pumped I-V curves of an SIS device at 700 GHz, together with the coupled LO power and the embedding impedance. Since this is obtained without assuming a particular power law between LO power and junction temperature, we will be able to find τeph, the electron-phonon interaction time of the superconducting material at various bath temperatures. We would deduce a power law that describes the dependence of the heat flow equation on temperature.

Details from ORA

Unilateral finline transition at THz frequencies

International Symposium on Space Terahertz Technology National Radio Astronomy Observatory (2009) 263-266

Authors:

Boon Tan, G Yassin

Abstract:

We present a new type of waveguide to microstrip transition designs for a 700 GHz SIS mixer. The transition comprised a unilateral finline taper and the RF power from the finline slot is coupled through coplanar waveguide to microstrip using two radial stubs. This transition is significantly easier to design and fabricate than the conventional antipodal finline taper since the fins do not overlap at any stage. A key feature of this design is that it can be deposited on Silicon-on-Insulator resulting in a finline mixer chip on approximately 15 µm silicon substrate. This allows the mixer chip to be held in the E-plane of the waveguide without a supporting groove in the waveguide wall, avoiding the excitation of higher order modes. The chip is simply supported by gold leads deposited on the substrate. It should be emphasized that the employment of such substrate will also decrease the loss and allow finline mixers design to be extended to the THz region.

Details from ORA

THE JAMES CLERK MAXWELL TELESCOPE NEARBY GALAXIES LEGACY SURVEY. I. STAR-FORMING MOLECULAR GAS IN VIRGO CLUSTER SPIRAL GALAXIES

The Astrophysical Journal American Astronomical Society 693:2 (2009) 1736-1748

Authors:

CD Wilson, BE Warren, FP Israel, S Serjeant, G Bendo, E Brinks, D Clements, S Courteau, J Irwin, JH Knapen, J Leech, HE Matthews, S Mühle, AMJ Mortier, G Petitpas, E Sinukoff, K Spekkens, BK Tan, RPJ Tilanus, A Usero, P van der Werf, T Wiegert, M Zhu
More details from the publisher

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