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the optical-to-radio wavelength range, from major surveys and space telescopes (e.g: Gaia, SDSS, JWST, Hubble, Roman, Rubin-LSST). These are analysed using advanced machine learning and data-driven methods. My
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I supervise projects in particle physics. My main emphasis is on phenomenology, comparison of predictions with experimental measurements. I follow developments in flavour physics: weak decays
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PhD Scholarship for Designing Dignity: Civic equity through public bathroom architecture Job No.: 692149 Location: Caulfield campus Employment Type: Full-time Duration: 3.5-year fixed-term
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Expressions of Interest for PhD Scholarships at SMaRT-Pack Job No.: 690308 Location: Clayton campus Employment Type: Full-time Duration: 3.5 years fixed-term appointment Renumeration: 41,555 in line
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PhD Scholarship in Vaccine Adjuvant Discovery Job No.: 690645 Location: Clayton campus Employment Type: Full-time Duration: 3.5-year fixed-term appointment Remuneration: The successful applicant
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, spectroscopy, astrometry) using massive optical telescopes on Earth and in space (e.g., Hubble, Gaia, JWST, Kepler, TESS). My group develops cutting-edge models to extract the most from noisy data and to better
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for probing the atomic world. Co- supervisors are typically collaborators from within the Physics of Imaging group. Example project areas are: Developing ways to image atoms in space, energy and time Designing