Optical phased array for space debris tracking and manoeuvring. Space junk in low Earth orbit is increasing at an alarming rate, jeopardising our access to critical navigation, communications, weather and natural disaster warning services. This project will prevent collisions of debris with satellites by developing a new laser system called an optical phased array to track and remotely manoeuvre space debris.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE140100013
Funder
Australian Research Council
Funding Amount
$300,000.00
Summary
A sensitive tip-tilt wave-front sensor for the multi-conjugate adaptive-optics system on the Gemini south telescope. A sensitive tip-tilt wavefront sensor for the multi-conjugate adaptive-optics system on the Gemini South telescope: This project will construct a sensitive tip-tilt wavefront sensor for GeMS, the multi-conjugate adaptive-optics system on the Gemini South telescope in Chile. GeMS is a unique and revolutionary new system that delivers near-infrared images at similar resolution to th ....A sensitive tip-tilt wave-front sensor for the multi-conjugate adaptive-optics system on the Gemini south telescope. A sensitive tip-tilt wavefront sensor for the multi-conjugate adaptive-optics system on the Gemini South telescope: This project will construct a sensitive tip-tilt wavefront sensor for GeMS, the multi-conjugate adaptive-optics system on the Gemini South telescope in Chile. GeMS is a unique and revolutionary new system that delivers near-infrared images at similar resolution to the Hubble Space Telescope at optical wavelengths over wide fields. With this improvement in technology it will be possible to do this on much fainter objects than is currently possible using this new wave-front sensor. This will allow GeMS to routinely study the morphologies of external galaxies at high angular resolution - greatly extending its science scope. Sharper images will also be obtained for all objects that are currently accessible, leading to higher quality science data.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE170100004
Funder
Australian Research Council
Funding Amount
$502,453.00
Summary
Semiconductor laser for adaptive optics in astronomy and space awareness. This project aims to create a laser system for use as a laser guide star. Semiconductor laser technology is a cost effective, highly reliable and compact alternative to expensive, inefficient, bulky laser systems. This laser has wide scientific appeal for research with telescopes in astronomy, and for satellite tracking and mitigation of the threat of space debris. Producing a sodium laser guide star in Australia is expect ....Semiconductor laser for adaptive optics in astronomy and space awareness. This project aims to create a laser system for use as a laser guide star. Semiconductor laser technology is a cost effective, highly reliable and compact alternative to expensive, inefficient, bulky laser systems. This laser has wide scientific appeal for research with telescopes in astronomy, and for satellite tracking and mitigation of the threat of space debris. Producing a sodium laser guide star in Australia is expected to secure the country's position as the premier provider of commercial-grade laser guide star adaptive optics systems for civil and defence telescopes around the world.Read moreRead less
Discovery Early Career Researcher Award - Grant ID: DE160101585
Funder
Australian Research Council
Funding Amount
$388,463.00
Summary
Harnessing Astrophotonics and Adaptive Optics to Discover Habitable Planets. This project aims to improve spectrographic design in order to increase precision in astronomical research. The discovery of Earth's twin, a habitable world in another stellar system, is one of the most remarkable scientific endeavours of our time. The gravitational tug of the planet on its host star causes a periodic Doppler shift of the star’s spectrum which is recorded using spectrographs. The instrumental precision ....Harnessing Astrophotonics and Adaptive Optics to Discover Habitable Planets. This project aims to improve spectrographic design in order to increase precision in astronomical research. The discovery of Earth's twin, a habitable world in another stellar system, is one of the most remarkable scientific endeavours of our time. The gravitational tug of the planet on its host star causes a periodic Doppler shift of the star’s spectrum which is recorded using spectrographs. The instrumental precision required to detect an Earth-like planet is a few centimetres per second, significantly better than the best current spectrographs can provide. This project plans to combine novel technologies from adaptive optics and astrophotonics into an innovative spectrograph design that will improve Doppler precision by a factor of ten, sufficient to find planets.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE200100012
Funder
Australian Research Council
Funding Amount
$632,000.00
Summary
Exploring the Dynamic Universe with DREAMS. DREAMS is a revolutionary wide-field infrared surveyor designed to allow astronomers to unlock new science and foster international collaborations focused on important but elusive, infrared transient cosmic phenomena. Continually scanning the southern sky, DREAMS will provide “real time” data that will transform the depth and quality of astronomical observation. Combining off-the-shelf parts with scientific expertise from around the world, this telesco ....Exploring the Dynamic Universe with DREAMS. DREAMS is a revolutionary wide-field infrared surveyor designed to allow astronomers to unlock new science and foster international collaborations focused on important but elusive, infrared transient cosmic phenomena. Continually scanning the southern sky, DREAMS will provide “real time” data that will transform the depth and quality of astronomical observation. Combining off-the-shelf parts with scientific expertise from around the world, this telescope will help answer questions that are both practical and profound. DREAMS is an important component of a longer-term international strategy that will reinforce Australia’s global leadership in the realm of Infrared Transient Astronomy.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.
