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“Beacons in the Night” unveiling how galaxies light up dark matter. How dark matter influences the formation and evolution of galaxies is to this day an outstanding question in astrophysics. To answer it, world-class facilities and a unique combination of observations and theory are required. This DP team, a world-class team of observers and theorists, will tackle this question by leveraging on two multi-million dollar projects: the MAGPI galaxy survey and the hydrodynamical simulations suite EA ....“Beacons in the Night” unveiling how galaxies light up dark matter. How dark matter influences the formation and evolution of galaxies is to this day an outstanding question in astrophysics. To answer it, world-class facilities and a unique combination of observations and theory are required. This DP team, a world-class team of observers and theorists, will tackle this question by leveraging on two multi-million dollar projects: the MAGPI galaxy survey and the hydrodynamical simulations suite EAGLE-XL. MAGPI will deliver exquisite kinematics for hundreds of galaxies in the middle ages of the Universe, providing a view to the effect of dark matter on galaxies at this critical time, while EAGLE-XL represents the technological frontier in simulations and provides the best interpretative framework for MAGPI.Read moreRead less
Feeding the faintest black holes: the nature of low-luminosity accretion. The overwhelming majority of black holes are found in an extremely faint quiescent state. This project aims to improve understandings of this large population of black holes, determining the geometry of the inflowing gas, the source of the faint X-ray emission, and the fraction of energy pumped outwards in fast-moving jets. Building on recent ground-breaking results, this project aims to conduct a survey to detect a new po ....Feeding the faintest black holes: the nature of low-luminosity accretion. The overwhelming majority of black holes are found in an extremely faint quiescent state. This project aims to improve understandings of this large population of black holes, determining the geometry of the inflowing gas, the source of the faint X-ray emission, and the fraction of energy pumped outwards in fast-moving jets. Building on recent ground-breaking results, this project aims to conduct a survey to detect a new population of black holes in dense star clusters, providing new laboratories to explore accretion physics. It aims to measure the distances of the black holes and their motion through space, test evidence for the existence of event horizons, and provide new insights into how black holes form and how they affect their surroundings.Read moreRead less
Discovery Early Career Researcher Award - Grant ID: DE150100618
Funder
Australian Research Council
Funding Amount
$354,000.00
Summary
Gas in the Cosmic Web: feeding and feedback of galaxies. This project aims to understand the complete cycle of gas in galaxies: from the process of feeding galaxies, going through star formation, to the process of outflowing gas from galaxies. This requires a full physical description of the inflow of gas from filaments going through the halo until reaching galaxies, the process of star formation in a multi-phase gas medium, and the effect energetic events have on the gas content of galaxies. Th ....Gas in the Cosmic Web: feeding and feedback of galaxies. This project aims to understand the complete cycle of gas in galaxies: from the process of feeding galaxies, going through star formation, to the process of outflowing gas from galaxies. This requires a full physical description of the inflow of gas from filaments going through the halo until reaching galaxies, the process of star formation in a multi-phase gas medium, and the effect energetic events have on the gas content of galaxies. This project in the field of extragalactic astrophysics is designed to complement major observational efforts in Australia, such as the Square Kilometre Array and its Pathfinder, as it will provide simulations with full physical descriptions of the neutral gas in the Universe.Read moreRead less
New Dimensions in Radio Astronomy: Mining Sparse Datasets with the Australian Square Kilometre Array Pathfinder. Radio astronomy is entering a new era, driven by technological advances that make rapid surveys of the sky possible. As leaders of three major surveys for the Australian Square Kilometre Array Pathfinder (ASKAP) telescope, we will explore three new dimensions of astronomy: searching for transient sources, detecting faint galaxies and investigating cosmic magnetism. The project will pu ....New Dimensions in Radio Astronomy: Mining Sparse Datasets with the Australian Square Kilometre Array Pathfinder. Radio astronomy is entering a new era, driven by technological advances that make rapid surveys of the sky possible. As leaders of three major surveys for the Australian Square Kilometre Array Pathfinder (ASKAP) telescope, we will explore three new dimensions of astronomy: searching for transient sources, detecting faint galaxies and investigating cosmic magnetism. The project will put Australian astronomers at the forefront of international research. In addition to novel scientific results we will produce data resources and software that will be critical for future Square Kilometre Array projects. These will be available online to amateur astronomers and the general public. We will train the next generation of astronomers with the skills required to make breakthrough discoveries.Read moreRead less
