Discovering the First Generation of Stars in the Galaxy - The Most Metal-Poor Stars. The most metal-poor stars carry a fossil record of the early chemical and dynamical evolution of the Galaxy. The most interesting objects are those with the lowest metal abundances representing the earliest generation of stars in the Galaxy. The aim of the present project is to extend the mining of the HES objective spectra to identify extremely metal-deficient giants, which together with the already identified ....Discovering the First Generation of Stars in the Galaxy - The Most Metal-Poor Stars. The most metal-poor stars carry a fossil record of the early chemical and dynamical evolution of the Galaxy. The most interesting objects are those with the lowest metal abundances representing the earliest generation of stars in the Galaxy. The aim of the present project is to extend the mining of the HES objective spectra to identify extremely metal-deficient giants, which together with the already identified dwarfs will be further distilled using 6dF and the DBS. We anticipate trebling the total number of the most metal deficient stars known and targeting these for observations with 8m telescopes.Read moreRead less
Star Formation at Millimetre Wavelengths with the CSIRO Australia Telescope. The newly-upgraded CSIRO Australia Telescope Compact Array, together with the CSIRO Mopra Telescope, provide a unique and powerful combination for studying the millimetre-wave emission from molecules and cold dust in star formation regions. We propose to combine the astrophysical expertise of UNSW with the instrumental expertise of CSIRO to use these instruments to study the processes of star formation. There are two pa ....Star Formation at Millimetre Wavelengths with the CSIRO Australia Telescope. The newly-upgraded CSIRO Australia Telescope Compact Array, together with the CSIRO Mopra Telescope, provide a unique and powerful combination for studying the millimetre-wave emission from molecules and cold dust in star formation regions. We propose to combine the astrophysical expertise of UNSW with the instrumental expertise of CSIRO to use these instruments to study the processes of star formation. There are two parallel themes to this research: to commission and develop optimal techniques for using the new instruments, and to make use of them to explore the poorly-understood processes that cause stars to form.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0347403
Funder
Australian Research Council
Funding Amount
$222,000.00
Summary
An ultra-wideband digital filterbank for the Mopra Radiotelescope. We seek funding to equip the Mopra radiotelescope with an ultra-wide-bandwidth digital filter bank. This will greatly improve the efficiency of the observatory, increasing the speed at which spectroscopic data is acquired by a factor of 8, and the speed of acquiring continuum data by a factor of 32. Once equipped in this way, Mopra, which is already the largest millimetre-wave radiotelescope in the southern hemisphere, will enjo ....An ultra-wideband digital filterbank for the Mopra Radiotelescope. We seek funding to equip the Mopra radiotelescope with an ultra-wide-bandwidth digital filter bank. This will greatly improve the efficiency of the observatory, increasing the speed at which spectroscopic data is acquired by a factor of 8, and the speed of acquiring continuum data by a factor of 32. Once equipped in this way, Mopra, which is already the largest millimetre-wave radiotelescope in the southern hemisphere, will enjoy an unbeatable edge over all other competing observatories around the world through its combination of collecting area and bandpass.Read moreRead less
Control of Instabilities in Advanced Gravitational Wave Detectors. Gravitational wave technology from UWA has already given rise to significant spin-offs including sapphire oscillators for radar applications and vibration isolators for airborne mineral exploration. This project will lead to techniques for increasing the sensitivity of already extraordinary sensitive instruments, and could have applications in many areas. The project will strengthen Australia's role in the world wide quest to det ....Control of Instabilities in Advanced Gravitational Wave Detectors. Gravitational wave technology from UWA has already given rise to significant spin-offs including sapphire oscillators for radar applications and vibration isolators for airborne mineral exploration. This project will lead to techniques for increasing the sensitivity of already extraordinary sensitive instruments, and could have applications in many areas. The project will strengthen Australia's role in the world wide quest to detect gravitational waves, which is one of the most significant and challenging human endeavours. The project will use the superb national research facility at Gingin. Its content contributes to the Eureka Prize winning Gravity Discovery Centre also located at the site, which is a major centre for science education.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0775523
Funder
Australian Research Council
Funding Amount
$223,000.00
Summary
A new field plate for the 6DF multi-object spectroscopy system on the Anglo-Australian Observatory's Schmidt telescope. Astronomy engages the public like no other science. This flagship project is Australian based, uses Australian technology and although international has a strong Australian flavour in scientific leadership and participation. The experiment will yield a massive leap forward in our understanding of our Milky Way Galaxy. Australia 'punches above its weight' in astronomy because ....A new field plate for the 6DF multi-object spectroscopy system on the Anglo-Australian Observatory's Schmidt telescope. Astronomy engages the public like no other science. This flagship project is Australian based, uses Australian technology and although international has a strong Australian flavour in scientific leadership and participation. The experiment will yield a massive leap forward in our understanding of our Milky Way Galaxy. Australia 'punches above its weight' in astronomy because of our innovation, ability to maximise limited resources and to cannily target projects with high return for the investment applied. The same rationale here is delivering excellent science. To secure this return into the second, most productive phase requires modest additional investment by Australia and our partners in the necessary project infrastructure.Read moreRead less
