Neutral hydrogen and galaxy assembly in the distant Universe. This research will produce a snapshot of hydrogen gas in the Universe 6-7 billion years ago. These results, together with galaxy formation models, will tell us how galaxies are assembled to make the beautiful spirals we see today. This project is only possible because of rapid advances in programmable chip technology, part of the massive increase in the speed and complexity of integrated circuit devices.
Our Galaxy: the last hundred million years. Star formation and evolution are the fundamental processes which energize a galaxy and recycle the interstellar medium. In our Galaxy, we have the opportunity to study these processes in great detail. This project uses sensitive radio continuum images from the Molonglo Observatory Synthesis Telescope to discover how this energizing and enrichment occurs. We will use innovative machine learning techniques to identify a potentially new population of Gala ....Our Galaxy: the last hundred million years. Star formation and evolution are the fundamental processes which energize a galaxy and recycle the interstellar medium. In our Galaxy, we have the opportunity to study these processes in great detail. This project uses sensitive radio continuum images from the Molonglo Observatory Synthesis Telescope to discover how this energizing and enrichment occurs. We will use innovative machine learning techniques to identify a potentially new population of Galactic sources and to patrol a new domain in source variability.Read moreRead less
Improving optical data storage and micromachining technology through better modelling and characterisation of their laser beams. The laser sources generally do not have simple (Gaussian) distributions. The applicant has recently developed a model, describing free propagation of complex (non-Gaussian) laser beams. This project seeks to develop a comprehending model for laser beams propagation through complex optical systems. The effects of various optical elements will be defined employing a no ....Improving optical data storage and micromachining technology through better modelling and characterisation of their laser beams. The laser sources generally do not have simple (Gaussian) distributions. The applicant has recently developed a model, describing free propagation of complex (non-Gaussian) laser beams. This project seeks to develop a comprehending model for laser beams propagation through complex optical systems. The effects of various optical elements will be defined employing a novel method known as SAFE (Stable Aggregate of Flexible Elements) which is a compromise between geometrical and physical optics. Applying this model to micromachining and optical data storage (ODS), which need high beam quality (low divergence and good focussibility), enable accurate predictive capability critical to the optimisation of micromachining and ODS designs.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0238884
Funder
Australian Research Council
Funding Amount
$220,000.00
Summary
Development of the CANGAROO III Very High Energy Gamma-ray telescope. This international project will explore the only part of the electromagnetic spectrum yet to be subjected to detailed astronomical study. CANGAROO III will span the energy range from ~100GeV to >10TeV, expanding upwards the range of satellite observations, and downwards the range accessible from previous ground-based systems. Gamma-ray observations have opened a new window on the universe and it is clear that there is much to ....Development of the CANGAROO III Very High Energy Gamma-ray telescope. This international project will explore the only part of the electromagnetic spectrum yet to be subjected to detailed astronomical study. CANGAROO III will span the energy range from ~100GeV to >10TeV, expanding upwards the range of satellite observations, and downwards the range accessible from previous ground-based systems. Gamma-ray observations have opened a new window on the universe and it is clear that there is much to be discovered with this new instrument. This project will provide an Australian infrastructure contribution to support the multi-million dollar contribution of our Japanese partners, and thus provide Australian access to a key astrophysical field at very modest cost.Read moreRead less
