Delegate Survey
Studying dwarf galaxies as cosmic delegates to understand galaxy formation and evolution in Local Group analogues, using spectroscopy to examine how satellite systems form during galactic mergers.
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Research Projects
Research spanning galaxy surveys, groups, high-z evolution, angular momentum, star clusters, and black holes.
SAMI Galaxy Survey
Sydney Australian Astronomical Observatory Multi-object Integral Field Spectrograph (SAMI) an instrument at the Anglo-Australian Telescope. The SAMI survey has mapped spatially-resolved spectra of over 3000 galaxies.
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Hector Galaxy Survey
The Hector Galaxy Survey uses the revolutionary new Hector instrument to conduct integral field spectroscopy of 15,000 galaxies, mapping their star formation and chemical evolution.
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The MAGPI Survey
The Multi-Unit Spectroscopic Explorer (MUSE) Advanced Galaxy Properties Investigation surveys intermediate-redshift galaxies to understand how they evolve.
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AGEL Survey
ASTRO 3D Galaxy Evolution with Lenses - confirming and studying strong gravitational lenses to facilitate galaxy evolution and cosmology research.
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Choirs, HI Galaxy Groups
Choirs are a type of gas-rich galaxy group, found in the Survey for Ionization in Neutral Gas Galaxies, that contain multiple star-forming galaxies.
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Chemical Abundance
Investigating the chemical composition of galaxies using the SAMI instrument.
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Angular Momentum Studies
Investigating the role of angular momentum in galaxy formation and evolution, from high-redshift clumpy galaxies to present-day spirals and ellipticals.
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Galaxy Morphology Evolution
How do the compact, massive galaxies at high redshift become today's giant ellipticals? Understanding morphological transformation across cosmic time.
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Star Clusters & Black Holes
Investigating the connection between stellar clusters, central massive objects, and galaxy evolution through multi-wavelength observations and theoretical modelling.
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