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ANSTO provides access to specialised facilities and capabilities by application. Please ensure that you contact the relevant ANSTO scientist for advice before submitting a proposal.

The ANSTO Research Portal is your gateway to submit proposals to access ANSTO's research infrastructure and capabilities in Sydney. Below is a list of ANSTO's selected research capabilities with the relevant local contacts available in the research portal.

Please note that the research capabilities for the Australian Centre for Neutron Scattering and the National Deuteration Facility can be located on their ACNS Customer Portal.

Sydney selections

Accelerators

Group - Radiocarbon dating

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CapabilityContact Scientist(s)
C-14 AMS sample prep & measurement: pre-prepared graphiteGeraldine Jacobsen
Vladimir Levchenko
Andrew Jenkinson
C-14 AMS sample prep & measurement: from CO2 in break sealGeraldine Jacobsen
Vladimir Levchenko
Andrew Jenkinson
C-14 AMS sample prep & measurement: standard treatment - charcoal, shell, bulk sediment, water DIC, water DOCGeraldine Jacobsen
Vladimir Levchenko
Andrew Jenkinson
C-14 AMS sample prep & measurement: complex treatment- bone, pollen, holo/alpha cellulose, method developmentGeraldine Jacobsen
Vladimir Levchenko
Andrew Jenkinson
C-14 AMS sample prep & measurement: samples already pre-treatedGeraldine Jacobsen
Vladimir Levchenko
C-14 AMS sample prep & measurement: raw rock - quartz (in-situ)Reka Fulop
C-14 AMS sample prep & measurement: pure quartz (in-situ)Reka Fulop
AMS data interpretation and consultingVladimir Levchenko
Andrew Jenkinson
Mike Hotchkis
David Child 

Group - Actinide isotopic analysis

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CapabilityContact Scientist(s)
Actinides AMS isotope capability development                                                                                                      Mike Hotchkis
David Child
 U isotopic AMS sample prep & measurement: pre-prepared U3O8 in FeMike Hotchkis
David Child
 U isotopic AMS sample prep & measurement: soil, sediment, biota,  water, swipesMike Hotchkis
David Child
Pu isotopic AMS sample prep & measurement: pre-prepared PuO2 in FeMike Hotchkis
David Child
Pu isotopic AMS sample prep & measurement: soil, sediment, biota,  water, swipesMike Hotchkis
David Child
  U & Pu AMS sample prep & measurement: soil, sediment, biota,  water, swipesMike Hotchkis
David Child
I-129 AMS sample prep & measurement: pre-prepared AgIMike Hotchkis
David Child
I-129 AMS sample prep & measurement: soil, sediment, biota, water,  swipesMike Hotchkis
David Child

Group - Cosmogenic isotope dating

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Capability

Contact Scientist(s)

Be-10 AMS measurement: from pre-prepared Be oxide or Be Hydroxide                                                             Klaus Wilcken
Be-10 AMS measurement only: rock (in situ)Klaus Wilcken
Be-10 AMS measurement only: sediment  (in situ)Klaus Wilcken
Be-10 AMS sample prep only: unprocessed quartz (in situ)Klaus Wilcken
Be-10 AMS sample prep only: pure quartz (in situ)Klaus Wilcken
Be-10 AMS sample prep only: sediment (meteoric)Klaus Wilcken
 Be-10 AMS sample prep only: ice, snow, water, filtersAndrew Smith
Krista Simon
  
Al-26 AMS measurement: from pre-prepared Al oxide or Al hydroxideKlaus Wilcken
Al-26 AMS sample prep only: rock (in situ)Klaus Wilcken
Al-26 AMS sample prep only: sediment (in situ)Klaus Wilcken
Al-26 sample prep only: unprocessed quartz (in situ)Klaus Wilcken
Al-26 sample prep only: pure quartz (in situ)Klaus Wilcken
  
Be-10 & Al-26 sample prep only: rock (in situ)Klaus Wilcken
David Fink
Toshiyuki Fujioka
Be-10 & Al-26 sample prep only: sediment (in situ)Klaus Wilcken
David Fink
Toshiyuki Fujioka
Be-10 & Al-26 sample prep only: unprocessed quartz (in situ)Klaus Wilcken
David Fink
Toshiyuki Fujioka
Be-10 & Al-26 sample prep only: pure quartz (in situ)Klaus Wilcken
David Fink
Toshiyuki Fujioka
  
Cl-36 AMS measurement from pre-prepared AgClKlaus Wilcken
Cl-36 AMS sample prep only: ice, snow, water, filters (meteoric)Klaus Wilcken
Andrew Smith

 

Group- Platinum group elemental analysis

 

CapabilityContact Scientist(s)
PGE AMS measurement: target preparation                                                                                                             Mike Hotchkis
David Child

 

Group - Surface Engineering,  Characterisation & Modification

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Capability

Contact Scientist(s)

ERDA-ToF (Elastic Recoil Detection Analysis - Time of Flight)                                                                                Rainer Siegele
Zeljko Pastuovic
High Energy Heavy Ion Microprobe AnalysisRainer Siegele
Zeljko Pastuovic
Medium energy ion implantation and in-situ depth profilingZeljko Pastuovic
Medium energy and high energy simultaneous ion implantationZeljko Pastuovic
Low energy ion implantation (< 50kV)Mihail Ionescu
Armand Atanacio
High energy ion implantationRainer Siegele 
Zeljko Pastuovic
IBIC (Ion Beam Induced Charge)Rainer Siegele
Radiation damage of materialsRainer Siegele 
Zeljko Pastuovic
2D, PIXE (Particle Induced X-ray Emission spectrometry)Rainer Siegele 
Zeljko Pastuovic

