Future Students
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Click here for potential PhD, Honours, and SAO projects in Astrophysics
Current PhD Students
Astrophysics
Glen Rees, Macquarie University, EMU Cosmology
Co-supervisors: David Bacon, Lee Spitler
Jordan Collier, University of Western Sydney, The History of Supermassive Black Holes in the Universe
Co-supervisor: Miroslav Filipovic
Andrew O’Brien, University of Western Sydney, The ATLAS-SPT Survey
Co-supervisor: Nick Tothill
Andreas Herzog, University of Bochum & Macquarie University, Infrared-Faint Radio Sources
Co-supervisors: Enno Middelberg & Lee Spitler
Alessandro Maini, University of Bologna & Macquarie University, Infrared-Faint Radio Sources
Co-supervisors: Isabella Prandoni & Lee Spitler
Francesco Cavallaro, University of Catania, SCORPIO project
Co-supervisors: Grazia Umana and Corrado Trigilio
Aboriginal Astronomy
Bob Fuller, Macquarie University, Australian Aboriginal Astronomy
Co-supervisor: Michelle Trudgett
John South, UWS, Australian Aboriginal Astronomy
Co-supervisor: Nick Tothill
Previous PhD students
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Alan Roy, Sydney Uni., 1989-94, Active Galaxies
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Simon Ellingsen, Uni. Tasmania, 1992-95, Methanol masers
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Richard Gooch, Macquarie Uni., 1992-1999, Visualisation of astronomical data
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Chris Phillips, Uni. Tasmania, 1994-1998 , Methanol masers
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Mark Bransford, Iowa State Uni., 1994-1999, The Seyfert-Starburst Connection
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David Rayner, Uni. Tasmania, 1996-2000, Circular Polarisation of extragalactic radio sources
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Minh Huynh, ANU, 2000-2005, Constraining the Star Formation History of the Universe with Deep Radio Data
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Minnie Mao, University of Tasmania, 2009-2012, Cosmic Evolution of Radio AGNs
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Kate Randall, University of Sydney, 2009-2012, Cosmic Evolution of Star-forming Radio Sources
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Chris Hales, University of Sydney, 2009-2012, Radio Polarisation and the Origin of the Cosmic Magnetic Field
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Duane Hamacher, Macquarie University, 2010-2012, Australian Aboriginal Astronomy
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Peter-Christian Zinn, University of Bochum, 2010-2013, New avenues in galaxy evolution studies: large-scale magnetic fields and properties of high-redshift radio emitters
Last updated by Ray Norris 20 March 2015