Tara Murphy is a Professor in physics at the University of Sydney. Her area of research is radio astronomy, and in particular radio transients. Her team played a key role in the detection of radio emission from the first neutron star merger detected by LIGO, GW170817.
Tara is leading the VAST project: An ASKAP Survey for Variables and Slow Transients. This project is investigating astronomical objects that vary on rapid timescales. These objects act as a laboratory for studying extreme physics. VAST will allow us to answer questions about the formation of black holes, the missing mass in our Galaxy, and the origin of many exotic objects that burst and flicker in the distant universe. Tara is also working on transients surveys with the Murchison Widefield Array, a low frequency SKA pathfinder.
Experience
2019–present
Professor, University of Sydney
2016–2018
Associate professor, University of Sydney
2010–2015
Senior lecturer, University of Sydney
2006–2009
ARC Australian Postdoctoral Fellow, The University of Sydney
Education
2004
The University of Edinburgh, PhD (Astrophysics)
1999
The University of Sydney, Bachelor of Science (Advanced) (Honours)
Grants and Contracts
2019
Radio follow-up of gravitational wave events
Role:
Chief Investigator
Funding Source:
ARC Discovery Project
2016
The radio transient sky in real time
Role:
Chief Investigator
Funding Source:
ARC Future Fellow
2011
Extreme Events: Mining the Radio Sky for Gamma-ray Bursts with Intelligent Algorithms
Role:
Chief Investigator
Funding Source:
ARC Discovery Project
2010
New Dimensions in Radio Astronomy: Mining Sparse Datasets with the Australian SKA Pathfinder
Role:
Chief Investigator
Funding Source:
ARC Super Science
Research Areas
Astronomical And Space Sciences (0201)
Galactic Astronomy (020104)
Cosmology And Extragalactic Astronomy (020103)
Artificial Intelligence And Image Processing (0801)