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The Australian Centre for Neutron Scattering Laboratories consists of four laboratories adjacent to the Neutron Guide Hall within the OPAL Neutron Beam Facility.

The Imaging and Medical beamline (IMBL) is a flagship beamline of the Australian Synchrotron built with considerable support from the NHMRC. It is one of only a few of its type, and delivers the world’s widest synchrotron x-ray ‘beam’.

ANSTO is seeking nominations for the ANSTO Australian Synchrotron Stephen Wilkins Thesis Medal.

ANSTO’s Radioanalytical Chemistry (RAC) facility combines techniques in radiochemistry and radiological measurement by alpha spectrometry, gamma-ray spectrometry, and liquid scintillation analysis to deliver radiological assessments.

ANSTO is seeking nominations for the ANSTO Australian Synchrotron Stephen Wilkins Thesis Medal.

The Centre for Accelerator Science provides complementary capabilities to Synchrotron-based and the neutron-based research with the operation of four accelerators, associated beamlines, clean laboratories and in-house expertise in ion beam analysis (IBA) and accelerator mass spectrometry (AMS).

The Scientific Computing team supports researchers by performing numerical simulations that complement experimental research. In particular, we use state-of-the-art software to perform computational quantum mechanical modelling, molecular dynamics simulations, lattice dynamics calculation, data analysis and visualisations.

ANSTO is seeking nominations for the ANSTO Australian Synchrotron Stephen Wilkins Thesis Medal.

Alkane Resources reports Hafnium product breakthrough

An investigation that set out to resolve some of the uncertainty in the sources and quantities of pollutants reaching Antarctica has produced a new experimental technique to identify and characterise recently terrestrially-influenced air reaching Antarctica.

The THz/Far-IR Beamline couples the high brightness and collimation of a bend-magnet synchrotron radiation to a Bruker IFS125HR spectrometer providing high-resolution spectra (0.00096 cm-1) with signal to noise ratio superior to that of thermal sources up to 1350 cm-1 for gas-phase applications; the beamline also delivers signal to noise ratio superior to that of thermal sources up to 350 cm-1 for condensed phase samples.

As a new or returning facility user, there are certain requirements that must be completed in advance to allow you to participate in your planned ANSTO experiment(s).

A lesson in Science and Sustainability.

The Multi-wavelength absorption black carbon instrument MABI can determine the concentration and source of black carbon pollution.

The User Office is the first point of contact for all new and returning facility users accessing ANSTO’s wide range of world-class research infrastructure. These users may be internal ANSTO researchers, external merit researchers, commercial clients, scientific collaborators and partners.

ANSTO’s user office in Melbourne offers access to the Australian Synchrotron, a world-class research facility with over 4,000 user visits per year. ANSTO seeks collaboration and partnerships with research organisations, scientific users and commercial users.