Unveiling the first billion years: enabling epoch of reionisation science. This project aims to deliver detections and exploration of the Epoch of Reionisation (EoR) through observation of the 21 cm hydrogen emission line from gas in the first billion years of the Universe. The EoR and Cosmic Dawn mark the two remaining unobserved periods in the history of the Universe. Together, they are witness to the formation, birth and illumination of the first stars, galaxies and x-ray sources, and the con ....Unveiling the first billion years: enabling epoch of reionisation science. This project aims to deliver detections and exploration of the Epoch of Reionisation (EoR) through observation of the 21 cm hydrogen emission line from gas in the first billion years of the Universe. The EoR and Cosmic Dawn mark the two remaining unobserved periods in the history of the Universe. Together, they are witness to the formation, birth and illumination of the first stars, galaxies and x-ray sources, and the consequent transformation of the intergalactic medium from a cold, neutral fog of hydrogen, to a heated, ionised canvas for the luminous Universe. The 21cm neutral hydrogen radio signal maps the astrophysics and cosmology of the first billion years, providing a direct tracer of their evolution and spatial distribution. The project will deliver advances in early Universe physics by circumventing limitations of current experiments, and will deliver lasting scientific and technological breakthroughs.Read moreRead less
Equipping VIKiNG: mid-infrared technology for exoplanet characterisation. This project aims to develop thermal infrared technologies for the Very large telescope interferometer Infrared Kernel-NullinG instrument (VIKiNG), making it the most capable direct exoplanet detection instrument on any existing, or under construction, facility. Australia is currently world leading in innovative photonics technologies, and these are currently the limiting factor in producing a manufacturable design for VIK ....Equipping VIKiNG: mid-infrared technology for exoplanet characterisation. This project aims to develop thermal infrared technologies for the Very large telescope interferometer Infrared Kernel-NullinG instrument (VIKiNG), making it the most capable direct exoplanet detection instrument on any existing, or under construction, facility. Australia is currently world leading in innovative photonics technologies, and these are currently the limiting factor in producing a manufacturable design for VIKiNG. This project provides a clear pathway for laboratory development of high-efficiency, active mid-infrared photonic circuits in the thermal infrared. Beyond benefits to astronomy, these circuits are the first step in developing remote molecule detectors for environmental monitoring and security.Read moreRead less
High-cadence near-infrared imaging. This project aims to deploy a cryogenic camera system to improve the outputs of astronomical telescopes. The system is equipped with an emerging detector technology, a near-infrared Avalanche Photo-Diode array, capable of high cadence imaging with frame rates of 10 - 1,000 Hz at a wavelength of around 2.2 microns. This new technology is a key component to the future of adaptive optics systems for astronomical telescopes as it allows the rapid measurements nece ....High-cadence near-infrared imaging. This project aims to deploy a cryogenic camera system to improve the outputs of astronomical telescopes. The system is equipped with an emerging detector technology, a near-infrared Avalanche Photo-Diode array, capable of high cadence imaging with frame rates of 10 - 1,000 Hz at a wavelength of around 2.2 microns. This new technology is a key component to the future of adaptive optics systems for astronomical telescopes as it allows the rapid measurements necessary to correct the image blurring introduced by the Earth's atmosphere. No expertise currently exists in Australia with this new technology. Capitalising on previous investment, the camera system is intended to fill a capability gap in local expertise and to ensure the potential of the next generation of telescopes is realised and strengthen our competitive edge for frontier instrumentation across the wider Australian imaging community.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE210100015
Funder
Australian Research Council
Funding Amount
$1,680,000.00
Summary
The Cherenkov Telescope Array - From Production towards Operation. The Cherenkov Telescope Array is a transformational facility in very-high-energy gamma-ray astronomy. It will be 10 times more sensitive than current instruments and will revolutionise many topics in high energy astrophysics, and in astro-particle physics such as dark matter. Over 1000 scientists from over 30 countries are involved and the first telescopes on the southern hemisphere site in Chile will be installed from about 2021 ....The Cherenkov Telescope Array - From Production towards Operation. The Cherenkov Telescope Array is a transformational facility in very-high-energy gamma-ray astronomy. It will be 10 times more sensitive than current instruments and will revolutionise many topics in high energy astrophysics, and in astro-particle physics such as dark matter. Over 1000 scientists from over 30 countries are involved and the first telescopes on the southern hemisphere site in Chile will be installed from about 2021. This project will ensure Australia's contribution to complete the facility, leading into its operations phase (starting in 2027). It will also fund unique optical astronomy hardware that will enable Australian scientific leadership in supporting some of the Cherenkov Telescope Array's Key Science Projects.
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