This project aims to develop a Python package to post-process 3-D hydrodynamics simulations (e.g., from RAMSES or Quokka) to create synthetic observations for JWST/HST/VLT.

In this project the student will investigate the feasibility of a 3D printed deformable mirror with an embedded water-cooling system, and its expected performance under extreme heat conditions based on the selected material and actuator configuration.

This project will use observations of star clusters with the Hubble Space Telescope to disentangle the multi scale nature of star formation in local spiral galaxies.

A resolved star formation study of galaxies using TYPHOON

The student will upgrade an existing seismic classifier using modern machine learning techniques and expanded training sets.

You will use 3D magnetohydrodynamic simulations to model asymmetric accretion on protostars and their discs.

Ambitious students will investigate optimal ways to measure the stellar properties (eg Teff, age, mass) and chemical composition of this immense amount of data.

In this project you will use existing and new data to understand the nature of filamentary structure in galaxies and how they relate to magnetic fields.

This project aims to determine what source is dominating in massive galaxies 4 Gyrs ago using MAGPI (MUSE), EMU (ASKAP) surveys and eROSITA public data.

This project aims to model performance of the MAVIS instrument on real galaxies samples drawn from available Hubble Space Telescope and James Webb Space Telescope imaging catalogues.

We are currently assembling a new supernova sample to constrain cosmology.

Redshifts are usually determined from the galaxies that host the supernovae, but some hosts are too faint. This project aims to improve the accuracy and precision of redshifts obtained from supernovae.

The student will process a database of sink-particle produced from 4pc^3 star cluster forming simulations to study how young binary and multiple stars evolve.

The successful applicant will join the ANU team and will participate in the design and testing of the Adaptive Optics Tracking and Pushing (AOTP) system.

Study of the statistics of turbulent, magnetised gases, relevant for the structure and evolution of the interstellar medium, the formation and evolution of stars and galaxies, using a combination of supercomputer simulations, theory, analytical calculations, and comparison to observations.

The kinematics and morphology of typically massive disk galaxies has changed dramatically over the last ~9 Gyrs.