Linkage Infrastructure, Equipment And Facilities - Grant ID: LE130100163
Funder
Australian Research Council
Funding Amount
$300,000.00
Summary
High performance clock facility for new-generation radar, imaging, measurement and radio-astronomy applications. At the heart of critical modern technologies (e.g. communications, navigation, radar) lies a high quality oscillator that generates an ultra-pure signal: it is this device that determines the overall system performance. The proposed facility will deliver breakthrough portable technology to improve the performance of these crucial technologies.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE160100045
Funder
Australian Research Council
Funding Amount
$360,000.00
Summary
Coherent Laser Links for Space Applications. Coherent laser links for space applications:
This project seeks equipment to establish a deployable, free-space, coherent laser link to enable Australia’s continued leadership and involvement in large-scale international space projects. It would support optical free-space frequency transfer to expand the capability of the European Space Agency’s Atomic Clock Ensemble in Space mission; tests to validate the inter-satellite interferometry acquisition s ....Coherent Laser Links for Space Applications. Coherent laser links for space applications:
This project seeks equipment to establish a deployable, free-space, coherent laser link to enable Australia’s continued leadership and involvement in large-scale international space projects. It would support optical free-space frequency transfer to expand the capability of the European Space Agency’s Atomic Clock Ensemble in Space mission; tests to validate the inter-satellite interferometry acquisition system for the NASA Gravity Recovery and Climate Experiment follow-on mission; and test-bed development for advanced coherent optical communications systems. Coherent, free-space laser links are an emerging technology for a range of high-impact research fields. The project would enable research relying on precision measurements of time and frequency; advanced inter-satellite laser interferometry, and coherent free-space optical communications. Read moreRead less
Creating a national time and frequency network for Australia. This project will develop the means to distribute accurate time and frequency across the Australian continent via an optical fibre network. This network will meet the needs of future telecommunications, science and astronomy projects including the Australian bid for the Square Kilometre Array radio-astronomy project.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE100100164
Funder
Australian Research Council
Funding Amount
$500,000.00
Summary
GNOSIS: a new window on the early universe using revolutionary photonic technology. Australian astronomers have a long history in innovative instrumentation and are some of the early pioneers in infrared astronomy. The GNOSIS project brings together leading Australian astronomers to build on past success. This facility instrument makes use of recent technological advances in photonics—a key strength of Australian research and industry—to provide a dramatic improvement in observational sensitivit ....GNOSIS: a new window on the early universe using revolutionary photonic technology. Australian astronomers have a long history in innovative instrumentation and are some of the early pioneers in infrared astronomy. The GNOSIS project brings together leading Australian astronomers to build on past success. This facility instrument makes use of recent technological advances in photonics—a key strength of Australian research and industry—to provide a dramatic improvement in observational sensitivity at these wavelengths. This will allow Australian astronomers to carry out new science programmes that have not been possible to date. These programmes include unprecedented observations of very cool low mass stars, the first chemical information on dust-embedded star clusters, and accurate ages for distant galaxies.Read moreRead less
Harnessing Mid-Infrared Photonic Technologies for Exoplanetary Discovery. This project will create new three-dimensional photonic technologies operating in the mid-infrared capable of discovering exoplanets. Starlight from this optimally-favourable spectral band will be collected over six of more apertures and undergo advanced on-chip photonic processing which will null out the bright starlight, but preserve the faint signature betraying the presence of an exoplanet. This device will empower vis ....Harnessing Mid-Infrared Photonic Technologies for Exoplanetary Discovery. This project will create new three-dimensional photonic technologies operating in the mid-infrared capable of discovering exoplanets. Starlight from this optimally-favourable spectral band will be collected over six of more apertures and undergo advanced on-chip photonic processing which will null out the bright starlight, but preserve the faint signature betraying the presence of an exoplanet. This device will empower visionary future astronomical instruments on the worlds most advanced telescopes.Read moreRead less
Sound and fury: finding planets amidst the noise of their dying stars. As solar-like stars expand to become red giants, their planetary systems gradual get destroyed, and the planet helps the stars to throw off their outer layers. This project will develop economic precise spectrographs to detect planets around giant stars and establish how this interaction occurs.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE160100191
Funder
Australian Research Council
Funding Amount
$175,000.00
Summary
PRAXIS: beating the infrared night sky with multicore fibre Bragg gratings. PRAXIS: beating the infrared night sky with multicore fibre Bragg gratings:
The PRAXIS project aims to deliver a new era in ground-based infrared observations. The infrared night sky is a hundred times brighter than the optical night sky, which has severely limited the sensitivity at these wavelengths. But 99 per cent of the infrared sky arises from hundreds of extremely bright, narrow emission lines due to hydroxyl in ....PRAXIS: beating the infrared night sky with multicore fibre Bragg gratings. PRAXIS: beating the infrared night sky with multicore fibre Bragg gratings:
The PRAXIS project aims to deliver a new era in ground-based infrared observations. The infrared night sky is a hundred times brighter than the optical night sky, which has severely limited the sensitivity at these wavelengths. But 99 per cent of the infrared sky arises from hundreds of extremely bright, narrow emission lines due to hydroxyl in the Earth's atmosphere. PRAXIS, at the Anglo-Australian Telescope, is designed to cancel these lines using new multicore fibre Bragg gratings developed in Australia. The new fibres would render the night sky very dark and allow Australian astronomers to obtain unique observations. The sky-suppressing fibres would also allow us to develop new instrument concepts for Australia's extremely large telescope.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE130100198
Funder
Australian Research Council
Funding Amount
$315,000.00
Summary
The SAMI facility: a revolutionary multi-object hexabundle spectrograph. SAMI is a new Australian instrument concept that uses fibre bundles to obtain detailed spectroscopic data at many positions across the face of numerous galaxies at a time. Now that the technology has been shown to work, with spectacular results, the project aims to turn this concept into a general-user facility at the Anglo-Australian Telescope.
How do galaxies get their gas? This project aims to build new understanding about the fundamental physics behind how galaxies get their gas. The way gas is accreted in galaxies affects how stars are made and what galaxies look like, including our own milky way. This project expects to build a new robotic instrument for three dimensional spectroscopy of galaxies, called Hector-I, to establish and run the Hector Galaxy Survey, the largest of its kind ever conducted. This survey data set will under ....How do galaxies get their gas? This project aims to build new understanding about the fundamental physics behind how galaxies get their gas. The way gas is accreted in galaxies affects how stars are made and what galaxies look like, including our own milky way. This project expects to build a new robotic instrument for three dimensional spectroscopy of galaxies, called Hector-I, to establish and run the Hector Galaxy Survey, the largest of its kind ever conducted. This survey data set will underpin broad investigations of gas accretion and the impact on the physical properties of galaxies. The project will clarify why our own galaxy looks so different to others, demonstrate Australian technologies for future commercialisation on international facilities, and train students for a high quality workforce.Read moreRead less