The origin and evolution of heavy elements in the early universe. Everything in our Solar System, including all life on Earth, was created long ago out of material forged inside fiery stellar furnaces. The latest theoretical simulations of element production in red giant stars reveals the processes that gave us our existence, as well as help us to understand the origin of the galaxy that we inhabit.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE140100052
Funder
Australian Research Council
Funding Amount
$350,000.00
Summary
TAIPAN - a spectrograph to survey the southern sky. TAIPAN - a spectrograph to survey the southern sky: The TAIPAN spectroscopic survey of the southern sky aims to quadruple the number of nearby galaxies with measured redshifts, distances and velocities. Science goals include measuring the expansion rate of the universe to 1 per cent precision, and combining optical spectroscopy and radio data for each galaxy to measure the rate at which gas is being converted into stars in the local universe. T ....TAIPAN - a spectrograph to survey the southern sky. TAIPAN - a spectrograph to survey the southern sky: The TAIPAN spectroscopic survey of the southern sky aims to quadruple the number of nearby galaxies with measured redshifts, distances and velocities. Science goals include measuring the expansion rate of the universe to 1 per cent precision, and combining optical spectroscopy and radio data for each galaxy to measure the rate at which gas is being converted into stars in the local universe. This project supports construction of the TAIPAN high-performance spectrograph that will be used to carry out the survey on the UK Schmidt Telescope (UKST). The results of the survey will be made freely available to all Australian astronomers.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE130100104
Funder
Australian Research Council
Funding Amount
$740,000.00
Summary
Mapping the universe with the Panoramic Survey Telescope and Rapid Response System (PanSTARRS). This project plans to build a powerful new observatory, Panoramic Survey Telescope and Rapid Response System (PanSTARRS-2), to be located in Hawaii. PanSTARRS-2 will have an enormous fish-eye-lens view of the northern stars, which we will combine with Australian telescopes to give a unique view of the entire sky. Australian scientists will use this data to solve fundamental problems in astrophysics an ....Mapping the universe with the Panoramic Survey Telescope and Rapid Response System (PanSTARRS). This project plans to build a powerful new observatory, Panoramic Survey Telescope and Rapid Response System (PanSTARRS-2), to be located in Hawaii. PanSTARRS-2 will have an enormous fish-eye-lens view of the northern stars, which we will combine with Australian telescopes to give a unique view of the entire sky. Australian scientists will use this data to solve fundamental problems in astrophysics and cosmology.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE150100024
Funder
Australian Research Council
Funding Amount
$760,000.00
Summary
Kunlun Infrared Sky Survey. Kunlun Infrared Sky Survey (KISS): KISS is the first exploration of the time varying Universe in the infrared. The location at Kunlun station offers the advantage of the whole sky being available for study for the duration of the Antarctic winter every year. The primary scientific targets are the physics of active galactic nuclei, supersupernovae (Gamma Ray Bursters), the terminal phases of red giants (Miras) and initial phases of protostars. The project also aims to ....Kunlun Infrared Sky Survey. Kunlun Infrared Sky Survey (KISS): KISS is the first exploration of the time varying Universe in the infrared. The location at Kunlun station offers the advantage of the whole sky being available for study for the duration of the Antarctic winter every year. The primary scientific targets are the physics of active galactic nuclei, supersupernovae (Gamma Ray Bursters), the terminal phases of red giants (Miras) and initial phases of protostars. The project also aims to find exoplanets and to measure the cosmic infrared background and its angular fluctuations using the low background advantage of the Antarctic. KISS is complementary to SkyMapper in that it is infrared, and complementary to 2MASS in that it is time sensitive.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
Space Science and Astronomy: Dissecting the Galaxy with High Resolution Multi-Object Echelle Spectrograph (HERMES) II: Decisive Observations. Australia has long been a world leader in wide-field astronomical surveys, and the new High Resolution Multi-Object Echelle Spectrograph (HERMES) being built for the Anglo-Australian Telescope (AAT) will enhance that leadership position. Through a combination of Australian technological and scientific advances, the surveys we conduct with HERMES will allow ....Space Science and Astronomy: Dissecting the Galaxy with High Resolution Multi-Object Echelle Spectrograph (HERMES) II: Decisive Observations. Australia has long been a world leader in wide-field astronomical surveys, and the new High Resolution Multi-Object Echelle Spectrograph (HERMES) being built for the Anglo-Australian Telescope (AAT) will enhance that leadership position. Through a combination of Australian technological and scientific advances, the surveys we conduct with HERMES will allow us to study galaxy formation and stellar astrophysics in unprecedented detail. There are powerful synergies between HERMES and Skymapper, another Australian astronomical survey, as well as with Gaia, the billion-dollar European space mission for studying the Galaxy; HERMES will thus promote both national and international research collaboration. In this proposal we lay the observational groundwork for maximising the scientific return from HERMES.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE100100054
Funder
Australian Research Council
Funding Amount
$200,000.00
Summary
Next-generation robotic observatories for the remote Antarctic plateau. Australia's astronomers are exceptionally well placed to lead and to partner with major international programs in Antarctic astronomy. These bring Australian industry increased access to cutting-edge technology, and create business opportunities in the infrastructure and support of Antarctic research. This project aims to maintain Australia's lead in Antarctic astronomy and, with the inclusion of a new partnership with Jap ....Next-generation robotic observatories for the remote Antarctic plateau. Australia's astronomers are exceptionally well placed to lead and to partner with major international programs in Antarctic astronomy. These bring Australian industry increased access to cutting-edge technology, and create business opportunities in the infrastructure and support of Antarctic research. This project aims to maintain Australia's lead in Antarctic astronomy and, with the inclusion of a new partnership with Japan, to build upon our existing strong collaboration with China and the USA. Australia's participation in this program also ensures continued technology exchange, and builds our knowledge base in robotics, harsh-environment engineering and computational fluid dynamics, while creating important new astronomical opportunities.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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