751 citations
- Monash UniversityAU11 papers
- St. Andrews UniversityUS3 papers
- Monash Medical CentreAU2 papers
- The University of MelbourneAU2 papers
- American Industrial Partners (United States)US1 paper
- Analysis & Policy ObservatoryAU1 paper
- ARC Centre of Excellence for Gravitational Wave DiscoveryAU1 paper
- ARC Centre of Excellence in Future Low-Energy Electronics TechnologiesAU1 paper
- Argonne National LaboratoryUS1 paper
- Australian Centre for Robotic VisionAU1 paper
- Australian Regenerative Medicine InstituteAU1 paper
- California Institute of TechnologyUS1 paper
23 papers
Adaptive Plane Reformatting for 4D Flow MRI using Deep Reinforcement Learning
Javier Bisbal, Julio Sotelo, Maria I Valdés +7
Background and Objective: Plane reformatting for four-dimensional phase contrast MRI (4D flow MRI) is time-consuming and prone to inter-observer variability, which limits fast card…
On shock capturing in smoothed particle hydrodynamics
Daniel J. Price
For the past 20 years, our approach to shock capturing in smoothed particle hydrodynamics (SPH) has been to use artificial viscosity and conductivity terms supplemented by switches…
Eddington envelopes: The fate of stars on parabolic orbits tidally disrupted by supermassive black holes
Daniel J. Price, David Liptai, Ilya Mandel +3
Stars falling too close to massive black holes in the centres of galaxies can be torn apart by the strong tidal forces. Simulating the subsequent feeding of the black hole with dis…
Frizzle: Combining spectra or images by forward modeling
David W. Hogg, Andrew R. Casey
When there are many observations of an astronomical source - many images with different dithers, or many spectra taken at different barycentric velocities - it is standard practice…
Inferring system parameters from the bursts of the accretion-powered pulsar IGR J17498-2921
D. K. Galloway, A. J. Goodwin, T. Hilder +2
Thermonuclear (type-I) bursts exhibit properties that depend both on the local surface conditions of the neutron stars on which they ignite, as well as the physical parameters of t…
Galaxy And Mass Assembly: The xSAGA Galaxy Complement in Nearby Galaxy Groups
B. W. Holwerda, S. Phillipps, S. Weerasooriya +5
Groups of galaxies are the intermediate density environment in which much of the evolution of galaxies is thought to take place. In spectroscopic redshift surveys, one can identify…