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
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0237527
Funder
Australian Research Council
Funding Amount
$170,000.00
Summary
Bioscope IV : Advanced Scanned Probe Microscopy. The Atomic Force Microscope presents a unique view of the microscopic and molecular world, for it is sensitive to force alone. This instrument can accurately map force over a surface at the molecular scale; picoNewtons at nanometre resolution. The host of intermolecular forces which cause phenomena such as self-assembly, colloid stability, cell interactions and friction are only directly measurable with this technique. In this field of force meas ....Bioscope IV : Advanced Scanned Probe Microscopy. The Atomic Force Microscope presents a unique view of the microscopic and molecular world, for it is sensitive to force alone. This instrument can accurately map force over a surface at the molecular scale; picoNewtons at nanometre resolution. The host of intermolecular forces which cause phenomena such as self-assembly, colloid stability, cell interactions and friction are only directly measurable with this technique. In this field of force measurement Australian researchers are leaders. The proposed instrument expands the capabilities of this effort, and develops exciting new directions including the direct manipulation of molecules through a novel feedback and control (haptic) interface.Read moreRead less
Pushing the frontiers of gravitational wave science: from technology to astrophysics. The direct detection of Einstein's elusive gravitational waves will not only confirm one of the most important theories in physics, it will unleash a new form of radiation (in addition to electromagnetic) with which to study the Universe. Our participation in this quest continues Australia's role in the vanguard of new astronomy and its exploitation. This proposal will produce scientists highly trained in ar ....Pushing the frontiers of gravitational wave science: from technology to astrophysics. The direct detection of Einstein's elusive gravitational waves will not only confirm one of the most important theories in physics, it will unleash a new form of radiation (in addition to electromagnetic) with which to study the Universe. Our participation in this quest continues Australia's role in the vanguard of new astronomy and its exploitation. This proposal will produce scientists highly trained in areas of national priority, including frontier technologies such as photonics and smart information use through GRID computing. Developing ways to build instruments of almost unimaginable sensitivity fosters innovation leading to spin-offs into other areas of optical sensing - fundamental research resulting in economic benefit.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0346515
Funder
Australian Research Council
Funding Amount
$507,000.00
Summary
Fluorescence Detector for the Australian National Beamline Facility. X-ray absorption spectroscopy (XAS) is an extremely important synchrotron radiation tool for determining the local structure around an X-ray absorbing atom. This has many applications in the study of materials, minerals, metal complexes, and metalloproteins and can often be used to obtain information that is not available by other techniques, because structural information can be obtained in the solid or solution state and in ....Fluorescence Detector for the Australian National Beamline Facility. X-ray absorption spectroscopy (XAS) is an extremely important synchrotron radiation tool for determining the local structure around an X-ray absorbing atom. This has many applications in the study of materials, minerals, metal complexes, and metalloproteins and can often be used to obtain information that is not available by other techniques, because structural information can be obtained in the solid or solution state and in mixtures. The current proposal is aimed at introducing new technology into the Australian National Beamline Facility that will greatly improve the quality and quantity of experiments that can be performed and extend studies into dilute solutions and protein samples.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0989915
Funder
Australian Research Council
Funding Amount
$127,000.00
Summary
X-ray Nano-scale Coherence Facility. Australia is rapidly developing into a world leader for x-ray imaging. This position has been supported by leading research groups and more recently by the development of the Australian Synchrotron. This project will fill a vital missing link in the experimental capability of Australian researchers - a flexible facility that can provide a nanoscale x-ray source. This enhanced capability will lead to new developments in coherent imaging methods. These new meth ....X-ray Nano-scale Coherence Facility. Australia is rapidly developing into a world leader for x-ray imaging. This position has been supported by leading research groups and more recently by the development of the Australian Synchrotron. This project will fill a vital missing link in the experimental capability of Australian researchers - a flexible facility that can provide a nanoscale x-ray source. This enhanced capability will lead to new developments in coherent imaging methods. These new methods will be used in the study of biological systems, leading to better drug design as well as in the study of materials, leading to stronger and lighter components. Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0989093
Funder
Australian Research Council
Funding Amount
$1,800,000.00
Summary
Australian Partnership in Advanced LIGO. Advanced Interferometer Gravitational-Wave Observatory (LIGO) (AdvLIGO) will be the first gravitational wave observatory capable of frequent observation of known sources of gravitational waves leading to the birth of gravitational wave astronomy. The development of instruments capable of doing this is driving technology in fields such as lasers , optics, photonics and data analysis. By playing a key role in this facility, Australia will reap the scienti ....Australian Partnership in Advanced LIGO. Advanced Interferometer Gravitational-Wave Observatory (LIGO) (AdvLIGO) will be the first gravitational wave observatory capable of frequent observation of known sources of gravitational waves leading to the birth of gravitational wave astronomy. The development of instruments capable of doing this is driving technology in fields such as lasers , optics, photonics and data analysis. By playing a key role in this facility, Australia will reap the scientific and technical rewards of being part of the most exciting frontier of physics in the 21st Century whilst training scientists and technologists for tomorrow.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
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0454166
Funder
Australian Research Council
Funding Amount
$1,305,029.00
Summary
Nanoscale Materials Characterization Facility. We request a transmission and a scanning electron microscope, each with specialist electron probes smaller than a nanometre, which can selectively analyse the atomic structure and chemistry of sub-nanometre regions of material.
These capabilities are essential to advance a large range of research projects at the cutting-edge of materials science and engineering, undertaken by Victoria's leading research institutions: five Victorian universities, ....Nanoscale Materials Characterization Facility. We request a transmission and a scanning electron microscope, each with specialist electron probes smaller than a nanometre, which can selectively analyse the atomic structure and chemistry of sub-nanometre regions of material.
These capabilities are essential to advance a large range of research projects at the cutting-edge of materials science and engineering, undertaken by Victoria's leading research institutions: five Victorian universities, the CSIRO, Nanotechnology Victoria Ltd, the Victorian Centre for Advanced Materials Manufacturing and the CRC for Microtechnology. Together they have contributed $2.58 million to this project.
This state-of-the-art facility will include the highest spatial resolution microscope in Australia.
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