– Professor Nick Seymour
This broad project aims to extract valuable science from the Murchison Widefield Array (MWA), with particular focus on:
- Characterising enigmatic objects such as pulsars and fast radio transients;
- Observations from the Epoch of Reionisation – a cosmic period 13 billion years ago when the first stars and galaxies formed; and
- Galaxies – by surveying the entire southern hemisphere sky, the MWA will make in-depth observations of our own galaxy and external galaxies, allowing ICRAR scientists to map the Universe in greater detail than ever before.
Available Projects
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Advanced Calibration and Imaging with the MWA -
Characterising the ionosphere over the Murchison Radio astronomy Observatory -
A Census of Radio Galaxy Components via Measurements of Interplanetary Scintillation -
Detecting nanohertz-frequency gravitational waves with current and future radio telescopes -
Rapid Follow-Ups of Fast Radio Bursts with the MWA -
An Effective Cross-matching Framework for Catalogues and Images -
HI Absorption in high-z radio galaxies -
Combining GLEAM and ATLBS to discover the history of active galactic nuclei -
Cooperative Sensor Networks for the Detection of Ultra-High Energy Cosmic Rays -
Identifying optical counterparts of radio sources using citizen science -
Fast follow-up of Gamma-Ray Bursts with the Murchison Widefield Array -
Finding Pulsars with a Next-generation Low-frequency Radio Telescope -
From Low-frequency Pulsar Observations to Interstellar Holography -
GLEAM-X: Exploring the Universe in Radio Colour -
How Does the Cosmic Microwave Background Impact the First Radio Galaxies? -
Implementing a Space Debris Detection and Tracking System Using Next Generation Radio Telescopes, Advanced Data Processing, and Data Analytics -
Machine Learning Techniques in Radio Astronomy -
Opening a Window on the Ionised Interstellar Medium of Nearby Galaxies -
Probing cosmic explosions and unveiling extreme astrophysics using rapid-response radio telescopes -
Probing the Environment of the Most Massive Proto-cluster -
Radio Morphology Evolution of Radio Sources at Low Frequency -
Radio Recombination Lines with the MWA -
Real-time Signal Processing and High Time Resolution Science with the MWA and EDA Radio Telescopes -
Searching for Optical Transients with the Desert Fireball Network - Searching for the Most Massive Clusters Around Radio Galaxies
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“The A-Team”: Low-frequency Observations of the Brightest Radio Galaxies in the Southern Sky - Tracing the Evolution of Supermassive Black Holes Across Cosmic Time
- Weighing Proto-clusters in the Early Universe
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Searching for transients and variables in the Galactic and Extragalactic All-Sky MWA (GLEAM) survey