 

Group - Bulk Sample Characterisation & Surface analysis

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Capability

Contact Scientist(s)

PIXE (Particle Induced X-ray Emission spectrometry)                                                                                             Armand Atanacio
PIGE (Proton-Induced Gamma-ray Emission spectrometry)  Armand Atanacio
RBS (Rutherford Back-Scattering spectrometry)Armand Atanacio
PESA (Proton Elastic-Scattering Analysis)Armand Atanacio
ERDA (Elastic Recoil Detection Analysis)Rainer Siegele
Armand Atanacio

 

Group - Aerosol Measurement & Fine Particle Characterisation

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Capability

Contact Scientist(s)

Complete PM2.5 Cyclone sampling unit, rent/year                            Armand Atanacio
IBA particle analysis of filters 2 per week, includes postage and despatch                                                          Armand Atanacio
Black carbon measurements on filtersArmand Atanacio
IBA data interpretation and consultingRainer Siegele
Armand Atanacio
Aerosol facilities technical effortRainer Siegele
Armand Atanacio

 

Isotope tracing

Group - Tritium in surface / groundwaters

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Capability

Contact Scientist(s)

Low Level analysis using LSC (Liquid Scintillation Counter)                                                                                   Robert Chisari

 

Group - Stable isotope ratios of carbon, nitrogen, oxygen, hydrogen

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CapabilityContact Scientist(s)
Stable isotope, delta C13,  C% , delta N15 & N% analyses in solids                                       Robert Chisari
Stable isotope, delta C13 & C% analysis in solidsRobert Chisari
Stable isotope delta N15 & N% analysis in solidsRobert Chisari
Stable isotope, delta C13 analysis in DICRobert Chisari
Carbon concentration determination in DICRobert Chisari
Bone (collagen) samples: collagen extraction prior to delta C13, C%, delta N15 & N% analyses                        Linda Barry
Bone (collagen) samples: N%  for collagen testLinda Barry
Acid treatment of sediments to remove carbonates prior to delta 13C analysisLinda Barry

 Group - Movement of fluids,  particulates and contaminants in aquatic and terrestrial environments 

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Capability

Contact Scientist(s)

Radioisotope tracer techniques                                                                                                                               Cath Hughes

 

Group - Dating of sediment cores using 210Pb

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Capability

Contact Scientist(s)

Pb-210 dating (by alpha spectrometry)                                                                                                                           Atun Zawadzki
Pb-210 dating and Cs-137 (by gamma spectrometry)Atun Zawadzki
Cs-137 dating (by gamma spectrometry)Atun Zawadzki

Group - High resolution image,  radiograph and XRF scan of sediment cores,  wood and other materials

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Capability

Contact Scientist(s)

ITRAX Core Scan at 1000 micron resolution (low) with 10sec exposure for  XRF analysisPatricia Gadd
ITRAX Core Scan at 500 micron resolution (medium) with 10sec  exposure for XRF analysis                                       Patricia Gadd
ITRAX Core Scan at 200 micron resolution (high) with 10sec exposure for  XRF analysisPatricia Gadd
ITRAX Core Scan at 200 micron resolution (high) with X radiograph for  wood samplesPatricia Gadd

 

Group - Grain size distribution determination by laser diffraction method in soil and sediment samples

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Capability

Contact Scientist(s)

Grain Size Analysis                                                                                                                                                             Atun Zawadzki

Group - Radon and thoron analysis and monitoring

 

Capability

Contact Scientist(s)

Continuous in situ radon measurements using portable AlphaGuard detectorsSylvester Werczynski
In situ spot measurements of radon/thoron from rocks and soil using emanometer-flux chamberSylvester Werczynski
Measurement of radon in solids, air, water and mixed phase samplesSylvester Werczynski
Radon surveys/measurements tailored to suit  specific requirementsSylvester Werczynski
Sample-based radon in water via mineral oil extraction and liquid scintillation counting (liquid scintillometer)Robert Chisari

 

Group - Elemental and Trace metal analysis

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CapabilityContact Scientist(s)
Analysis by ICPAES     Henri Wong
Analysis by qICPMS (simple matrices)Henri Wong
Analysis by qICPMS with CRI (for difficult matrices)Henri Wong
Analysis by SeaFast qICPMS (ultratrace Rare Earth Element)                                                                                                        Henri Wong
Analysis by IC (anions)Henri Wong
Physical measurements (pH, Cond, Alkalinity)Henri Wong
Sample Preparation (microwave digestion)Henri Wong

 

Group - Laser ablation - ICPs

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CapabilityContact Scientist(s)
Laser ablation ICPAES     Henri Wong
Laser ablation qICPMS                                                                                                                                                                        Henri Wong

 

Group - Environmental radioactivity measurements

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Capability

Contact Scientist(s)

Low level radioactivity measurements using alpha spectrometry (U  radionuclides)Atun Zawadzki
Low level radioactivity measurements using alpha spectrometry (Th radionuclides)Atun Zawadzki
Low level radioactivity measurements using alpha spectrometry (Pu-  239+240 radionuclides)                                                Atun Zawadzki
Low level radioactivity measurements using alpha spectrometry (Am-241)Atun Zawadzki
Low level radioactivity measurements using alpha spectrometry (Po-210)Atun Zawadzki
Low level radioactivity measurements using alpha spectrometry (Ra-226)Atun Zawadzki
Low level radioactivity measurements using alpha spectrometry (Ra-228  on BaSO4 source)Atun Zawadzki
Low level radioactivity measurements using gamma spectrometryAtun Zawadzki
Low level strontium-90 (Sr-90) measurements using beta spectrometryAtun Zawadzki
Low level lead-210 (Pb-210) measurements using beta spectrometry Atun Zawadzki

