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
The Evolution of Gas in Galaxy Groups. The evolution of gas in galaxy groups is poorly understood, but is crucial to understanding galaxy evolution. This project provides a training opportunity for a talented postdoc to conduct the first `multiwavelength census' of southern galaxy groups, perform simulations and make predictions of group properties at early times. We will better understand the evolutionary processes in groups and provide a `local anchor' for future surveys. The knowledge gained ....The Evolution of Gas in Galaxy Groups. The evolution of gas in galaxy groups is poorly understood, but is crucial to understanding galaxy evolution. This project provides a training opportunity for a talented postdoc to conduct the first `multiwavelength census' of southern galaxy groups, perform simulations and make predictions of group properties at early times. We will better understand the evolutionary processes in groups and provide a `local anchor' for future surveys. The knowledge gained will feed directly into the design of the future Square Kilometre Array, and raise Australia's profile in this $1B project. We exploit Australia's best astronomical facilities, and establish a new University-CSIRO collaboration.
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Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0236657
Funder
Australian Research Council
Funding Amount
$210,000.00
Summary
Renewed Great Melbourne Telescope: Opening a Window on the Universe. We propose to refurbish the Great Melbourne Telescope (GMT) located at Mount Stromlo Observatory with a new state-of-the-art imager. This instrument will be available to the entire Australian Astronomical community, and will allow Australian researchers to undertake cutting edge research with this world leading two colour wide field imager. A fully automated observing and data reduction pipeline, a world first for a telescope o ....Renewed Great Melbourne Telescope: Opening a Window on the Universe. We propose to refurbish the Great Melbourne Telescope (GMT) located at Mount Stromlo Observatory with a new state-of-the-art imager. This instrument will be available to the entire Australian Astronomical community, and will allow Australian researchers to undertake cutting edge research with this world leading two colour wide field imager. A fully automated observing and data reduction pipeline, a world first for a telescope of this size, means astronomers can work on their data, analyzing everything from the Solar System, to the most distant objects in the Universe, rather than spending night after night at the telescope.Read moreRead less
From Nanosecond Timing to Nanohertz Gravitational Wave Detection. Radio pulsars are the collapsed cores of once-massive stars that are renowned for their exceptional rotational stability. Ever since their discovery Australia has played a prominent role in the discovery and monitoring of these enigmatic sources. The timing and discovery of millisecond pulsars is an area where Australia is a world leader. This programme will use a powerful new instrument on the Parkes radio telescope to search for ....From Nanosecond Timing to Nanohertz Gravitational Wave Detection. Radio pulsars are the collapsed cores of once-massive stars that are renowned for their exceptional rotational stability. Ever since their discovery Australia has played a prominent role in the discovery and monitoring of these enigmatic sources. The timing and discovery of millisecond pulsars is an area where Australia is a world leader. This programme will use a powerful new instrument on the Parkes radio telescope to search for the minute influence of gravitational waves from supermassive black hole binaries on the millisecond pulsars.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0882778
Funder
Australian Research Council
Funding Amount
$201,224.00
Summary
Water vapour radiometers for millimetre-wave phase correction for the Australia Telescope. Australia has a tradition of excellence in astronomy. Inspired by wonder about the cosmos, it stimulates public interest in science, so leading to the training of highly skilled graduates. In turn, this drives the development of technologies needed to pursue the science. The nation has invested in the technology for millimetre-wave astronomy, building the first interferometer in our hemisphere. This equipm ....Water vapour radiometers for millimetre-wave phase correction for the Australia Telescope. Australia has a tradition of excellence in astronomy. Inspired by wonder about the cosmos, it stimulates public interest in science, so leading to the training of highly skilled graduates. In turn, this drives the development of technologies needed to pursue the science. The nation has invested in the technology for millimetre-wave astronomy, building the first interferometer in our hemisphere. This equipment will capitalise on this investment, extending the capabilities of the Australia Telescope to maintain it as a front line instrument, attracting the best scientists here to use it. This will help nurture a vigorous radio-science community, one able to actively participate in the billion-dollar investment being made internationally in the field.Read moreRead less
New Pulsar Instrumentation for Gravitation Wave Detection and Understanding the Emission Mechanism. Millisecond pulsar timing currently provides the most sensitive method of detecting long-period gravitational waves which permeate the Universe. Parkes leads the world in the discovery and timing of millisecond pulsars. This has motivated the development of three new advanced instruments including a cyrogenic dual-band receiver, a very wide-band correlator and a baseband recorder with an in-built ....New Pulsar Instrumentation for Gravitation Wave Detection and Understanding the Emission Mechanism. Millisecond pulsar timing currently provides the most sensitive method of detecting long-period gravitational waves which permeate the Universe. Parkes leads the world in the discovery and timing of millisecond pulsars. This has motivated the development of three new advanced instruments including a cyrogenic dual-band receiver, a very wide-band correlator and a baseband recorder with an in-built supercomputer. We aim to exploit these new technologies to systematically study the pulsar population. We will establish a timing array which can detect gravitational waves, enable GLAST to identify over 100 gamma-ray pulsars and study the pulsar emission mechanism at sub-microsecond time resolution.
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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
The Early History of Dark Energy. The national benefit will be the inclusion of Australian researchers (Glazebrook and his students/postdocs) in a major UK-Japanese international research project to study dark energy. This will be the successor to the highly successful WiggleZ project (on which Glazebrook is a designer and CI) using the much larger mirror of Subaru to push back the mapping of cosmic sound to much earlier epochs in the history of the Universe. Although Australia built parts of th ....The Early History of Dark Energy. The national benefit will be the inclusion of Australian researchers (Glazebrook and his students/postdocs) in a major UK-Japanese international research project to study dark energy. This will be the successor to the highly successful WiggleZ project (on which Glazebrook is a designer and CI) using the much larger mirror of Subaru to push back the mapping of cosmic sound to much earlier epochs in the history of the Universe. Although Australia built parts of the FMOS instrument (under contract) there is currently no national right of access to any of the science surveys so it is only by developing these collaborations that we can capitalize on our innovative instrument design.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0561136
Funder
Australian Research Council
Funding Amount
$376,352.00
Summary
36-megapixel CCD camera for wide-field astronomy. This project aims to design and build a state-of-the-art 36-megapixel charge-coupled device (CCD) camera for wide-field imaging on a robotic telescope at Siding Spring Observatory. The camera will employ a mosaic of two 18-megapixel CCDs, which are amongst the largest ever fabricated. This new facility will have an unprecedented ability to obtain precision photometry over a wide field, and will enable breakthroughs in research into areas as diver ....36-megapixel CCD camera for wide-field astronomy. This project aims to design and build a state-of-the-art 36-megapixel charge-coupled device (CCD) camera for wide-field imaging on a robotic telescope at Siding Spring Observatory. The camera will employ a mosaic of two 18-megapixel CCDs, which are amongst the largest ever fabricated. This new facility will have an unprecedented ability to obtain precision photometry over a wide field, and will enable breakthroughs in research into areas as diverse as detection of extra-solar planets and nearby supernovae. The camera will also lead to collaborative research with ANU's newly-funded Skymapper telescope, as well as the Anglo-Australian Observatory's 6dF and 2dF instruments.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