AMSTAR - Advanced Millimetre and Sub-mm Technology for Astronomical Research
03 Dec 2010
Yes
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The overall objective of Focal Plane Array Development​ is to design, construct and demonstrate a novel focal plane heterodyne array receiver suitable for radio astronomical use within the millimetre wavelength range (2-3mm).

No

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This will be achieved through the development and integration of a novel photomixing local oscillator (LO) with a super-conducting tunnel junction (SIS) detector element in a common waveguide embedding circuit.

The project is a joint activity between the Rutherford Appleton Laboratory and the Institut de RadioAstronomie Millimétrique (link opens in a new window), France, and falls under the auspices of the AMSTAR ​programme. AMSTAR is a RadioNet (link opens in a new window) Joint Research Activity funded by the European Union Fram​ework 6 (link opens in a new window) programme.

equipment  graph

For more information please contact: RAL Space Enquiries

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