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program, aiming to reprogram DMG biology and improve immunotherapy responsiveness. The overarching goal is to define how cell lineage, differentiation, and antigen presentation intersect to create
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My research focuses on the dramatic final stages of massive stars, exploring how they end their lives as gamma-ray bursts, supernovae, and kilonovae. To unravel these mysteries, I employ a combination of multi-wavelength observational data with sophisticated simulations. I am a member of various...
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I am an ARC Future (former DECRA) Fellow and lead the Structured Nanophotonics Group at Monash University. My research in nanophotonics explores the full potential and multi-dimensional nature of light, focusing on controlled light-matter interactions at the nanoscale. Driven by the fascinating...
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will be required to enrol in a Curtin University Doctoral program on a full-time basis for 4-years. Student type Future Students Faculties and centres Faculty of Business and Law Course type Higher
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also not be in receipt of any other scholarship. Essential: English language IELTS level of 7 and above Essential: Successful completion of an Honours or Masters programme with a research component (or
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in evidence synthesis methodology research, research methods, and experience in conducting systematic reviews Knowledge of software innovations to support the conduct of systematic reviews and ability
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The successful candidate must meet the minimum academic entry requirement for admission into the Doctor of Philosophy program https://research.curtin.edu.au/postgraduate/ including the English proficiency levels
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https://www.curtin.edu.au/study/offering/course-research-doctor-of-philosophy---civil-engineering--dr-cvengrv1/ Eligibility criteria For both domestic and international students. Minimum requirement
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I supervise projects considering the evolution of accretion discs and their connection to observations. In particular, I consider discs that are warped or distorted (not flat). This geometry has been directly observed in planet forming discs around young stars (protoplanetary discs) and is...
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, which are some of the most numerous stars in the Universe. "Weighing stars using stellar vibrations: Asteroseismic masses of Red Giant Stars using space telescope data" "Using optical telescope