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.
Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE150100070
Funder
Australian Research Council
Funding Amount
$270,000.00
Summary
The Cherenkov Telescope Array. The Cherenkov Telescope Array: The Cherenkov Telescope Array (CTA) is a major advance in very high energy gamma-ray astronomy. It will be ten times more sensitive than current instruments and will transform many topics in high energy astrophysics concerning extreme particle acceleration, and in astro-particle physics such as dark matter. Over 1000 scientists from over 25 countries are involved and prototype telescopes are under construction. This project will enabl ....The Cherenkov Telescope Array. The Cherenkov Telescope Array: The Cherenkov Telescope Array (CTA) is a major advance in very high energy gamma-ray astronomy. It will be ten times more sensitive than current instruments and will transform many topics in high energy astrophysics concerning extreme particle acceleration, and in astro-particle physics such as dark matter. Over 1000 scientists from over 25 countries are involved and prototype telescopes are under construction. This project will enable a hardware contribution to the pre-production array of telescopes, bringing with it full membership, plus access to all data and core science programmes of CTA. Australian astronomers can then influence astrophysics goals of CTA, and add new scientific value to Australia's radio astronomical facilities.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE170100104
Funder
Australian Research Council
Funding Amount
$1,390,000.00
Summary
The Cherenkov Telescope Array - Production phase. This project aims to ensure Australia’s contribution to the five-year production phase of the Cherenkov Telescope Array (CTA), a very high energy gamma-ray astronomy instrument that is expected to transform both high energy astrophysics and astro-particle physics. Gamma-ray astronomy probes extreme processes in the Universe such as exploding stars, black holes, and mysterious dark matter. The project will maintain Australian access to all data an ....The Cherenkov Telescope Array - Production phase. This project aims to ensure Australia’s contribution to the five-year production phase of the Cherenkov Telescope Array (CTA), a very high energy gamma-ray astronomy instrument that is expected to transform both high energy astrophysics and astro-particle physics. Gamma-ray astronomy probes extreme processes in the Universe such as exploding stars, black holes, and mysterious dark matter. The project will maintain Australian access to all data and key science programmes of the CTA. Australian astronomers will be able to directly influence the major astrophysics goals of CTA, and link in with Australia's flagship astronomical infrastructure. This is expected to benefit astrophysics, big data processing, electronics, atmospheric physics and optics.Read moreRead less
ARC Centre of Excellence for Gravitational Wave Discovery. This Centre aims to explore the historic first detections of gravitational waves to understand the extreme physics of black holes and warped spacetime, and inspire the next generation of Australian scientists and engineers. The next-generation gravity wave detectors will enable a thousand-fold increase in detection volume and result in the new gravitational wave discoveries, triggering a new era of gravitational wave astrophysics. Buil ....ARC Centre of Excellence for Gravitational Wave Discovery. This Centre aims to explore the historic first detections of gravitational waves to understand the extreme physics of black holes and warped spacetime, and inspire the next generation of Australian scientists and engineers. The next-generation gravity wave detectors will enable a thousand-fold increase in detection volume and result in the new gravitational wave discoveries, triggering a new era of gravitational wave astrophysics. Building on decades of Australian investment in gravitational wave and pulsar science, this Centre will coalesce research activities into a focussed national programme whose discoveries are intended to experimentally validate Einstein’s General Theory of Relativity and educate the public about the wonders of Einstein's Universe.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.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE180100009
Funder
Australian Research Council
Funding Amount
$340,160.00
Summary
Doubling the power of a unique astronomical survey facility. This project aims to double the number of fibres in the spectrograph on the UK Schmidt Telescope and so double the number of stars and galaxies that it can observe simultaneously. This would allow rapid and timely completion of two major projects: the Taipan galaxy survey would be first to test a potential discrepancy in the expansion rate of the universe that may signal new physics, while the FunnelWeb stellar survey would (in tandem ....Doubling the power of a unique astronomical survey facility. This project aims to double the number of fibres in the spectrograph on the UK Schmidt Telescope and so double the number of stars and galaxies that it can observe simultaneously. This would allow rapid and timely completion of two major projects: the Taipan galaxy survey would be first to test a potential discrepancy in the expansion rate of the universe that may signal new physics, while the FunnelWeb stellar survey would (in tandem with two space missions) identify potential nearby exoplanets and trace the history of the Milky Way. The benefits include high scientific impact for the two surveys, international showcasing of the Australian Starbug technology, and a national astronomical survey facility for the next decade.Read moreRead less
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
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: LE120100023
Funder
Australian Research Council
Funding Amount
$185,000.00
Summary
Detailed spectrophotometric/velocity mapping of galaxies and identifying transient Gamma-Ray Burst Sources (GRBs) and the first stars with the unique upgraded Wide Field Spectrograph (WiFeS) facility. This project will allow light from galaxies be more efficiently detected and analysed. In particular details of a galaxy's composition, rotation, recessional velocity and star formation history will be possible following extensive refurbishment of the Siding Spring Observatory's Wide Field Spectrog ....Detailed spectrophotometric/velocity mapping of galaxies and identifying transient Gamma-Ray Burst Sources (GRBs) and the first stars with the unique upgraded Wide Field Spectrograph (WiFeS) facility. This project will allow light from galaxies be more efficiently detected and analysed. In particular details of a galaxy's composition, rotation, recessional velocity and star formation history will be possible following extensive refurbishment of the Siding Spring Observatory's Wide Field Spectrograph and installation of new extremely sensitive charged couple device (CCD) detectors.Read moreRead less