Group2: Difference between revisions
From canSAS
No edit summary |
No edit summary |
||
| Line 3: | Line 3: | ||
Brian Pauw Leading | Brian Pauw 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? | * 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 | * 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 | * Data repositories and data mining – making dark data useful and getting more bang for the buck on expensive facilities | ||
Revision as of 21:46, 5 June 2017
NOTES FOR GROUP B
Brian Pauw 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