Electrodynamics of magnetic explosions in astrophysics. The project aims to develop a new model for solar flares and pulsars that more realistically describes these phenomena. Solar flares and pulsars involve strong magnetic fields changing rapidly as a function of time, implying enormous inductive potentials. The project aims to show how the inductive field and the plasma response to it can be included in an electrodynamic theory. It plans to apply this theory to solar flares, and show how it c ....Electrodynamics of magnetic explosions in astrophysics. The project aims to develop a new model for solar flares and pulsars that more realistically describes these phenomena. Solar flares and pulsars involve strong magnetic fields changing rapidly as a function of time, implying enormous inductive potentials. The project aims to show how the inductive field and the plasma response to it can be included in an electrodynamic theory. It plans to apply this theory to solar flares, and show how it can resolve the long-standing ‘number problem’. It also plans to apply the model to pulsars, and show how the long-standing dichotomy between the vacuum-dipole and rotating-magnetosphere models can be resolved by synthesising them. The project intends to combine these ideas into a new model for the most extreme examples of magnetic explosions: superflares and giant bursts on magnetars.Read moreRead less
Magnetic skeletons, solar flares, and space weather. This project aims to investigate how magnetic reconnection occurs during solar flares through accurate reconstruction of coronal magnetic fields from solar data before and after flares, and by reliable determination of field skeletons. Solar flares are dynamic events in the Sun's corona which cause local space weather storms. Magnetic reconnection is the accepted mechanism for flares but conventional models neglect the three-dimensional (3D) n ....Magnetic skeletons, solar flares, and space weather. This project aims to investigate how magnetic reconnection occurs during solar flares through accurate reconstruction of coronal magnetic fields from solar data before and after flares, and by reliable determination of field skeletons. Solar flares are dynamic events in the Sun's corona which cause local space weather storms. Magnetic reconnection is the accepted mechanism for flares but conventional models neglect the three-dimensional (3D) nature of the process. The project will improve 3D reconnection models for flares, and advance the ability to predict large events and hence space weather storms.Read moreRead less
Mechanism Of Anoxic Iron Acquisition In Pathogenic Bacteria
Funder
National Health and Medical Research Council
Funding Amount
$536,280.00
Summary
All organisms require iron for their survival, including all bacterial species. Bacterial pathogens growing in anaerobic environments, such as in our gut, gum, or tissue, sequester iron through the divalent iron transporter FeoB. We aim to divulge the mechanism of iron transport through FeoB by structural and functional studies, and thus provide a scaffold for a non-conventional antimicrobial target.
The Dawn of Extreme Gamma Ray Astronomy. This project aims to reveal the highest energy cosmic-ray particles in our galaxy, produced in extreme and still unknown astrophysical processes. Their interaction with nuclei in space produces the highest energy gamma ray light. Our project will make use of this extreme gamma ray light with upgraded and next-generation gamma-ray telescope arrays. With accompanying data from Australian radio telescopes, and computer models of the cosmic ray interactions, ....The Dawn of Extreme Gamma Ray Astronomy. This project aims to reveal the highest energy cosmic-ray particles in our galaxy, produced in extreme and still unknown astrophysical processes. Their interaction with nuclei in space produces the highest energy gamma ray light. Our project will make use of this extreme gamma ray light with upgraded and next-generation gamma-ray telescope arrays. With accompanying data from Australian radio telescopes, and computer models of the cosmic ray interactions, our project can finally determine from where these cosmic rays originate, yielding insight into our galaxy's evolution. Complex machine learning methods will be needed in a project that provides a world-leading student training ground, motivated by a century old mystery in astronomy.Read moreRead less
Characterising The Beta-catenin Nuclear Targeting Pathway In Cancer
Funder
National Health and Medical Research Council
Funding Amount
$485,081.00
Summary
Bowel cancer is caused by inherited gene mutations that cause build-up of beta-catenin protein in the cell nucleus. Bowel cancer is the second largest cause of cancer deaths in Australia. We aim to study the mechanisms controlling beta-catenin accumulation in the nucleus. We will characterise new signalling pathways that control movement and activity of beta-catenin in the nucleus. This will yield insights into the role of beta-catenin in cancer and possible targets for therapy.
The Carina Nebula: a massive star factory and the anchor for calibrating extragalactic star formation. Massive stars are vital to the life cycle of a galaxy, providing material and controlling the environment where new stars are made. This project will use the Australia Telescope to map the spectacular Carina Nebula, a hotbed of massive stars, to provide a picture of its stars and gas and a template for understanding star formation in distant galaxies.