Nuclear Stewardship

Group - Nuclear and Ionising Radiation Detection & Dosimetry

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Capability

Contact Scientist(s)

High precision gamma-ray spectrometry                                                                                                                             David Boardman
Dale Prokopovich
GEANT 4 radiation transport modellingDavid Boardman
Dale Prokopovich
Radiation detector characterisationDavid Boardman
Dale Prokopovich

 

Group - Radioanalytical  Chemistry

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Capability

Contact Scientist(s)

Gamma spectrometry (naturals and anthropogenics)Lida Mokhber Shahin
Sangeeth Thiruvoth 
Radioanalytical Chemistry/Alpha Spectrometry/Liquid Scintillation Analysis
(U, Th, Pu or Am isotopes by alpha spectrometry; Sr-90 by liquid scintillation analysis)                    
Tier 1- single elemental analysis
Lida Mokhber Shahin
Sangeeth Thiruvoth
Radioanalytical Chemistry/Alpha Spectrometry/Liquid Scintillation Analysis
(U, Th, Pu or Am isotopes by alpha spectrometry; Sr-90 by liquid scintillation analysis)
Tier 2- double elemental analysis
Lida Mokhber Shahin
Sangeeth Thiruvoth 
Radioanalytical Chemistry/Alpha Spectrometry/Liquid Scintillation Analysis
(U, Th, Pu or Am isotopes by alpha spectrometry; Sr-90 by liquid scintillation analysis)
Tier 3- triple elemental analysis
Lida Mokhber Shahin
Sangeeth Thiruvoth
Radioanalytical Chemistry/Alpha Spectrometry/Liquid Scintillation Analysis
(U, Th, Pu or Am isotopes by alpha spectrometry; Sr-90 by liquid scintillation analysis)
Tier 4- quadruple elemental analysis
Lida Mokhber Shahin
Sangeeth Thiruvoth 
Radioanalytical Chemistry/Alpha Spectrometry/Liquid Scintillation Analysis
(U, Th, Pu or Am isotopes by alpha spectrometry; Sr-90 by liquid scintillation analysis)
Tier 5- full suite actinide analysis and Sr-90
Lida Mokhber Shahin
Sangeeth Thiruvoth 
Radioanalytical Chemistry/Liquid Scintillation Analysis (Tritium)
Tier 1 -  tritium on freshwater and leachate
Lida Mokhber Shahin
Sangeeth Thiruvoth 
Potentiometric measurements - automated; pH static and dynamic  titrationsSangeeth Thiruvoth  
Josick Comarmond
Potentiometric measurements - automated; Isotope reversibility studySangeeth Thiruvoth  
Josick Comarmond
Determination of the distribution of contaminant between aqueous phase  and geomedia.
Distribution coefficient (Kd) determination using batch sorption methods
Sangeeth Thiruvoth  
Josick Comarmond
Measurement of zeta potential and particle size of concentrated colloidal  suspensions;
Zeta potential and particle size determination
Sangeeth Thiruvoth  
Josick Comarmond
Radioanalytical chemical method development (alpha and/or beta  emitters)Sangeeth Thiruvoth  

 

Radioisotopes and Radiotracers

Group - Neutron Irradiation

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CapabilityContact Scientist(s)
OPAL low flux pneumatic irradiation facility                                                                                                                          Attila Stopic
OPAL medium flux pneumatic irradiation facilityAttila Stopic
OPAL high flux pneumatic irradiation facilityAttila Stopic
OPAL short residence pneumatic irradiation facilityAttila Stopic

 

Group - Elemental Analysis

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CapabilityContact Scientist(s)
NAA Short Irradiation                                                                                                                                                                 Attila Stopic
NAA Medium IrradiationAttila Stopic
NAA Long IrradiationAttila Stopic
DNAAAttila Stopic

Group - Radioisotope Provision

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CapabilityContact Scientist(s)
Medical Radioisotopes                                                                                                                                                                Ivan Greguric
Paul Pellegrini
Leena Hogan
Environmental and Industrial RadioisotopesIvan Greguric
Paul Pellegrini
Leena Hogan

 

Group - Radioisotope Development

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CapabilityContact Scientist(s)
Radioisotope Handling and Separations                                                                                                                                    Ivan Greguric
Paul Pellegrini
Leena Hogan
Reactor Target ProcessingIvan Greguric
Paul Pellegrini
Leena Hogan

Group - Radiotracer Production

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CapabilityContact Scientist(s)
Radiotracer production for pre-clinical research                                                                                                                        Tien Pham
Nigel Lengkeek
Ivan Greguric 
Radiotracer production for clinical researchTien Pham
Nigel Lengkeek
Ivan Greguric 

Group - Radiotracer Development

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CapabilityContact Scientist(s)
Radiochemistry Development                                                                                                                                                        Nigel Lengkeek
Tien Pham
Ivan Greguric
Radiotracer MethodsNigel Lengkeek
Tien Pham
Ivan Greguric
Translation of Radiotracers for Clinical ResearchNigel Lengkeek
Tien Pham
Ivan Greguric
Radiopharmaceutical DevelopmentNigel Lengkeek
Tien Pham
Ivan Greguric

 

Group - Radiochemistry Automation

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CapabilityContact Scientist(s)
Radiochemistry Automation                                                                                                                                                        Gary Perkins
Tien Pham
Ivan Greguric 

 

Group - Radioanalytical Measurement

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CapabilityContact Scientist(s)
Radioanalytical Measurement                                                                                                                                                     Ivan Greguric 
Radiobiology & Bioimaging

Group - Radiobiology​​​​​

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CapabilityContact Scientist(s)
Radiobiology                                                                                                                                                                 Nick Howell

