The CASS Engineering Front End Group
Led by Mark Bowen, this group is composed of engineers and technicians that, as a group, has the capabilities to design and construct both room temperature and cryogenic radioastronomy front ends. The CASS workshop staff contribute the essential skills and specialised expertise to make the technical staff's designs a reality. High precision machining of large and small scale structures using both computer controlled and manually operated machines is complemented by more conventional 'hands on' precision craftsmanship including sheet metal work and all forms of welding/brazing.
The Front End Group's expertise lies principally in the areas of passive microwave devices, InP MMICs , HEMT LNAs, cryogenics, signal frequency and IF frequency processing (microstrip circuits), control and monitor electronics, 3D EM modelling, assembly of RF and DC electronics including clean room techniques, PCB assembly, cryogenics (design, systems, servicing), metal surface treatment (cleaning, anodising, high precision plating) and quasioptic design.
Front ends are constructed for ATNF antennas as well as overseas observatories. The Arecibo Observatory has benefitted from the 7 beam receiver designed and fabricated by the CASS Front End Group and shown here.
An upgrade in 2007/2008 completed a program to equip the Compact Array antennas with the latest in millimetre wave technology. This 7mm Upgrade project enabled the already operational 3mm / 12mm receivers to have 7mm capability. In frequency terms, a 30-50GHz capability has been added to the single package that is already capable of observations at 18-26GHz and 85-105GHz.
Parkes is benefitting from a new 22 GHz receiver.
Current major projects include: