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Linkage Infrastructure, Equipment And Facilities - Grant ID: LE120100181
Funder
Australian Research Council
Funding Amount
$650,000.00
Summary
Strengthening merit-based access and support at the new National Computing Infrastructure petascale supercomputing facility. World-leading high-performance computing is fundamental to Australia's international research success. This facility will provide access to the new National Computational Infrastructure facility by world-leading researchers from six research universities, and sustain ground-breaking work in an increasingly competitive environment.
“Beacons in the Night” unveiling how galaxies light up dark matter. How dark matter influences the formation and evolution of galaxies is to this day an outstanding question in astrophysics. To answer it, world-class facilities and a unique combination of observations and theory are required. This DP team, a world-class team of observers and theorists, will tackle this question by leveraging on two multi-million dollar projects: the MAGPI galaxy survey and the hydrodynamical simulations suite EA ....“Beacons in the Night” unveiling how galaxies light up dark matter. How dark matter influences the formation and evolution of galaxies is to this day an outstanding question in astrophysics. To answer it, world-class facilities and a unique combination of observations and theory are required. This DP team, a world-class team of observers and theorists, will tackle this question by leveraging on two multi-million dollar projects: the MAGPI galaxy survey and the hydrodynamical simulations suite EAGLE-XL. MAGPI will deliver exquisite kinematics for hundreds of galaxies in the middle ages of the Universe, providing a view to the effect of dark matter on galaxies at this critical time, while EAGLE-XL represents the technological frontier in simulations and provides the best interpretative framework for MAGPI.Read moreRead less
Rarefied hypervelocity separated flow in the transitional to continuum regimes. The transition regime for low-density flows is a no-man's-land between free-molecular and continuum flow, where the flow behaves differently to the assumptions typically used for modelling either flow type. Bird's direct Simulation Monte Carlo (DSMC) method is typically thought to be the best way of modelling these flows, but has not produced excellent agreement with previous experiments on low-density separated flow ....Rarefied hypervelocity separated flow in the transitional to continuum regimes. The transition regime for low-density flows is a no-man's-land between free-molecular and continuum flow, where the flow behaves differently to the assumptions typically used for modelling either flow type. Bird's direct Simulation Monte Carlo (DSMC) method is typically thought to be the best way of modelling these flows, but has not produced excellent agreement with previous experiments on low-density separated flows, due to computational limitations and lack of knowledge of the flow's internal energy. This proposal is a blind test of the best current DSMC codes against our experiments and a hypersonic continuum code, with the full internal energy state of the flow experimentally quantified for the first time.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE140100013
Funder
Australian Research Council
Funding Amount
$300,000.00
Summary
A sensitive tip-tilt wave-front sensor for the multi-conjugate adaptive-optics system on the Gemini south telescope. A sensitive tip-tilt wavefront sensor for the multi-conjugate adaptive-optics system on the Gemini South telescope: This project will construct a sensitive tip-tilt wavefront sensor for GeMS, the multi-conjugate adaptive-optics system on the Gemini South telescope in Chile. GeMS is a unique and revolutionary new system that delivers near-infrared images at similar resolution to th ....A sensitive tip-tilt wave-front sensor for the multi-conjugate adaptive-optics system on the Gemini south telescope. A sensitive tip-tilt wavefront sensor for the multi-conjugate adaptive-optics system on the Gemini South telescope: This project will construct a sensitive tip-tilt wavefront sensor for GeMS, the multi-conjugate adaptive-optics system on the Gemini South telescope in Chile. GeMS is a unique and revolutionary new system that delivers near-infrared images at similar resolution to the Hubble Space Telescope at optical wavelengths over wide fields. With this improvement in technology it will be possible to do this on much fainter objects than is currently possible using this new wave-front sensor. This will allow GeMS to routinely study the morphologies of external galaxies at high angular resolution - greatly extending its science scope. Sharper images will also be obtained for all objects that are currently accessible, leading to higher quality science data.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE170100004
Funder
Australian Research Council
Funding Amount
$502,453.00
Summary
Semiconductor laser for adaptive optics in astronomy and space awareness. This project aims to create a laser system for use as a laser guide star. Semiconductor laser technology is a cost effective, highly reliable and compact alternative to expensive, inefficient, bulky laser systems. This laser has wide scientific appeal for research with telescopes in astronomy, and for satellite tracking and mitigation of the threat of space debris. Producing a sodium laser guide star in Australia is expect ....Semiconductor laser for adaptive optics in astronomy and space awareness. This project aims to create a laser system for use as a laser guide star. Semiconductor laser technology is a cost effective, highly reliable and compact alternative to expensive, inefficient, bulky laser systems. This laser has wide scientific appeal for research with telescopes in astronomy, and for satellite tracking and mitigation of the threat of space debris. Producing a sodium laser guide star in Australia is expected to secure the country's position as the premier provider of commercial-grade laser guide star adaptive optics systems for civil and defence telescopes around the world.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE200100012
Funder
Australian Research Council
Funding Amount
$632,000.00
Summary
Exploring the Dynamic Universe with DREAMS. DREAMS is a revolutionary wide-field infrared surveyor designed to allow astronomers to unlock new science and foster international collaborations focused on important but elusive, infrared transient cosmic phenomena. Continually scanning the southern sky, DREAMS will provide “real time” data that will transform the depth and quality of astronomical observation. Combining off-the-shelf parts with scientific expertise from around the world, this telesco ....Exploring the Dynamic Universe with DREAMS. DREAMS is a revolutionary wide-field infrared surveyor designed to allow astronomers to unlock new science and foster international collaborations focused on important but elusive, infrared transient cosmic phenomena. Continually scanning the southern sky, DREAMS will provide “real time” data that will transform the depth and quality of astronomical observation. Combining off-the-shelf parts with scientific expertise from around the world, this telescope will help answer questions that are both practical and profound. DREAMS is an important component of a longer-term international strategy that will reinforce Australia’s global leadership in the realm of Infrared Transient Astronomy.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE130100198
Funder
Australian Research Council
Funding Amount
$315,000.00
Summary
The SAMI facility: a revolutionary multi-object hexabundle spectrograph. SAMI is a new Australian instrument concept that uses fibre bundles to obtain detailed spectroscopic data at many positions across the face of numerous galaxies at a time. Now that the technology has been shown to work, with spectacular results, the project aims to turn this concept into a general-user facility at the Anglo-Australian Telescope.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE210100156
Funder
Australian Research Council
Funding Amount
$289,500.00
Summary
3D Two-Photon Nanoprinter for Advanced Multi-Functional Materials & Devices. The Nanoscribe Photonic Professional GT2 Two-Photon 3D Printer enables tailoring materials’ architecture at nanoscale. This results in unique optical, mechanical, electrical, chemical, biochemical, and acoustic properties enabling a wealth of cutting-edge research activities in variety of fields including mechanical/optical/electrical metamaterials, bioinspired hard/soft materials, biomaterials (e.g., structured cell-ti ....3D Two-Photon Nanoprinter for Advanced Multi-Functional Materials & Devices. The Nanoscribe Photonic Professional GT2 Two-Photon 3D Printer enables tailoring materials’ architecture at nanoscale. This results in unique optical, mechanical, electrical, chemical, biochemical, and acoustic properties enabling a wealth of cutting-edge research activities in variety of fields including mechanical/optical/electrical metamaterials, bioinspired hard/soft materials, biomaterials (e.g., structured cell-tissue interfaces), biomedical devices (implantable devices and drug-delivery systems), nanofluidics, and photonic crystals. In each of these fields, we will use GT2 to print variety of polymers, hydrogels, metals and ceramics, for example by printing polymer-derived nanoceramics that will be simultaneously strong and tough.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE210100015
Funder
Australian Research Council
Funding Amount
$1,680,000.00
Summary
The Cherenkov Telescope Array - From Production towards Operation. The Cherenkov Telescope Array is a transformational facility in very-high-energy gamma-ray astronomy. It will be 10 times more sensitive than current instruments and will revolutionise many topics in high energy astrophysics, and in astro-particle physics such as dark matter. Over 1000 scientists from over 30 countries are involved and the first telescopes on the southern hemisphere site in Chile will be installed from about 2021 ....The Cherenkov Telescope Array - From Production towards Operation. The Cherenkov Telescope Array is a transformational facility in very-high-energy gamma-ray astronomy. It will be 10 times more sensitive than current instruments and will revolutionise many topics in high energy astrophysics, and in astro-particle physics such as dark matter. Over 1000 scientists from over 30 countries are involved and the first telescopes on the southern hemisphere site in Chile will be installed from about 2021. This project will ensure Australia's contribution to complete the facility, leading into its operations phase (starting in 2027). It will also fund unique optical astronomy hardware that will enable Australian scientific leadership in supporting some of the Cherenkov Telescope Array's Key Science Projects.
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Linkage Infrastructure, Equipment And Facilities - Grant ID: LE170100118
Funder
Australian Research Council
Funding Amount
$1,800,000.00
Summary
UltraTEM: Resolving the structure of matter in space, energy and time. This project aims to establish a transmission electron microscope facility to analyse materials structure at the atomic level. A small number of atoms in critical locations governs the properties of materials from solar cells and catalysts to aerospace alloys, bio-sensors and quantum computers. To understand and engineer matter at this atomic level, tools are needed to characterise these critical atoms. This open access, nati ....UltraTEM: Resolving the structure of matter in space, energy and time. This project aims to establish a transmission electron microscope facility to analyse materials structure at the atomic level. A small number of atoms in critical locations governs the properties of materials from solar cells and catalysts to aerospace alloys, bio-sensors and quantum computers. To understand and engineer matter at this atomic level, tools are needed to characterise these critical atoms. This open access, national facility will be able to characterise matter at the atomic-level. Expected outcomes include better understanding of the natural world and advanced materials to solve problems in energy, technology, health, environment, communications, advanced manufacturing, transport and security.Read moreRead less