March MX User Drop In Zoom Meeting

Mar 17.

MX User Drop In Zoom Meeting

The Diamond Light Source Macromolecular Crystallography group would like to invite all interested users to our second MX User Drop In Zoom Meeting on 17 March 2026. The aim is to provide Diamond MX users with the opportunity to ask questions of our staff, to solve problems, and for us to provide brief updates on the beamlines and software here.

Date
17/03/20262026-03-17T15:00:00
Time
15:00
Location
Diamond Light Source, Oxfordshire, UK
Link
Sign up here

Programme and content

17 March 2026 at 3pm GMT

Featured staff:

  • Mark Williams, Senior Beamline Scientist I03 and ISPyB/Synchweb developer
  • David Aragao, Senior Beamline Scientist I04
  • Ramona Duman, Beamline Scientist I23
  • Sofia Jaho, Beamline Scientist I24
  • Neil Paterson, Senior Beamline Scientist I03
  • Adam Crawshaw, Beamline Scientist VMXm
  • Juan Sanchez-Weatherby, Senior Beamline Scientist, VMXi
  • Amy Thompson, Senior Data Analysis Scientist
  • David Waterman, Scientific Programmer, Dials

Break out rooms will be provided to allow more in depth questions, and data analysis experts from Diamond and elsewhere will be on hand to help solve tricky problems.

Sign up

Please register for this event at the link below. This event is free of charge.

SIGN UP HERE

 

For any queries please contact [email protected]

Diamond Light Source

Diamond Light Source is the UK's national synchrotron science facility, located at the Harwell Science and Innovation Campus in Oxfordshire.

Diamond Light Source Ltd
Diamond House
Harwell Science & Innovation Campus
Didcot
Oxfordshire
OX11 0DE

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Copyright © Diamond Light Source. Diamond Light Source® and the Diamond logo are registered trademarks of Diamond Light Source Ltd

Registered in England and Wales at Diamond House, Harwell Science and Innovation Campus, Didcot, Oxfordshire, OX11 0DE, United Kingdom. Company number: 4375679. VAT number: 287 461 957. Economic Operators Registration and Identification (EORI) number: GB287461957003.

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