Chemical Crystallography - Remote robot collection

 

Background - Why use the robot?

Advantages of remote access robot mounting:

  • Convenience – no need to travel.

  • Easier to split shift between more people.

  • Pre-mounting crystals can save precious beamtime.

  • Very reactive crystals can be mounted in a fume hood in your lab.

  • Some crystals can crack, shatter, or degrade in quality when transported by air or road to get to the synchrotron.

  • Faster – no need to lock up hutch every time, wait for detector to move etc.

  • Good for standard crystallography

When to still handmount crystals:

  • Non-standard experiments

  • Very difficult crystals, where you may need to mount 10-20 crystals and base mounting decisions on diffraction data.

  • Using synchrotron equipment to mount (cold-mount, humidity control, gases etc.)

  • When you need advice and assistance from beamline staff.

Background - Introduction to the AS pucks and tools

This video is from when the Australian Synchrotron pucks were first introduced. Enjoy the music!

https://www.youtube.com/watch?v=EJltEp-nb0M

Sample handling at the Synchrotron

Watch below for how your pucks are loaded into puck adapters to be transferred to the robot dewar. Make sure you turn on captions.

Even more fun videos of how the robot works!

 

Before your beamtime

Mounting and cryo-cooling crystals

 

You can use this handy puck tracking sheet for keeping track of which crystal goes in each port.

 

Workflow

Relevant User Interfaces

Step 0: Experimental setup

For chemical crystallography collections, there are a few things you should check before starting to collect:

Step 1: Log on remotely

Log on to the Remote access pages for the beamlines. It is recommended to have more than one monitor.

Make sure you open the connection labelled with AXDV before you open ADXV for viewing your diffraction.

Step 2: Mount a crystal

Use the robot webpage to select the samples you want to mount. See Robot mounting and user interface for detailed instructions.

Step 3: Rastering

If you can’t find your crystal on the loop, use Rastering to find it by diffraction. Skip this step if you can see your crystal. Rastering is not really necessary on MX1 since the beam is very large.

 

Step 4: Screening

Collect a small wedge of data to see if the crystals are worth collecting, instructions: Screening

Step 5: Strategy

Use the results from screening to calculate the optimum Strategy for your collection.

Step 6: Collect dataset

Collect your perfect and beautiful Collecting a Dataset

Step 7: View processing results and solution

Check your results and decide if you want to collect again for higher quality data or to achieve more data. Data Processing

This can be done via the data processing webpage, but to find more information, you will want to view the initial solution, which is in the CXASAP-Brute folder in the folder for your dataset. See CX - accessing and analysing data on the beamline CX - accessing and analysing data on the beamlinefor how to find your data and CXASAP on MX for information on how to find your CXASAP results.

Later steps

Prepare your structure for publication

  • Import the relevant synchrotron information into your cif, from the autoprocess.cif file generated for each dataset: CIF file entries

  • Reference the synchrotron and relevant software: Publishing MX data

 

 

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