Group - Vivarium

CapabilityContact Scientist(s)
Animal House and Holding Facilities                                                                                                                                       ANSTO Biological Facilities
Aquatic MonitoringANSTO Biological Facilities
GreenhouseANSTO Biological Facilities

 

Group - In Vivo Studies

CapabilityContact Scientist(s)
Functional Imaging: PET/CT                                                                                                                                                       Arvind Parmar
Andrew Arthur
David Zahra
Functional Imaging: SPECT/CT Arvind Parmar
Andrew Arthur
David Zahra
Functional Imaging: PET/SPECT/CT Arvind Parmar
Andrew Arthur
David Zahra
Structural Imaging: MicroCT ImagingDavid Zahra
Biodistribution/ Blocking studiesArvind Parmar
Mitra Safavi-Naeini
David Zahra
Imaging QuantificationDavid Zahra
Mitra Safavi-Naeini

Group - In Vitro Studies

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CapabilityContact Scientist(s)
Receptor autoradiography                                                                                                                                                        Michelle Cielesh
Receptor binding assayArvind Parmar
Histological and immunochemical staining Arvind Parmar

Group - Radiotracer characterisation

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CapabilityContact Scientist(s)
Radioligand uptake                                                                                                                                                                  Arvind Parmar 
Radioligand bindingArvind Parmar
In vitro metabolism    Gita Rahardjo

 

Group - Gamma Irradiation

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CapabilityContact Scientist(s)
High dose gamma irradiation                                                                                                                                                 Justin Davies
Deuteration

Chemical Deuteration

Capabilities

Contact Scientist(s)

Saturated diacids and bifunctional surface active
molecules

Professor Peter Holden
or Dr Tamim Darwish
via ndf-enquiries@ansto.gov.au

Unsaturated fatty acids (e.g. oleic acid)

As above

Lipids including glycerides; phospholipids (e.g.DOPC
and POPC); and selective deuteration of lipids (head
deuterated, tail deuterated and fully deuterated)

As above

Sugars

As above

Membrane protein detergents (e.g. DDM and OG)

As above

Deuterated surfactants including ionic and non-ionic

As above

Deuterated silanes

As above

Glyme and glycol ethers

As above

Aromatics and heterocyclics for MOFs

As above

Compounds for organic light emitting diodes

As above

Compounds for solar cells

As above

Electrolytes for batteries

As above

Selective deuteration of small molecules 

As above

Cholesterol

As above

 

Deuteration - Biological

 

Capability

Contact Scientist(s)

Double (2H/15N, 13C/15N) and triple labelled
recombinant proteins  (2H/13C/15N)

Professor Peter Holden
or Dr Tamim Darwish
via ndf-enquiries@ansto.gov.au

Partial and perdeuterated recombinant proteins

As above

Selectively labelled recombinant proteins

As above

DNA

As above

Biopolymers – cellulose, chitosan, chitin, PHAs

As above

 

 

Beamlines at the Australian Synchrotron 

The Australian Synchrotron Portal is your gateway to submit proposals to access Melbourne infrastructure and capabilities. Below is a list of our beamline capabilities and their local contacts.

Imaging and Medical

Beamline contact

Email: IMBL@synchrotron.org.au

Phone: +61 3 8540 4162

Fax: +61 3 8540 4200

IMBL IS OFFERING THE FOLLOWING 3 OPERATING MODES:

  • 2-Dimensional imaging of live animals, and 3-Dimensional imaging of materials in hutch 3B
  • Fast computed tomography (CT) of small objects in hutch 2B
  • Micro-beam radiation therapy (MRT) in hutches 1B and hutch 2B

PREPARING FOR BEAMTIME APPLICATIONS

For information on how to prepare your application and more detail on the available options refer to the Beamtime on this beamline (IMBL) information page.

ANIMAL ETHICS

For experiments using live animals first read the guidance provided.
Animal ethics procedures must be addressed well in advance of submission of the beamtime proposal.

Infrared Microscope

Beamline Contact: 

irm@synchrotron.org.au

Transmission measurements
•    For transmission FTIR microanalysis of thin samples we strongly recommend that your samples are mounted on IR transmitting windows such as CaF2 (cut-off 50 %T at 900 cm-1 for 0.5 mm thick window), BaF2 (cut-off 50 %T at 750 cm-1 for 0.5 mm thick window), or ZnSe (cut-off 50 %T at 500 cm-1 for 0.5 mm thick window).  We do not recommend the use of IR reflective slides, such as Kevley slides, for “transflectance” measurements.
•    A limited supply of windows of various dimensions is kept at the beamline, but we recommend purchasing your own windows to enable you to prepare your samples prior to your beamtime.  Further information on the material properties, and availability, of a wide range of window materials is available on the website of Crystran Ltd http://www.crystran.co.uk/
•    For thin sectioning of samples, a microtome is available on-site for use during your beamtime.  HOWEVER we strongly recommend that any sectioning required is performed before your beamtime to save time while you are at the beamline.  Please contact the beamline staff for advice on sample thickness and sample preparation.
•    A microcompression cell is available with diamond windows for flattening of sample sections, or crushing of harder materials. 

Micro ATR measurements
•    A micro ATR objective is available for use and can be used for ATR mapping of sample surfaces and embedded materials. Two germanium crystal sizes (100 µm and 250 µm diameter) are available for hard and less hard materials respectively.  The sample surface must be polished or microtomed flat (to approximately 1-5 µm roughness, depending on hardness) to ensure good optical contact between the ATR crystal and your sample. Please indicate in your proposal if this is required.
•    For ATR spectroscopy of soft samples (e.g. biological materials or lipid coatings) please contact the beamline staff to discuss your requirements as the conventional micro ATR objective will probably produce too much force for analysis of our materials.

