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NOTES FOR GROUP B | |||
Joe Kline Leading | |||
=== Top Thoughts for Going Forward === | |||
* Standard sample – large interest in q-resolution standard. Also a combined q and intensity standard. How to make it work across many instruments/energy? | |||
* Propagation of uncertainty – software propagation (black box packages), accounting for modeling uncertainties, and potential round robin to compare fitting results from different groups | |||
* Data repositories and data mining – making dark data useful and getting more bang for the buck on expensive facilities | |||
Latest revision as of 23:00, 8 June 2017
NOTES FOR GROUP B
Joe Kline Leading
Top Thoughts for Going Forward
- Standard sample – large interest in q-resolution standard. Also a combined q and intensity standard. How to make it work across many instruments/energy?
- Propagation of uncertainty – software propagation (black box packages), accounting for modeling uncertainties, and potential round robin to compare fitting results from different groups
- Data repositories and data mining – making dark data useful and getting more bang for the buck on expensive facilities
