Dunlap Institute announces new director, astronomer Prof. Bryan Gaensler
June 11, 2014
TORONTO, ON – After an international search, the Dunlap Institute for Astronomy & Astrophysics, University of Toronto, announces the appointment of its new director, Prof. Bryan Gaensler, a leading international researcher in cosmic magnetism, supernova explosions and interstellar gas.
Gaensler comes to the Dunlap Institute from the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO) where he is the founding director. He is also an Australian Laureate Fellow at the Sydney Institute for Astronomy within the School of Physics at The University of Sydney.
“I am thrilled to be taking up the directorship,” says Gaensler. “The Dunlap is an institute with unique capacities and enormous potential. I’m excited by the prospect of developing new and innovative approaches to instrumentation, and combining this with the University of Toronto’s already impressive credentials in astronomy and astrophysics.”
For the past decade, Gaensler has made significant contributions to building long-term research capacity for observational astronomy. Much of that effort has been in the development and planning of the Square Kilometre Array which, when completed in twin locations in South Africa and Australia, will be the largest radio telescope ever built and will help answer questions about the very early Universe and how it evolved into the cosmos we see today.
“I want to understand why the Universe is magnetic,” says Gaensler, “and I aim to use explosions, flashes and flares throughout the cosmos as a unique probe of fundamental physics. The Dunlap Institute is the ideal environment for me to pursue these programs, because of its focus on groundbreaking instrumentation and on unique ways of studying the sky. I look forward to the chance to begin working with Toronto students on these projects.”
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For more information:
Dunlap Institute for Astronomy & Astrophysics
UNIVERSITY OF TORONTO
50 St. George Street
Toronto, ON M5S 3H4