Grazing angle studies of surfaces
•    A Grazing Angle Objective (GAO) is currently available and is suitable for the study of thin coatings on reflective metallic surfaces. Contact beamline staff for more details if this is required.  Lateral resolution with the GAO is approximately 20 µm.

Sample heating stage
•    A Linkam heated sample stage is available for use.  This can cool samples to close to liquid nitrogen temperature and heat to 600 °C.  As a longer working distance is required to accommodate the Linkam stage, the 15x objective used with this device will give a reduced lateral resolution of approximately 10 µm Contact beamline staff for more details if this is required.

Live biological samples
•    Sample chambers dedicated to the study of live cells in a liquid environment have been developed by the IR beamline staff, and are under continued development. These are suitable for both static (approximate hold time of 30 minutes) and continuous flow conditions.  The use of CaF2 windows in our liquid cells currently limits the spectral range available to approximately 1000 cm-1.  
•    Class II containment facilities are available within the Biochemistry support laboratory for the preparation of cell cultures. Users requiring access to this facility should contact IR beamline staff prior to submitting a proposal.

Off-line Focal Plane Array IR microscope
•    The off-line Focal Plane Array FTIR microscope is currently available for booking in conjunction with your beamtime proposals, if successful. Contact beamline staff if this is required.
 

THz / Far-IR

Beamline Contact: 

farir@synchrotron.org.au

Please contact the THz/Far-IR beamline staff if you wish to use any of these instruments or if you would like to discuss a potential experiment.

The following instruments are available to users from May 2015:

Gas-phase

  • An Enclosive Flow Cooling (EFC) cell with multipass optics is available for the study of gases & molecular clusters at cryogenic temperatures. The EFC cell is generally operated at temperatures ranging from79-300 K, but can also be operated with liquid helium. The cell can be equipped with TPX, PE, or KBr windows offering spectral coverage from 10-4000 cm-1; with a base optical path length of 0.65 m, it can achieve path lengths up to 27 m.
  • 2 room temperature multipass glass gas-cells: one of them can be coupled to furnace for the study of short-lived molecules, and can offer a path length up to 20 m, while the other designated for non-reactive gases can offer up to 30 m in path length.
  • A 10 cm single pass gas-cell designed to mix gases in-situ

 Condensed-phase

  • A Janis ST-100 cryostat to study solid homogeneous samples in transmission down to 77 K.
  • A Cryo Industries of America closed-loop pulse tube (CLPT) cryostat to study solid homogeneous samples in transmission down to 6.3 K.
  • A Grazing Incidence Angle (30-80 ̊) (GIA) accessory that is ideal for the study of thin samples or surfaces at grazing angles at room temperature
  • A Near-Normal Incident (11̊) Transmission/Reflection Optics (N2ITRO) accessory ideal for the study of optical properties of materials; it can be equipped with a far-ir polarizer.

 

The following instruments are offered to expert users only:

Gas-phase

  • A room-temperature 15 cm  multipass gas-cell coupled to a 25W CO2 laser operating at 10.6 μm, or a 4.8 W Ar ion laser operating at 1064 nm, 532 nm, 355, nm and 266 nm to generate short-lived molecules by photolysis, and can offer path lengths up to 3 m.
  • A furnace to generate short-lived species by pyrolysis that can be coupled to the EFC cell

 Condensed-phase

  • A Linkam based furnace for the study of solids up to 1000 K; it can also be coupled to the N2ITRO setup.
  • A vacuum-proof cell for qualitative and quantitative analysis of liquid samples; the cell is equipped with polyethylene, and spacers ranging from 6-250 microns.

 

Future capabilities:

Condensed-phase

  • A Grazing Incidence Angle optical setup combined with the ST-100 cryostat for the study of thin samples or surfaces at grazing angle at low-temperatures
  • Diamond Anvil Cell
  • Laser excitation using a 25W CO2 laser operating at 10.6 µm, or a 4.8 W Ar ion laser operating at 1064 nm, 532 nm and 266 nm to generate short-lived molecules or to induce chemical changes by photolysis

 

Macromolecular Crystallography

Beamline Contact: 

mx@synchrotron.org.au

MX1: MACROMOLECULAR CRYSTALLOGRAPHY BEAMLINE

  • Energy range from 5.5 - 18 keV
  • User changeable energy from 8.5 to 17.5 keV
  • Fluorescence scans for MAD and metal identification
  • UV laser for radiation damage induced phasing
  • Robotic loading and remote access
  • Rapid access is available

MX2: MICRO CRYSTALLOGRAPHY BEAMLINE

  • Energy range from 4.8 - 20.0 keV
  • User changeable energy from 8.5 to 15.5 keV
  • Microfocus beam with FWHM of 25x15 microns (HxV)
  • Beamline operating modes: channel cut (fixed energy at 13 keV) and double crystal
  • High flux with up to 3e12 ph/s/mm2 in the focussed beam
  • Fluorescence scans for MAD and metal identification
  • User-changeable micro-collimator with 20, 10, and 7.5 micron apertures
  • Robotic loading and remote access
  • Rapid access is available

 

Powder Diffraction

Beamline Contact:

powder.diffraction@synchrotron.org.au

PROPOSAL PREPARATION

  • Users can find tips on proposal preparation under Beamtime on this beamline on the powder diffraction beamlines' webpage.
  • Proposers interested in performing total scattering experiments should consult the Total Scattering Analysis page and prepare their proposal accordingly.
  • All proposals must be accompanied by evidence of previous diffraction measurements; i.e. a laboratory or synchrotron powder diffraction pattern that is indicative of the data obtained from the sample(s) of interest.
  • Experiments at high pressure are complex and users new to the technique should contact beamline staff before submitting their proposals

