The 6dF Galaxy Survey - Mass and Motions in the Nearby Universe. The 6dF Galaxy Survey will yield by far the largest and most detailed map of the positions and motions of galaxies in the nearby universe. The goal of the survey is to determine the distributions of both the galaxies and the dark matter in order to measure fundamental cosmological parameters and constrain models of galaxy formation. The survey will cover the whole southern hemisphere, measuring redshifts for 120,000 galaxies and di ....The 6dF Galaxy Survey - Mass and Motions in the Nearby Universe. The 6dF Galaxy Survey will yield by far the largest and most detailed map of the positions and motions of galaxies in the nearby universe. The goal of the survey is to determine the distributions of both the galaxies and the dark matter in order to measure fundamental cosmological parameters and constrain models of galaxy formation. The survey will cover the whole southern hemisphere, measuring redshifts for 120,000 galaxies and distances and motions for 15,000 galaxies. The survey will use the unique 6dF robotic fibre spectrograph we have constructed for the Anglo-Australian Observatory's Schmidt Telescope.Read moreRead less
A study of vocal tract resonances in the singing voice to develop tools for teaching singing. The voice is our oldest and most widely used musical instrument, but it is incompletely understood because of the difficulty of studying the vocal tract precisely during singing. We shall determine the main techniques used by singers to control and to adapt the acoustic resonances of their vocal tracts. This advance in understanding will enhance Australia's scientific reputation in an area of wide publi ....A study of vocal tract resonances in the singing voice to develop tools for teaching singing. The voice is our oldest and most widely used musical instrument, but it is incompletely understood because of the difficulty of studying the vocal tract precisely during singing. We shall determine the main techniques used by singers to control and to adapt the acoustic resonances of their vocal tracts. This advance in understanding will enhance Australia's scientific reputation in an area of wide public interest. Further, when combined with developments of our novel techniques to operate in real time, it will provide a new tool for students of singing to adjust their resonances and prevent damage to the vocal tract. We shall publish our work not only in the top scientific journals, but also on our popular, multi-award winning web site.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0882778
Funder
Australian Research Council
Funding Amount
$201,224.00
Summary
Water vapour radiometers for millimetre-wave phase correction for the Australia Telescope. Australia has a tradition of excellence in astronomy. Inspired by wonder about the cosmos, it stimulates public interest in science, so leading to the training of highly skilled graduates. In turn, this drives the development of technologies needed to pursue the science. The nation has invested in the technology for millimetre-wave astronomy, building the first interferometer in our hemisphere. This equipm ....Water vapour radiometers for millimetre-wave phase correction for the Australia Telescope. Australia has a tradition of excellence in astronomy. Inspired by wonder about the cosmos, it stimulates public interest in science, so leading to the training of highly skilled graduates. In turn, this drives the development of technologies needed to pursue the science. The nation has invested in the technology for millimetre-wave astronomy, building the first interferometer in our hemisphere. This equipment will capitalise on this investment, extending the capabilities of the Australia Telescope to maintain it as a front line instrument, attracting the best scientists here to use it. This will help nurture a vigorous radio-science community, one able to actively participate in the billion-dollar investment being made internationally in the field.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0775602
Funder
Australian Research Council
Funding Amount
$100,000.00
Summary
A ground station for the NANTEN2 sub-millimetre wave telescope. Australia has a tradition of excellence in astronomy. Inspired by our natural wonder about the cosmos, it helps stimulate public interest in science, so leading to the training of highly skilled graduates. This in turn drives development of technologies needed to pursue the science. The nation has invested in technology for millimetre-wave astronomy, building the first interferometer in our hemisphere. We aim to capitalise on this i ....A ground station for the NANTEN2 sub-millimetre wave telescope. Australia has a tradition of excellence in astronomy. Inspired by our natural wonder about the cosmos, it helps stimulate public interest in science, so leading to the training of highly skilled graduates. This in turn drives development of technologies needed to pursue the science. The nation has invested in technology for millimetre-wave astronomy, building the first interferometer in our hemisphere. We aim to capitalise on this investment, leveraging it to access a frontline facility under construction on the Atacama plateau in Chile. This will help nurture a vigorous radio-science community, one able to actively participate in the billion-dollar investment being made by the international community in astronomical facilities there.Read moreRead less
