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Home
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About Us
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The Pawsey Centre
Discover Setonix
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Documents Library & Annual Reports
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Supercomputing and Data Processing
Setonix
Nectar Cloud
Data Workflows
Acacia
Banksia
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Analysis and Visualisation
Nebula
Setonix RemoteVis
Visualisation Lab
Remote Virtual Reality
Support & Consultancy
PULSE Collaborations (formerly Uptake Projects)
Support
Pawsey Centre for Extreme Scale Readiness (PaCER)
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The detectability of radio emission from exoplanets
Posted on
September 26, 2019
by
harmonic
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An all-sky survey of circular polarization at 200 MHz
Three-dimensional simulations of neutrino-driven core-collapse supernovae from low-mass single and binary star progenitors
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