Phased array feed (PAF) receivers are being developed to provide dishes with a wide field of view for
the next generation of radiotelescopes, such as the Australian Square Kilometre Array Pathfinder
(ASKAP). These systems are not only very complex to design and build but they also present new
challenges in characterization and operation. To study FPAs systems, a prototype interferometerradiotelescope
was built at the CSIRO Radiophysics Laboratory in Sydney. This talk will discuss
the beamforming and evaluation methods employed on this system the subject of Doug’s recently
completed PhD co-supervised by Peter Hall.
Doug will also be more than happy to field questions about ASKAP and PAFs in general.
Biography:
Doug Hayman graduated with a Bachelor of Science (1985) and Bachelor of Engineering (1987) from Sydney University. He then
spent three years working on the development, manufacture, testing and repair of FM broadcast transmitters and UHF Studio to
Transmitter Links. He then moved to AUSSAT, now Optus, and for two years worked on project managing reconfiguring earth
stations, commissioning testing as well as circuit level supervisory and control system design.
Since 1992 he has been with CSIRO. He worked on antenna metrology and led a comprehensive upgrade of CSIRO’s antenna measurement
facility hardware and software. He also designed components such as waveguide rotary joints and orthomode transducers and
managed a number of antenna related projects.
Since 2003, he has been involved in the development and testing of focal plane arrays for radio astronomy. He recently completed a
PhD in the field, titled Beamforming and evaluation of focal plane arrays for radio astronomy. He is now working on a calibration
system for the Australian Square Kilometre Array Pathfinder (ASKAP) project and commissioning the telescope. His interests are in
antenna measurement techniques, particularly noise performance, phased array feeds and antenna theory and design.
Refreshments will be served following the seminar