DETECTORS

The detectors which are currently available are:

  • Mythen microstrip
  • MAR345 image plate
  • MAR165 CCD

ANCILLARIES

  • Details of the ancillaries available at the beamline can be found under Sample stages and Environments.
  • Users should, as much as possible, select all of the appropriate ancillaries for their proposed experiment using the list of options within the portal
  • Note that users seeking to use their own sample stage and/or ancillaries should discuss this in advance with the powder diffraction beamline staff AND provide drawings of the equipment to show how it is anticipated that this equipment will fit at the end station
  • Available for experiments are:
    • Cryostream (80 - 450 K)
    • Hot-air blower (100 - 950 °C)
    • Anton Paar HTK 2000 strip furnace (25 - 1600 °C)
    • Anton Paar DHS-1100 domed furnace (25 - 1100 °C)
    • STOE capillary furnace (25 - 1350 °C)
    • Gas/vacuum flow cell for capillary samples
    • High-throughput stage
    • Cryostat for samples in transmission geometry (10 - 300 K)
    • Diamond Anvil Cell (DAC) at ambient temperature only
    • Single battery holder
    • Multiple battery cell carousel

BEAMLINE CONSUMABLES

The typical consumables required for most experiments on the Powder Diffraction beamline are listed below.

Capillary experiments

  • Quartz and borosilicate capillaries can be purchased from Hilgenberg. Remember to allow plenty of time to order your capillaries as the beamline does not provide them.
  • For experiments requiring pressures: 5 - 10 bar, quartz capillaries with a wall thickness of 0.02 mm are required.
  • For experiments requiring pressures: 10 – 20 bar, quartz capillaries with a wall thickness of 0.05 mm are required.
  • Sapphire capillaries are required for experiments using the capillary furnace for temperatures >1100°C and those experiments requiring pressures greater than 2 MPa (20 bar).
  • For experiments using the Norby or capillary flow cell, graphite Supelco M2-A ferrules are also required and can be obtained from here.

Anton Paar furnace experiments

  • Anton Paar furnace experiments requiring either platinum or tungsten heating strips must be supplied by Users.
  • The heating strips can be purchased from Anton Paar, see here for more details.
  • For experiments requiring temperatures 900°C or less, inconel heating strips may be used and are available for Users.

High pressure Diamond Anvil Cell (DAC) experiments

For experiments at pressures >10 GPa users will need to provide their own diamonds and seats. They can be purchased from: https://www.diamondanvils.com/ or http://www.almax-industries.com/ . Users must consult beamline staff for more information before purchasing.

NOTE: DAC experiments require a significant amount of beamline endstation set-up and it is recommended that 8-10 hours be included in the timing calculations for relevant proposals.

HIGH PRESSURE AND TEMPERATURE CONDITIONS AVAILABLE AT THE POWDER DIFFRACTION BEAMLINE

Capillary Flow Cell Experiments

The maximum pressure at the beamline in a capillary is 2 MPa (thick-walled capillaries required as above) unless prior agreement is reached with beamline staff prior to proposal submission.
For experiments which use > 5% Hydrogen gas, the maximum temperature which can be used is 500°C.

Capillary Furnace Experiments

The maximum operating temperature is 1100°C for quartz capillaries
The maximum operating temperature is 1350°C for sapphire capillaries.

 

Soft X-ray Spectroscopy

Beamline Contact:

softxray@synchrotron.org.au  

The beamline scientists of the soft x-ray beamline are very happy to hear directly from potential users and we would urge you if you would like to perform an experiment on this beamline to email or telephone us directly. For information, the beamline contact address below sends your email to all three beamline scientists.

  • The beamline continues to operate well, and recent tests with the undulator mean we can now offer the potential of rotating the linear polarisation of the x-ray beam. For small samples this offers an easier method of making a polarisation analysis than by rotating the sample.

The beamline has new thermal evaporation sources. One source is optimised for organic evaporants in the temperature range from 50 to 300°C. The other is optimised for 200-800°C, but can operate to 1100°C with a suitable crucible. The beamline would prefer to offer these systems to users who wish to thermally evaporate material. A higher temperature evaporator, to 1400°C, may also be available. Further information on source specifications can be found in the beamline technical pages. We have a supply of crucibles available which we will exchange for each new evaporant. We are happy to support users who wish to use the full in situ surface science capabilities of the beamline. We are also happy to discuss how we can extend our capabilities, but we cannot guarantee that we will be able to do this in every case.

A new 4 point probe for measuring the surface conductivity of samples in UHV has been installed and tested in the preparation chamber. This is a specialist device that can be useful for a limited range of experiments. As an experimenter you will probably have knowledge of the information that can be obtained using such a device. If this would be useful as an adjunct to your experiment please contact us to discuss its use during your experiment. We are not offering this device as a general part of the user environment.

 

Small and Wide Angle X-ray Scattering

Beamline Contact: 

saxswaxs@synchrotron.org.au

One to Two Shift Access for Protein Solution Scattering
The SAXS/WAXS beamline is now able to support a limited number per cycle of 1 or 2 shift experiments for protein solution scattering. This option is aimed at:

  • encouraging, facilitating and training new Users of SAXS who don’t need a full 24 hours of beamtime, but have a strong case for synchrotron solution SAXS time. For new protein Users experiments, you can now apply for a one shift experiment which would be run during the day and have close staffing support to help train you to run the beamline and help start you on basic data processing and analysis.
  • experienced groups who need 1-2 shifts of beamtime to complete a previous experiment, particularly if anticipated to complete a publication or a piece of research. In such cases, experiments would most likely commence at 4pm and run overnight, hence previous experience running the beamline is essential.