The birth of massive stars. Australia has an international reputation for the quality of its astronomy. This in turn stimulates public interest in science, and helps drive the development of technologies needed to pursue it. Over the past decade our nation has invested in the technology for millimetre-wave astronomy, building competitive instrumentation and the first interferometer in our hemisphere. We aim to capitalise on this investment, leveraging it to access frontline facilities in Chile b ....The birth of massive stars. Australia has an international reputation for the quality of its astronomy. This in turn stimulates public interest in science, and helps drive the development of technologies needed to pursue it. Over the past decade our nation has invested in the technology for millimetre-wave astronomy, building competitive instrumentation and the first interferometer in our hemisphere. We aim to capitalise on this investment, leveraging it to access frontline facilities in Chile being built by our international partners. In doing so, we will expose our students to the leading-edge and help nurture a vigorous radio science community, one able to actively participate in the billion-dollar international ALMA radio-telescope, due for completion in 2012.Read moreRead less
A programme to study quarkonium-like states at ATLAS. Particle physics, the study of the fundamental building blocks of matter, has pioneered the use of large collaborations --- hundreds of scientists working in dozens of countries --- to solve difficult research problems. Australian groups have contributed to several such experiments, studying cosmic rays, neutrinos, and broken symmetries, as well as developing ATLAS, a vast experiment dedicated to understanding the origin of mass. This projec ....A programme to study quarkonium-like states at ATLAS. Particle physics, the study of the fundamental building blocks of matter, has pioneered the use of large collaborations --- hundreds of scientists working in dozens of countries --- to solve difficult research problems. Australian groups have contributed to several such experiments, studying cosmic rays, neutrinos, and broken symmetries, as well as developing ATLAS, a vast experiment dedicated to understanding the origin of mass. This project seeks to use ATLAS for a new purpose: searching for exotic mesons. Our existing commitment to ATLAS provides an opportunity to develop this as a new avenue of fundamental research in this country.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
Singular Causation: A Conceptual Analysis. The concept of causation plays a central role in structuring our experience of the world. Bu how is the concept of causation itself to be understood? This project aims to answer this question by advancing a novel theory to explain the content and structure of the concept. A book monograph outlining the new theory will be of interest not only to philosophers, but also to natural and social scientists concerned to understand the application of the concept ....Singular Causation: A Conceptual Analysis. The concept of causation plays a central role in structuring our experience of the world. Bu how is the concept of causation itself to be understood? This project aims to answer this question by advancing a novel theory to explain the content and structure of the concept. A book monograph outlining the new theory will be of interest not only to philosophers, but also to natural and social scientists concerned to understand the application of the concept in their disciplines, and to cognitive psychologists and artificial intelligence experts concerned to understand its role in human cognition.
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Field Statistics of Space and Astrophysical Phenomena. Waves and radiation typically occur in bursts and persist, with their driving particle distributions, for unexpectedly long distances in space and astrophysical sources. These features cannot be accounted for with older plasma theory but are explained naturally with stochastic growth theory (SGT). Recent observations show SGT to be widely applicable in space and for pulsars. We propose to make SGT into a quantitative dynamic theory tested on ....Field Statistics of Space and Astrophysical Phenomena. Waves and radiation typically occur in bursts and persist, with their driving particle distributions, for unexpectedly long distances in space and astrophysical sources. These features cannot be accounted for with older plasma theory but are explained naturally with stochastic growth theory (SGT). Recent observations show SGT to be widely applicable in space and for pulsars. We propose to make SGT into a quantitative dynamic theory tested on known SGT systems, to discover and interpret field statistics of natural radio emissions, and to develop and test observationally theories based on SGT and associated wave/radiation processes for key space and astrophysical phenomena.Read moreRead less