Interstellar Physics at the Epoch of Galaxy Formation. With large telescopes and major space observatories, we can finally reach back in time and see how galaxies were assembled in the first few billion years of our Universe. We need to determine how gas forms into stars, how massive black holes feed on and interact with their nascent galaxies, how heavy elements are produced, and how dust obscuration or re-radiation affects observations. This proposal brings a world-class team together to devel ....Interstellar Physics at the Epoch of Galaxy Formation. With large telescopes and major space observatories, we can finally reach back in time and see how galaxies were assembled in the first few billion years of our Universe. We need to determine how gas forms into stars, how massive black holes feed on and interact with their nascent galaxies, how heavy elements are produced, and how dust obscuration or re-radiation affects observations. This proposal brings a world-class team together to develop and apply new and unique pan-spectral tools based on physical models of the interstellar plasma and conceived to determine fundamental parameters of collapsing galaxies.Read moreRead less
Molecules as probes of the interstellar medium. It is one of the greatest challenges in Nature is to remotely identify what is in space. Interstellar molecules are identified by their spectra, but many features in these spectra are unknown, implying that there are many more molecules in space than we know about. With a stronger understanding of space chemistry, we could predict what should be there and verify it in the lab. Conversely, identification of these features will provide the tools to u ....Molecules as probes of the interstellar medium. It is one of the greatest challenges in Nature is to remotely identify what is in space. Interstellar molecules are identified by their spectra, but many features in these spectra are unknown, implying that there are many more molecules in space than we know about. With a stronger understanding of space chemistry, we could predict what should be there and verify it in the lab. Conversely, identification of these features will provide the tools to understand interstellar chemistry. In this project we combine skills in spectroscopy and astronomy to make these molecules in the laboratory, measure their spectra and thereby identify unknown molecules in space.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0989648
Funder
Australian Research Council
Funding Amount
$350,000.00
Summary
Optical test-bed facility for mid infrared components for sensing, imaging and astrophotonics. This test facility will enable Australian researchers to validate optical components and technologies at wavelengths from 2.5 to 20 microns, that are crucial for a wide range of applications including biophotonics, sensing, imaging, defense, and astro-photonics. Technologies related to the Mid IR are
expected to have a significant impact on quality of life and global economy. It will enable Australi ....Optical test-bed facility for mid infrared components for sensing, imaging and astrophotonics. This test facility will enable Australian researchers to validate optical components and technologies at wavelengths from 2.5 to 20 microns, that are crucial for a wide range of applications including biophotonics, sensing, imaging, defense, and astro-photonics. Technologies related to the Mid IR are
expected to have a significant impact on quality of life and global economy. It will enable Australian researchers to achieve a major impact in many areas of Mid IR fundamental and applied science as well as industry sectors such as sensing, biophotonics, defence, health, bio-security and imaging. Read moreRead less
The First Deep Infrared Study of the Nearby Galaxy Population. We will conduct two major near-infrared (IR) surveys: The Southern Galactic Cap near-IR survey, and the Local Sphere of Influence survey. These surveys will capitalise on the innovative and award winning Australian IRIS2 facility. The two surveys push the observational frontier by orders of magnitude. They will be used to explore the close connection between the near-IR global properties of a galaxy and its underlying physics and pro ....The First Deep Infrared Study of the Nearby Galaxy Population. We will conduct two major near-infrared (IR) surveys: The Southern Galactic Cap near-IR survey, and the Local Sphere of Influence survey. These surveys will capitalise on the innovative and award winning Australian IRIS2 facility. The two surveys push the observational frontier by orders of magnitude. They will be used to explore the close connection between the near-IR global properties of a galaxy and its underlying physics and provide a generic local reference for the upcoming next generation infrared space-telescope missions.