Please note there are some key technical and operational constraints needed to make short access experiments feasible:

 

  • Short access (less than 24 hours) is only available for solution scattering experiments given its well established and fixed experimental setup. The wide variety and custom requirements of many materials science measurements is not suited to allocations under 24 hours.
  • Only a 2.68 m camera length at 12 keV will be available, and no camera length changes would be allowed. This covers 0.006 to 0.35 Å-1and suits the majority of proteins from ~ 10 to 300 kDa (smaller for highly extended proteins). This standard setup would normally be ready to use at the start of beamtime with a minimum of setup and delay.
  • Both autoloaded static samples (50 – 100 microlitres), and size exclusion chromatography will be available. If you are using SEC, we recommend you pre-equilibrate your column(s).
  • For experiments commencing at 4pm, the Experiment Spokesperson must be an experienced User of the beamline, able to run the beamline and lead their experiment group without training from the beamline staff. We need to know who your spokesperson is likely to be in the proposal, and will require this information in the Detailed Experiment form in order to approve the experiment.
  • The number of people provided travel support by AS may be less than 3.
  • Short access experiments would be submitted, reviewed and scheduled at the same time and through the same process all other proposals. This is not a rapid access scheme.
  • For evening starts, consider arriving early to potentially equilibrate columns on site, and/or prepare and configure plates ready for analysis.

Guidance for Proposals

Short access proposal go through the same submission and review system as all other proposals, and uses exactly the same online form as all other proposals (i.e. there is no special form for short-access proposals), experiments.

  • Just indicate the number of shifts (of 8 hours each) you estimate you need. If this is less than 3 shifts, this automatically identifies it to the review process as a short request.
  • In the proposal (for example in the track record section) describe whether you are new to SAXS and therefore need to be scheduled from 8 am. If you are an experienced User and able to make use of 4pm -8 am scheduling, you will need to declare who will be the likely on-site experiment spokesperson to lead the experiment.

The short access scheme for proteins is not a substitute for laboratory SAXS. As for all protein experiment proposals, make sure you explain why synchrotron SAXS is needed rather than a laboratory SAXS instrument. We strongly advise you provide evidence that samples have been adequately screened/characterised as suitable for synchrotron SAXS (e.g. include basic data in the Figures section such as gels, SEC traces, light scattering, AUC etc.).

The number of short experiments allocated in a cycle will depend on the ranking of review scores, and the capacity of the beamline to sustainably support more experiments amongst already busy operations. We envisage trialling this access pathway on a small scale to assess the impact on scientific output (i.e. will this prove a productive mode of access), its impact on staffing, and the potential impact on experienced Users running 2-shift experiments starting in the evening.

 

Minibeam: A New Capability
Until recently the beamline has had a very limited ability to produce a beam at the sample position significantly smaller than its focal size (which is currently ~250 x 120 micron H/V FWHM). This has been a fundamental aspect of the optical design of the beamline which is designed to convert the storage ring properties for low-q SAXS (0.001Å-1 at 8 keV), which generally mandates a moderate beamsize. The main slit layout has been optimised for low-q performance, so normally the beamsize defined by the focal properties of the beamline. 
In April 2015, an additional slit was installed on the beamline not far from the focal point. The original low-q capability of the beamline is still available and will remain the standard setup for general SAXS use. However, the new slits add the option to produce small beams well below the focal size still to quite low q (with some constraints about camera length and photon energy described below). The final guard slit is able to control slit scattering to produce good q-minimum ranges, albeit with limitations due to the much shorter collimation length than the standard setup. Because this is done with slits rather than additional or upgraded focussing, which is considerably more expensive and an intended longer term upgrade, there is significantly less flux than the full beam. However, it may still be adequate flux for your needs, especially if you are not particularly limited by exposure time. These new slits allow better definition of small beams when required, with much more flux than was previously possible.

 

 

Percentage of full flux vs approximate full width size (µm) for minibeam setup. Area shaded darker grey with bold text are maximum limits for 7m camera and can only be used at 12-18 keV. Area shaded lighter grey with underlined text can are maximum limits for 3.3 m camera and can be used at any energy. Larger settings (white, plain text) can be used at 1.5 m or shorter camera lengths at any energy. Settings smaller than maximum for each camera length can always be used. Please note exact beam sizes below 50 µm are quite approximate and have not yet been measured in detail. Also, please note these numbers are currently full width sizes rather than full-width at half maximum because more characterisation of minibeam is still required.

 

Applications of minbeam mode
The most obvious applications of small beam modes are:

  • Analysis or rastering of heterogeneous samples at higher spatial resolutions (e.g. 50 micron spatial resolution)
  • Small samples, such as fibres. By limiting the beam size in one direction (e.g. vertical) to size of fibre you can increase signal:noise.
  • Grazing incidence, to help control the footprint of the beam within the length of the specimen
  • Smaller capillaries and microfluidics. Not only can the size of the bright part of the beam be constrained, so can the width of the background intensity that affects the minimum working diameter of capillaries. It should be straightforward to use 0.5 mm capillaries where desired (however this reduces sample scattering power and sample:glass thickness ratio).
X-ray Absorption Spectroscopy

Beamline contact:

  • We need you to contact us before you submit any non-standard (Hutch C) experiment proposal, or if you have not used the XAS beamline before. Please contact us via xas@synchrotron.org.au

OVERVIEW

  • The available energy range is 5 - 31 keV via the following operational modes:

Mode 1*: 5 - 9 keV using Si(111)

Mode 2: 8.5 - 18.5 keV using Si(111)

