Astrophotonics: exploiting a new technological frontier to probe back to the Dark Ages. Photonics, a key research strength in Australia, emerged from the telecommunications industry. But this exciting field has now begun to foster new scientific disciplines. One of the most recent is astrophotonics, a field at the interface of photonics and another Australian research strength, astronomy. Astrophotonics will deliver cutting-edge technologies to ensure Australia's astronomical lead in the next de ....Astrophotonics: exploiting a new technological frontier to probe back to the Dark Ages. Photonics, a key research strength in Australia, emerged from the telecommunications industry. But this exciting field has now begun to foster new scientific disciplines. One of the most recent is astrophotonics, a field at the interface of photonics and another Australian research strength, astronomy. Astrophotonics will deliver cutting-edge technologies to ensure Australia's astronomical lead in the next decade. These new facilities will serve as a vital stepping stone to the Giant Magellan Telescope, a $500M project promising enormous economic, engineering and scientific opportunities for Australia. Astrophotonics will also lead to innovative technology transfer to fields such as medical science, optical computing and sensor technology.Read moreRead less
Gamma-ray burst astronomy in the Swift era and beyond. The study of gamma-ray bursts is one of the most active and exciting fields in astrophysics, and touches on subjects that are of interest to all humans: e.g., to what extent was life on Earth shaped by cataclysmic explosions in our Galaxy? Australia's ROTSE-III telescope is the only facility in the southern hemisphere capable of rapidly (within 10 seconds) finding optical light from gamma-ray bursts. It will provide Australian astronomers ....Gamma-ray burst astronomy in the Swift era and beyond. The study of gamma-ray bursts is one of the most active and exciting fields in astrophysics, and touches on subjects that are of interest to all humans: e.g., to what extent was life on Earth shaped by cataclysmic explosions in our Galaxy? Australia's ROTSE-III telescope is the only facility in the southern hemisphere capable of rapidly (within 10 seconds) finding optical light from gamma-ray bursts. It will provide Australian astronomers with a competitive advantage in this high-profile field. The project will involve and inspire some of our best physics and engineering students.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
Advanced X-ray Optical Systems: From innovative idea to intelligent implementation. This project combines advances made in x-ray optics by the x-ray physics group at the University of Melbourne with sophisticated microfabrication techniques developed at Swinburne University of Technology and at the Argonne National Laboratory synchrotron. This fusion gives us immediate access into a major space science initiative - an x-ray telescope for the International Space Station. At the same time we will ....Advanced X-ray Optical Systems: From innovative idea to intelligent implementation. This project combines advances made in x-ray optics by the x-ray physics group at the University of Melbourne with sophisticated microfabrication techniques developed at Swinburne University of Technology and at the Argonne National Laboratory synchrotron. This fusion gives us immediate access into a major space science initiative - an x-ray telescope for the International Space Station. At the same time we will be building a kernel of excellence, based on new approaches to x-ray imaging, that will be strategically placed to become an integral part of the development of experimental facilities for the Australian Synchrotron.Read moreRead less
Very high energy gamma-ray astronomy in Australia and the development of future gamma-ray detectors. Australia contributes to the burgeoning field of ground-based gamma-ray astronomy via its involvement in the CANGAROO-III project.
I will continue the development of CANGAROO-III and establish links with the other collaborations in this field, in particular H.E.S.S., also in the southern hemisphere. Studies with CANGAROO-III of high energy gamma-ray sources such as supernova remnants and active ....Very high energy gamma-ray astronomy in Australia and the development of future gamma-ray detectors. Australia contributes to the burgeoning field of ground-based gamma-ray astronomy via its involvement in the CANGAROO-III project.
I will continue the development of CANGAROO-III and establish links with the other collaborations in this field, in particular H.E.S.S., also in the southern hemisphere. Studies with CANGAROO-III of high energy gamma-ray sources such as supernova remnants and active galaxies will finally reveal the type of particles that are accelerated in such violent regions of our universe. The development of future ground-based gamma-ray detectors beyond CANGAROO-III is also a project aim, and will expand the energy coverage of gamma-ray detectors into uncharted territory.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
The Origin and Evolution of Cosmic Magnetism. This research will significantly advance our understanding of structure and evolution in the Universe, in keeping with Australia's outstanding track record of astronomical discovery. This program will also train students and build research capacity in the frontier area of X-ray astronomy, in which Australia currently has limited expertise. The instrumentation and techniques to be developed will lead to innovative transfers of technology to fields su ....The Origin and Evolution of Cosmic Magnetism. This research will significantly advance our understanding of structure and evolution in the Universe, in keeping with Australia's outstanding track record of astronomical discovery. This program will also train students and build research capacity in the frontier area of X-ray astronomy, in which Australia currently has limited expertise. The instrumentation and techniques to be developed will lead to innovative transfers of technology to fields such as telecommunications and medical imaging. These new facilities will also serve as vital stepping stones to the Square Kilometre Array, a billion-dollar international project which promises enormous economic, engineering and scientific opportunities for Australia.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