Digital Interferometry: A platform technology for robust optical measurements. Digital interferometry is a new concept which will allow the measurement precision of interferometry to be applied in otherwise inaccessible or unsuitable environments. It will enhance the performance of major scientific instruments, such as gravitational wave detectors and optical telescopes, whilst reducing the cost, giving Australia a high profile in the quest to understand the universe. When applied to everyday ....Digital Interferometry: A platform technology for robust optical measurements. Digital interferometry is a new concept which will allow the measurement precision of interferometry to be applied in otherwise inaccessible or unsuitable environments. It will enhance the performance of major scientific instruments, such as gravitational wave detectors and optical telescopes, whilst reducing the cost, giving Australia a high profile in the quest to understand the universe. When applied to everyday situations, such as surveillance, traffic flow or vibration monitoring, it can give Australian industry a economic and social advantage, increasing the wealth and security of the nation. Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0775546
Funder
Australian Research Council
Funding Amount
$370,000.00
Summary
Construction of the blue-arm of the ANU 2.3m telescope Wide-Field Spectrograph. The new blue and red arms of the WiFeS spectrograph on the SSO 2.3m telescope utilizes new optical techniques and advances in detector technology to provide unique capabilities for front-line research and student training. The novel integral field units on WiFeS extract spectra across the face of faint, distant galaxies enabling the dynamics of the stellar and gas content to be analysed in unprecedented detail. Anoth ....Construction of the blue-arm of the ANU 2.3m telescope Wide-Field Spectrograph. The new blue and red arms of the WiFeS spectrograph on the SSO 2.3m telescope utilizes new optical techniques and advances in detector technology to provide unique capabilities for front-line research and student training. The novel integral field units on WiFeS extract spectra across the face of faint, distant galaxies enabling the dynamics of the stellar and gas content to be analysed in unprecedented detail. Another important project will be to follow-up interesting objects discovered by the new SkyMapper telescope and establish those that need to be observed on 8 m telescopes such as Gemini, Magellan or VLT. Read moreRead less
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
A clearer view of the evolving universe. The two complementary research objectives of this proposal are (i) a basic research program to understand star formation in galaxies through a study of the correlation betwen far infrared and radio continuum emission and (ii) a strategic research program to develop interference mitigation techniques to enable the next generation of radio telescopes which will study star formation in the early Universe. This programme of research innovation in radio astron ....A clearer view of the evolving universe. The two complementary research objectives of this proposal are (i) a basic research program to understand star formation in galaxies through a study of the correlation betwen far infrared and radio continuum emission and (ii) a strategic research program to develop interference mitigation techniques to enable the next generation of radio telescopes which will study star formation in the early Universe. This programme of research innovation in radio astronomy will also promote the broad aims of furthering opportunities for Australian participation in international science and of gaining insight into ways in which Australia can exploit its niche advantages in the global economy.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
Surface adsorption, repulsion and attraction: A new experimental approach to surface forces. The ability to understand and manipulate the stability of finely dispersed particles (colloids) in water is essential to modern living. It is necessary in processes as diverse as water purification, minerals separation, food and paper production. The behaviour of the colloidal system can often be understood in terms of the interaction between the dispersed particles. This project aims to improve our abil ....Surface adsorption, repulsion and attraction: A new experimental approach to surface forces. The ability to understand and manipulate the stability of finely dispersed particles (colloids) in water is essential to modern living. It is necessary in processes as diverse as water purification, minerals separation, food and paper production. The behaviour of the colloidal system can often be understood in terms of the interaction between the dispersed particles. This project aims to improve our ability to predict the nature of the interaction between dispersed particles, through an understanding of the events at a particle surface during a collision with another particle. This will enable us to better understand and control real colloidal systems.Read moreRead less
Across the Gravitational Wave Spectrum. Violent astrophysical events in the universe emit gravitational waves across a spectrum from mHz to kHz, producing an infinitesimal?but detectable'strain in space-time itself. Like high energy physics projects, gravitational wave detection involves giant multi million dollar research facilities and extensive international collaboration. This project will develop ideas, equipment and algorithms which will enhance the performance of both high frequency (gro ....Across the Gravitational Wave Spectrum. Violent astrophysical events in the universe emit gravitational waves across a spectrum from mHz to kHz, producing an infinitesimal?but detectable'strain in space-time itself. Like high energy physics projects, gravitational wave detection involves giant multi million dollar research facilities and extensive international collaboration. This project will develop ideas, equipment and algorithms which will enhance the performance of both high frequency (ground) and low frequency (space) based laser interferometer type detectors, and see Australia expand its already important role in searching for nature's most elusive signals.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
Exploring the last frontier: cosmic reionization and the first galaxies. This program will help to position Australia as a leader in the development of the Square Kilometre Array, a 1.5 billion Euro radio telescope that Australia is vying to host. The program takes advantage of the uniquely radio quiet environment of Western Australia to achieve unprecedented measurements of the 'first light fossils' in the Universe, which reside in the portion of the radio spectrum that is filled by FM radio tr ....Exploring the last frontier: cosmic reionization and the first galaxies. This program will help to position Australia as a leader in the development of the Square Kilometre Array, a 1.5 billion Euro radio telescope that Australia is vying to host. The program takes advantage of the uniquely radio quiet environment of Western Australia to achieve unprecedented measurements of the 'first light fossils' in the Universe, which reside in the portion of the radio spectrum that is filled by FM radio transmissions in most parts of the planet. This ground-breaking research program will provide training for the next generation of world-class scientists and add to the already high profile of Australian astrophysics.Read moreRead less