Beyond appearance: revealing the physics of galaxy transformation. This project aims to reveal the physical origin of the large variety of galaxies in the universe by utilising multi-wavelength observations of nearby galaxies combined with advanced data analysis techniques and cutting-edge numerical simulations. The project expects to generate new knowledge in the area of astrophysics by providing a physically-motivated foundation to the subjective and qualitative taxonomic scheme generally used ....Beyond appearance: revealing the physics of galaxy transformation. This project aims to reveal the physical origin of the large variety of galaxies in the universe by utilising multi-wavelength observations of nearby galaxies combined with advanced data analysis techniques and cutting-edge numerical simulations. The project expects to generate new knowledge in the area of astrophysics by providing a physically-motivated foundation to the subjective and qualitative taxonomic scheme generally used to understand how galaxies, and ultimately stars and planets, formed and evolve. 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
Unveiling the first billion years: enabling epoch of reionisation science. This project aims to deliver detections and exploration of the Epoch of Reionisation (EoR) through observation of the 21 cm hydrogen emission line from gas in the first billion years of the Universe. The EoR and Cosmic Dawn mark the two remaining unobserved periods in the history of the Universe. Together, they are witness to the formation, birth and illumination of the first stars, galaxies and x-ray sources, and the con ....Unveiling the first billion years: enabling epoch of reionisation science. This project aims to deliver detections and exploration of the Epoch of Reionisation (EoR) through observation of the 21 cm hydrogen emission line from gas in the first billion years of the Universe. The EoR and Cosmic Dawn mark the two remaining unobserved periods in the history of the Universe. Together, they are witness to the formation, birth and illumination of the first stars, galaxies and x-ray sources, and the consequent transformation of the intergalactic medium from a cold, neutral fog of hydrogen, to a heated, ionised canvas for the luminous Universe. The 21cm neutral hydrogen radio signal maps the astrophysics and cosmology of the first billion years, providing a direct tracer of their evolution and spatial distribution. The project will deliver advances in early Universe physics by circumventing limitations of current experiments, and will deliver lasting scientific and technological breakthroughs.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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The astrophysical stochastic background of gravitational waves and detection by advanced high optical power interferometers: an Australia-US collaboration. The proposed project is designed to enable one of the most exciting and least studied components of the gravitational wave spectrum, the Astrophysical Gravitational wave Background (AGB), to be detected by Advanced LIGO. It will extend the Australia-US collaboration in Advanced LIGO to include modeling, simulation and detection methods of the ....The astrophysical stochastic background of gravitational waves and detection by advanced high optical power interferometers: an Australia-US collaboration. The proposed project is designed to enable one of the most exciting and least studied components of the gravitational wave spectrum, the Astrophysical Gravitational wave Background (AGB), to be detected by Advanced LIGO. It will extend the Australia-US collaboration in Advanced LIGO to include modeling, simulation and detection methods of the AGB and the study of the optical noise in LIGO and Advanced LIGO type systems. In particular we plan to search for anomalous noise sources and, especially those arising in high optical power cavities that could limit detection of the AGB.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE200100201
Funder
Australian Research Council
Funding Amount
$530,000.00
Summary
A major upgrade to the Australia Telescope Compact Array. This project aims to upgrade the $150m CSIRO Australia Telescope Compact Array ("the telescope"), by replacing the signal processing electronics and doubling the bandwidth. This will significantly enhance the performance of the telescope, enabling more ambitious science by the 450 researchers and students who use it each year. For example, it will enable the telescope to study radio counterparts to Gravitational Wave sources, and it will ....A major upgrade to the Australia Telescope Compact Array. This project aims to upgrade the $150m CSIRO Australia Telescope Compact Array ("the telescope"), by replacing the signal processing electronics and doubling the bandwidth. This will significantly enhance the performance of the telescope, enabling more ambitious science by the 450 researchers and students who use it each year. For example, it will enable the telescope to study radio counterparts to Gravitational Wave sources, and it will enable it to make detailed observations of initial discoveries made with the Australian Square Kilometre Array Pathfinder and other Australian telescopes. In short, it will enable Australian researchers to do more ambitious research, and make more discoveries, across broad areas of astrophysics.Read moreRead less