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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.

Ghassan Yassin

Emeriti

Sub department

  • Astrophysics

Research groups

  • Superconducting quantum detectors
ghassan.yassin@physics.ox.ac.uk
Telephone: 01865 (2)73440
Denys Wilkinson Building, room 750
  • About
  • Publications

A superconducting millimetre switch with multiple nano-bridges

ISSTT 2014 - 25th International Sympsoium on Space Terahertz Technology, Proceedings (2014) 164-169

Authors:

BK Tan, G Yassin, L Kuzmin, E Otto, H Merabet, C North

Abstract:

In this paper, we describe the design of a planar superconducting on/off switch comprising a high normal resistance nano-bridge deposited across a slotline transmission line. We present preliminary experimental results measured at 220 GHz range, and we discuss in detail the various parameters that affect the performance of the planar on/off switch, including the optimum thickness required for the nano-bridge to achieve high dynamic range and low transmission loss. The analysis is done by combining the accurate superconducting surface impedance description with rigorous electromagnetic simulations, and comparing the simulated results with the measured performance of a previously fabricated on/off switch fed by a backto- back unilateral finline taper. Finally, we propose an improved method to further increase the dynamic range of the switch, by introducing a multi-bridge design to tune out the residual inductance of the nano-bridges.

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
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Easy to fabricate feeds for astronomical receivers

2013 International Workshop on Antenna Technology, iWAT 2013 (2013) 15-18

Authors:

G Yassin, J Leech, BK Tan, P Kittara

Abstract:

Modern ground-based radio-telescopes have stringent requirements on the receiver's feed-horn performance. These include a bandwidth covering a full atmospheric window from good sites (∼ 30%), low cross polarization and high beam circularity. In addition the unprecedented sensitivity required by recent proposed experiments requires large format focal plane arrays consisting of a large number of high performance feeds. While these feeds are straightforward to fabricate at microwave frequencies, the tight tolerances required in the THz region makes the realization of a large format array both expensive and time consuming. In this paper we describe feed designs that can be fabricated cheaply and rapidly without compromising the science requirements within the operating bandwidth. We present simulated and measured far-field beam patterns showing low sidelobe levels, good beam circularity and low cross-polarization levels over a fractional bandwidth of 20%. Having demonstrated the efficacy of our horn designs and fabricating technique experimentally, we have designed, fabricated and tested a prototype focal plane array of 37 hexagonally close packed horns milled in a single block of aluminum. Experimental testing of the radiation patterns of the array feeds demonstrated that they were essentially identical to the patterns of the feeds fabricated individually and that cross coupling between adjacent feeds was negligible. © 2013 IEEE.
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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
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Smooth walled feed horns for mm and submm radio astronomy

UCMMT 2013 - 2013 6th UK, Europe, China Millimeter Waves and THz Technology Workshop (2013)

Authors:

J Leech, BK Tan, G Yassin

Abstract:

Here we describe our work designing multiple flare-angle horns, optimised using a genetic algorithm. Several horns designs will be described and experimentally measured beam patterns for horns at 230 GHz will be presented. In addition, we will present new, wide bandwidth horns offering good performance over a ∼30% bandwidth. © 2013 IEEE.
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