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
Development of Optical Clocks and Their Applications to Precision Frequency Measurements and Time Keeping. The goal of the proposed international researcher exchange program is to enhance the ongoing collaboration between the Frequency Standards and Metrology (FSM) Group at the University of Western Australia and leading US research institutions, including National Institute of Standards and Technology (NIST) in the field of (i) laser cooled atomic frequency standards, (ii) methods of optical ....Development of Optical Clocks and Their Applications to Precision Frequency Measurements and Time Keeping. The goal of the proposed international researcher exchange program is to enhance the ongoing collaboration between the Frequency Standards and Metrology (FSM) Group at the University of Western Australia and leading US research institutions, including National Institute of Standards and Technology (NIST) in the field of (i) laser cooled atomic frequency standards, (ii) methods of optical frequency synthesis and coherent time transfer between widely separated parts of electromagnetic spectrum and (iii) generation of low noise microwave signals directly from frequency stabilised ultra-fast pulsed lasers.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
Entanglement renormalization: a new route to strongly correlated fermions and novel states of matter in two dimensions. The expected outcome of the research program is a significant boost in our understanding of strongly correlated fermion systems, which will reinforce Australia's competitiveness and international profile in aspects of breakthrough science and frontier technologies. By strengthening both the underpinning theory and innovative computational tools to study fermion systems, and by ....Entanglement renormalization: a new route to strongly correlated fermions and novel states of matter in two dimensions. The expected outcome of the research program is a significant boost in our understanding of strongly correlated fermion systems, which will reinforce Australia's competitiveness and international profile in aspects of breakthrough science and frontier technologies. By strengthening both the underpinning theory and innovative computational tools to study fermion systems, and by applying them to specific problems of recognized importance, this program will have direct implications in condensed matter physics and will exert significant influence in areas such as quantum chemistry, particle, nuclear and atomic physics, quantum computing, quantum atom optics and nanotechnology.Read moreRead less