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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
Dying stars, mass loss and the creation of the elements. This project aims to observationally estimate the mass loss rates and the surface chemical enrichments exhibited by low and intermediate-mass stars during their final evolutionary stages. The study has become possible because of new telescopes and instruments just arrived or imminently to arrive. Another part of the project is to use the observations to calibrate theoretical models for the evolution of dying stars. Such models are requi ....Dying stars, mass loss and the creation of the elements. This project aims to observationally estimate the mass loss rates and the surface chemical enrichments exhibited by low and intermediate-mass stars during their final evolutionary stages. The study has become possible because of new telescopes and instruments just arrived or imminently to arrive. Another part of the project is to use the observations to calibrate theoretical models for the evolution of dying stars. Such models are required for an understanding of the chemical enrichment of the universe from the time of first star formation to the present.
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Special Research Initiatives - Grant ID: SR0354517
Funder
Australian Research Council
Funding Amount
$20,000.00
Summary
Adaptive Optics for Australian Astronomy, Medicine, Industry, and Defence. Adaptive optics is a technique for correcting wavefront distortions in light beams to improve optical imaging performance. The Research Network for Adaptive Optics aims to draw together isolated Australian and New Zealand research groups working on adaptive optics applications in disparate areas to achieve a critical mass of researchers in this burgeoning field. Adaptive optics has wide application in areas as diverse as ....Adaptive Optics for Australian Astronomy, Medicine, Industry, and Defence. Adaptive optics is a technique for correcting wavefront distortions in light beams to improve optical imaging performance. The Research Network for Adaptive Optics aims to draw together isolated Australian and New Zealand research groups working on adaptive optics applications in disparate areas to achieve a critical mass of researchers in this burgeoning field. Adaptive optics has wide application in areas as diverse as astronomy, vision science, ophthalmology, microscopy, optical communications, laser radar, and laser beam shaping. The Research Network will coordinate and expand Australian involvement in these areas and inform industry, as have similar networks in the USA and Europe.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0561104
Funder
Australian Research Council
Funding Amount
$402,128.00
Summary
A 10 Gbit/s Fibre Optic link to the Mt Pleasant and Mt Canopus Observatories. A 10 gigabit per second fibre optic link to the Mt Pleasant and Mt Canopus observatories will enable a wide range of new and exciting research opportunities. Very long baseline interferometry (VLBI) allows imaging of distant astronomical objects with much higher resolution than any other technique. The proposed fibre optic link will revolutionise Australia's VLBI capability, giving it the world's most sensitive array, ....A 10 Gbit/s Fibre Optic link to the Mt Pleasant and Mt Canopus Observatories. A 10 gigabit per second fibre optic link to the Mt Pleasant and Mt Canopus observatories will enable a wide range of new and exciting research opportunities. Very long baseline interferometry (VLBI) allows imaging of distant astronomical objects with much higher resolution than any other technique. The proposed fibre optic link will revolutionise Australia's VLBI capability, giving it the world's most sensitive array, with enhanced reliability and faster access to results for researchers. This project will greatly facilitate studies of astrophysical processes in Galactic and extra-galactic environments as well as precision measurements of the Earth's crustal dynamics.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
Special Research Initiatives - Grant ID: SR0354794
Funder
Australian Research Council
Funding Amount
$10,000.00
Summary
Australian e-Astronomy. Australian e-Astronomy will provide a pre-eminent example of an integrated e-Science program. The Australian e-Astronomy Research Network will build on and extend the LIEF-funded national program to participate in the International Virtual Observatory. The network includes key members of most Australian astronomy research groups, a strong group representing grid research and advanced computing partnerships and an extensive group of international experts. The network dev ....Australian e-Astronomy. Australian e-Astronomy will provide a pre-eminent example of an integrated e-Science program. The Australian e-Astronomy Research Network will build on and extend the LIEF-funded national program to participate in the International Virtual Observatory. The network includes key members of most Australian astronomy research groups, a strong group representing grid research and advanced computing partnerships and an extensive group of international experts. The network developed by Australian e-Astronomy will service the entire Australian astronomical research community (eg theory codes, databases, software telescopes) and provide new programs for postgraduate research training.Read moreRead less