Mode 3: 15 - 31 keV using Si(311)

*Note that in Hutch C the lowest accessible energy is 7 keV (Fe K edge)

 

PROPOSAL GUIDELINES

  • proposal guidelines document has been prepared by the Proposal Advisory Committee (PAC) and the beamline team. Please read these guideliens carefully and follow them diligently as they give important information on how to write a sound proposal for access to the XAS beamline. Failure to follow the guidelines makes it difficult for the PAC and beamline scientists to assess the viability of an experiment, thus likely rendering a proposal less competitive.
  • Proposals will necessarily be grouped together based on their energy range / operational mode and each proposal will only be allocated time for a SINGLE mode. If you need access to more than one beamline mode, please submit TWO separate proposals, one for each mode, and indicate that they are linked.
  • For fluorescence measurements an estimate of the absorber concentration is needed to assess feasibility. Typical scan times are 20 minutes for XANES and 45 minutes for EXAFS.

EXPERIMENTAL ENVIRONMENTS

  • Standard experiments, that is where samples are mounted using standard sample holders and analysed at room temperature or in the He cryostat at 10K, are available in the first experimental station (Hutch B). Hutch B has 3 ion chambers and a 100 element Ge fluorescence detector. The setup in this end station is fixed and cannot be modified.
  • Non-standard experiments are run in the second experimental station (Hutch C). Hutch C is currently available for transmission type experiments, e.g. for in-situ heater work. You need to contact the beamline team BEFORE you submit a proposal that seeks access to Hutch C. Please note that the lowest accessible energy in Hutch C is the Fe K-edge at 7 keV.
  • Fast shutter, soller slits, and filters are available in Hutch B for fluorescence experiments.
  • A sample cryostat is available for use in Hutch B. Although the cryostat is vibration-less, as a matter of good XAS practice, samples always need to be prepared as homogeneously as possible in order to promote good spectral results.
  • The fluorescence detector readout time (overhead) is about 1 s per point.
  • We also have a PIPS fluorescence detector, which can be useful for certain experiments. This type of detector is not energy resolving and can be used for non-complex samples where the concentration of the element of interest is around a few 1000s ppm.

 

    X-ray Fluorescence Microscopy

    Beamline contact: 

    If your experiment requires other capabilities, please contact the beamline scientists prior to submitting your proposal.
    Proposals that do not fit within these capabilities may still be considered for beamtime at the discretion of the PAC.
    Please contact beamline scientists to discuss your particular sample mounting requirements.
    Beamline Contact: xfm@synchrotron.org.au

    BEAMLINE

    Incident energy range: 4.2 to ~22 keV
    Incident energy resolution: DeltaE/E = 10-4

    MICROPROBES

    KB mirror microprobe: ~1 μm focal spot. Stage range 100 mm * 100 mm.  Can be used with Vortex or Maia detector

    Cryostream  Contact Martin de Jonge to discuss if interested.

    Fast stages and tomography available in 2017. Contact Martin de Jonge to discuss

    'Milliprobe' / large area scanner  Beam is defined by the exit silt, and so typical resolution is 200-μm. Capable of scanning objects of order 600-mm by 1200-mm, principally artworks. With some effort (and call for need) could be used for mapping western-blots simultaneously with the use of the microprobes. Contact Daryl Howard to discuss if interested.

    DETECTORS

    Vortex: silicon drift diode detector. Detector orientation: 90-degree. Energy sensitivity above 1.6 keV; energy resolution ~140 eV. Typical dwell 0.2-2 sec/pixel. 

    Maia: 384-element silicon array detector for on-the-fly acquisition in 180 degree ‘backscatter’ geometry.  Energy resolution ~275 eV. Typical dwell 0.5-50 msec/pixel. Default operation is on KB mirror microprobe. While this detector is extremely reliable, it is a research detector and so we do not carry a complete spare. As such, it is available on a best-effort basis: every experiment should anticipate using the Vortex detector as a back up if required.

    UPDATE: Maia Rev C available. Able to map S (~2.2 keV), and P (~2 keV). Helium or nitrogen (argon exclusion) environment is available with concomitant smaller scan area.

    DPC: segmented photodiode detector for differential phase contrast in transmission. Can be used with the KB microprobe.

    Transmission: Ion chambers and photodiodes
    On axis, in-line optical microscope with ~1-2 μm resolution, 700 μm field-of-view. Backside viewing only.

    MODES OF OPERATION

    SFXM Scanning Fluorescence X-ray Microscopy

    2D elemental mapping of fluorescence emission in the range 1.6 keV to ~22 keV (Vortex detector) or 1.6 keV to 19.5 keV (Maia detector).

    Micro-XANES - spatially resolved x-ray fluorescence near edge spectroscopy

    Single point XANES from 4.2 keV to ~22 keV (Sc to Ru, and L-edges falling within this energy range) using the Vortex detector. Stack XANES / imaging XANES from 4.2 keV to 19.5 keV covering modest areas using the Maia detector.
    High monochromaticity XANES (311 crystal) is available - potential users should contact David Paterson to discuss their proposed study.

    STXM Scanning Transmission X-ray Microscopy

    Fast transmission maps (absorption and differential phase contrast) with incident energy range from 4.2 keV to ~22 keV

    Fluorescence tomography

    Single-slice (2-D) or volumetric (3-D) tomography on the KB microprobe is well established - ultimate resolution around 2-5 μm.  Specimen diameter must be small enough to avoid self-absorption (for a discussion of self absorption, see de Jonge & Vogt, Current Opinion in Structural Biology 20 (2010)).  Typical specimen size is 150 μm diameter, up to 1-mm long.

    Potential tomography users should contact Martin de Jonge to discuss their proposed study.