Global Gravitational Wave Astronomy. To listen to the universe with gravitational waves needs a global array of gravitational wave observatories, and one of these must be in the southern hemisphere - in Australia. By definitively answering outstanding questions about an Australian gravitational wave observatory - Where should it be? How sensitive? What astronomy will it aid? - we make the case for the international community to help build this observatory, investing hundreds of millions of dolla ....Global Gravitational Wave Astronomy. To listen to the universe with gravitational waves needs a global array of gravitational wave observatories, and one of these must be in the southern hemisphere - in Australia. By definitively answering outstanding questions about an Australian gravitational wave observatory - Where should it be? How sensitive? What astronomy will it aid? - we make the case for the international community to help build this observatory, investing hundreds of millions of dollars in rural Australia and keeping Australia on the cutting edge of all branches of astronomy. As a flagship client of advanced data GRID technologies, we will also shape the growth of Australian knowledge of, and infrastructure for, next-generation communications technologies.Read moreRead less
Pulsed oscillating mass analyser. Mass spectrometers are ubiquitous components in chemical analysis, but are often large and expensive. We have developed a new method for mass analysis, which is smaller and cheaper than existing technology. However, the analyser needs further research to determine whether it has the performance specifications to match the other technologies. The objective of this research is to characterise, explore and extend the prototype and to develop the appropriate math ....Pulsed oscillating mass analyser. Mass spectrometers are ubiquitous components in chemical analysis, but are often large and expensive. We have developed a new method for mass analysis, which is smaller and cheaper than existing technology. However, the analyser needs further research to determine whether it has the performance specifications to match the other technologies. The objective of this research is to characterise, explore and extend the prototype and to develop the appropriate mathematical algorithm for mass analysis. Success in this project may lead to a new mass analyser that can be incorporated into analytical instruments, many of which are manufactured in Australia.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0560672
Funder
Australian Research Council
Funding Amount
$202,705.00
Summary
Ultrafast laser facility for chemical, biological and physical investigations of advanced materials. Ultrafast laser techniques are becoming indispensable in many diverse scientific disciplines. Within the Australian scientific community, there is a great need for enhanced access to sophisticated ultrafast laser instrumentation. The expansion to the femtosecond laser facility through the addition of state-of-the-art laser devices, will enable novel laser spectroscopy measurements and advanced op ....Ultrafast laser facility for chemical, biological and physical investigations of advanced materials. Ultrafast laser techniques are becoming indispensable in many diverse scientific disciplines. Within the Australian scientific community, there is a great need for enhanced access to sophisticated ultrafast laser instrumentation. The expansion to the femtosecond laser facility through the addition of state-of-the-art laser devices, will enable novel laser spectroscopy measurements and advanced optical microscopy techniques to be applied to investigations of advanced materials and biological systems. Access to such instrumentation is crucial to fields including photoluminescent conductive polymers, nanoparticles, engineered supramolecules for artificial photosynthetic systems, and photoactivated therapy and drug delivery/release technology.Read moreRead less
WAVES IN THE MIDDLE ATMOSPHERE. Atmospheric waves have a profound influence in the atmosphere. A unique network of radars in the southern hemisphere will be used to study wave processes in the upper atmosphere. The project will investigate causes of wave variability, wave sources and wave-wave interactions and will involve satellite measurements and international collaboration. Results will guide the development and testing of schemes that incorporate the effects of small-scale waves in numerica ....WAVES IN THE MIDDLE ATMOSPHERE. Atmospheric waves have a profound influence in the atmosphere. A unique network of radars in the southern hemisphere will be used to study wave processes in the upper atmosphere. The project will investigate causes of wave variability, wave sources and wave-wave interactions and will involve satellite measurements and international collaboration. Results will guide the development and testing of schemes that incorporate the effects of small-scale waves in numerical weather and climate models. Outcomes from the project will have application in modelling climate change.Read moreRead less
Industrial-strength X-ray Phase Tomography. The unique 3D imaging capability provided as a result of this project will have application to advanced manufacturing as a non-destructive evaluation for materials and micro-components. For instance, the internal structure of aerogels, porous light metals, polymers and carbon fibre based materials can all be imaged at the microscale. Similar benefits flow in health sciences where organic processes can be observed in place and where, for instance, small ....Industrial-strength X-ray Phase Tomography. The unique 3D imaging capability provided as a result of this project will have application to advanced manufacturing as a non-destructive evaluation for materials and micro-components. For instance, the internal structure of aerogels, porous light metals, polymers and carbon fibre based materials can all be imaged at the microscale. Similar benefits flow in health sciences where organic processes can be observed in place and where, for instance, small animals used in research and clinical testing can be inspected internally without having to destroy them, thus allowing for repeated measurements.Read moreRead less