Linkage Infrastructure, Equipment And Facilities - Grant ID: LE110100030
Funder
Australian Research Council
Funding Amount
$350,000.00
Summary
Koala: a new integral field capability for the Anglo-Australian Telescope. This new instrument will be used by the Anglo-Australian Telescope and will be capable of simultaneously collecting over one thousand individual spectra from a region of sky. The data obtained will provide a wealth of information on extended astrophysical sources, such as star clusters, planetary nebulae and nearby galaxies.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE150100055
Funder
Australian Research Council
Funding Amount
$560,000.00
Summary
The Australian European Southern Observatory Positioner (AESOP). The Australian European Southern Observatory Positioner (AESOP): The aim of the Australian European Southern Observatory Positioner (AESOP) is to fund the construction costs of an innovative instrument to be built in Australia and installed onto the European Southern Observatory's (ESO) VISTA telescope. Australia leads the world in fibre-positioning instrumentation and their scientific exploitation. This project will allow Australi ....The Australian European Southern Observatory Positioner (AESOP). The Australian European Southern Observatory Positioner (AESOP): The aim of the Australian European Southern Observatory Positioner (AESOP) is to fund the construction costs of an innovative instrument to be built in Australia and installed onto the European Southern Observatory's (ESO) VISTA telescope. Australia leads the world in fibre-positioning instrumentation and their scientific exploitation. This project will allow Australian researchers to take a leading role through major studies of the spatial distributions of galaxies. The outcomes of the project will be construction and delivery of an optical fibre-positioning system to the ESO, resulting in general access to the ESO's premier survey facility for eight Australian researchers.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE160100145
Funder
Australian Research Council
Funding Amount
$430,000.00
Summary
Australian membership of the European 4MOST Consortium. Australian membership of the European 4MOST consortium:
The objective of this project is to build the positioner at the Australian Astronomical Observatory to enable participation in the upcoming programs of the European Southern Observatory (ESO). The 4MOST Consortium is modifying one of the ESO telescopes for a 10-year campaign of dedicated wide-field astronomy programs. A key component of this upgrade will be the Australian built fibre- ....Australian membership of the European 4MOST Consortium. Australian membership of the European 4MOST consortium:
The objective of this project is to build the positioner at the Australian Astronomical Observatory to enable participation in the upcoming programs of the European Southern Observatory (ESO). The 4MOST Consortium is modifying one of the ESO telescopes for a 10-year campaign of dedicated wide-field astronomy programs. A key component of this upgrade will be the Australian built fibre-positioning system. In exchange for covering the labour costs associated with this instrument, Australian astronomers are being provided with the opportunity to lead one of the eight design reference missions and to participate in the other seven. The potential benefits are therefore two-fold: showcasing Australian technologies, and a leadership role for Australian scientists on one of ESO’s key facilities.Read moreRead less
Discovery Early Career Researcher Award - Grant ID: DE140100316
Funder
Australian Research Council
Funding Amount
$325,515.00
Summary
Seeing in the dark: measuring the signature of the early Universe with low-frequency radio telescopes. This project will detect and measure the signature of the first ionising sources in the early Universe. It uses a unique intersection of information theory and analysis methodology to design and implement a method of extracting the faint neutral hydrogen signal of reionisation from complex datasets. The hydrogen structure around these first light sources will be measured using data from the Mur ....Seeing in the dark: measuring the signature of the early Universe with low-frequency radio telescopes. This project will detect and measure the signature of the first ionising sources in the early Universe. It uses a unique intersection of information theory and analysis methodology to design and implement a method of extracting the faint neutral hydrogen signal of reionisation from complex datasets. The hydrogen structure around these first light sources will be measured using data from the Murchison Widefield Array telescope in Western Australia, revealing the signature of reionisation for the first time. Measurement of this signal constrains our understanding of the large-scale evolution of the Universe, defines properties of the first generation of stars and galaxies, and expands our understanding of the full history of the Universe.Read moreRead less
Discovery Early Career Researcher Award - Grant ID: DE160100849
Funder
Australian Research Council
Funding Amount
$326,637.00
Summary
Measuring the Universe’s early evolution using lunar occultations. This project seeks to measure a radio signal for the first time, using the Murchison Widefield Array telescope and a novel technique involving the Moon, to learn what luminous objects dominated the early Universe. There is an entire period in the early Universe that remains unobserved because familiar objects such as stars and galaxies have yet to form. One of the few observables from this period, and the time directly following ....Measuring the Universe’s early evolution using lunar occultations. This project seeks to measure a radio signal for the first time, using the Murchison Widefield Array telescope and a novel technique involving the Moon, to learn what luminous objects dominated the early Universe. There is an entire period in the early Universe that remains unobserved because familiar objects such as stars and galaxies have yet to form. One of the few observables from this period, and the time directly following it, is the radio signal emitted by neutral hydrogen atoms. Innovative analysis techniques may be developed and new training pathways for astronomers should be initiated. The Project aims to raise Australia’s scientific profile and engage the public, promoting astronomy by making results accessible and using the Moon as a familiar foundation.Read moreRead less
Capturing gravitational wave and electromagnetic flashes from binary merger. This project aims to contribute to one of the most momentous and long-anticipated discoveries in physics: the first detection of gravitational waves. The project plans to develop innovative technologies to detect gravitational waves using laser interferometers and enable prompt follow-up observations of gravitational wave sources by conventional telescopes. The outcome of this research would greatly help probe the natur ....Capturing gravitational wave and electromagnetic flashes from binary merger. This project aims to contribute to one of the most momentous and long-anticipated discoveries in physics: the first detection of gravitational waves. The project plans to develop innovative technologies to detect gravitational waves using laser interferometers and enable prompt follow-up observations of gravitational wave sources by conventional telescopes. The outcome of this research would greatly help probe the nature of matter and gravity at extreme densities.Read moreRead less
Detection and Localisation of Gravitational Waves using Pulsar Timing Array. This project aims to contribute to one of the most significant breakthroughs in science - the direct detection of gravitational waves. It will develop innovative techniques to detect and localise gravitational waves in the nanohertz frequency band from radio timing data of millisecond pulsars. The technique developed by this project will help maximise the scientific output of Australia's legendary Parkes Radio Telescope ....Detection and Localisation of Gravitational Waves using Pulsar Timing Array. This project aims to contribute to one of the most significant breakthroughs in science - the direct detection of gravitational waves. It will develop innovative techniques to detect and localise gravitational waves in the nanohertz frequency band from radio timing data of millisecond pulsars. The technique developed by this project will help maximise the scientific output of Australia's legendary Parkes Radio Telescope, and boost the opportunities of the first detections of gravitational waves using the upcoming radio telescopes, Five hundred meter Aperture Spherical Telescope (FAST) and Square Kilometre Array (SKA).Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE120100181
Funder
Australian Research Council
Funding Amount
$650,000.00
Summary
Strengthening merit-based access and support at the new National Computing Infrastructure petascale supercomputing facility. World-leading high-performance computing is fundamental to Australia's international research success. This facility will provide access to the new National Computational Infrastructure facility by world-leading researchers from six research universities, and sustain ground-breaking work in an increasingly competitive environment.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE180100003
Funder
Australian Research Council
Funding Amount
$318,900.00
Summary
Vector network analyser suite for advanced terahertz materials and devices. This project aims to establish terahertz measurement capabilities to further Australia's strength and momentum in terahertz research. This will comprise of two terahertz extension modules, working with a dedicated vector-network analyser, and high-precision probes and probe station. The project will enable point-feeding, monochromatic, coherent, and fine spectral-resolution measurement at an atmospheric window of 220-330 ....Vector network analyser suite for advanced terahertz materials and devices. This project aims to establish terahertz measurement capabilities to further Australia's strength and momentum in terahertz research. This will comprise of two terahertz extension modules, working with a dedicated vector-network analyser, and high-precision probes and probe station. The project will enable point-feeding, monochromatic, coherent, and fine spectral-resolution measurement at an atmospheric window of 220-330 GHz. The capabilities are essential for development of two-dimensional materials, active components, waveguides, and antennas towards a common goal of efficient integrated terahertz devices and systems. The project will serve emerging terahertz applications including standoff imaging and short-range high-speed data transmission. This will have broad impact in the areas of surveillance, biomedicine, security, and public safety and well-being.Read moreRead less
Engineering high-efficiency all-dielectric antennas for terahertz channels. This project aims to create unconventional antenna platforms to support terahertz links. The project expects to deliver high-efficiency, high-gain dielectric resonator antennas and dielectric rod antenna arrays fed by dielectric wave-guides. The expected outcomes of this project will build critical components for future terahertz communication infrastructure. These antennas will support demands in point-to-point wireless ....Engineering high-efficiency all-dielectric antennas for terahertz channels. This project aims to create unconventional antenna platforms to support terahertz links. The project expects to deliver high-efficiency, high-gain dielectric resonator antennas and dielectric rod antenna arrays fed by dielectric wave-guides. The expected outcomes of this project will build critical components for future terahertz communication infrastructure. These antennas will support demands in point-to-point wireless transmission between mobile base stations, within data centres, and at information kiosks.Read moreRead less