Difference between revisions of "TransverseAnalysisMeeting June 2 2020"
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== Agenda == | == Agenda == | ||
| − | # CREX AT runs update: Weibin & Robert | + | # CREX AT runs update: Weibin & Robert [http://ace.phys.virginia.edu/HAPPEX/4120 haplog4120] |
| − | #* | + | #* WZ: for the dpp i have the mean and RMS |
| − | # PREX2 AT runs update: Ryan | + | #* KK: it's important to see the tails (5-10 sigma away) and log plots |
| − | #* | + | #* KK: for the narrow peak we should look into detail (vs event number) |
| + | #* Ryan: started looking at the form factors. At 2GeV the C fraction is much larger than at 1GeV. 4.2MHz for C and 13.6MHz for Pb. Still cross checking the form factors. DA: Using a different technique, I get 2.23 ration of C/Pb (will upload calculation). These are different things and Devi and Ryan will work through it. | ||
| + | #* CG: we should get some dithering results for these runs as well. | ||
| + | # PREX2 AT runs update: Ryan [http://ace.phys.virginia.edu/HAPPEX/4119 haplog4119] | ||
| + | #* Ryan: still need to recover what the raster size is. | ||
| + | #* CG: we should confirm 4120, 4121 was hitting the frame. Ryan: will do | ||
| + | #* Ryan: will work on getting more detailed plots (similar to what Weibin has) | ||
| + | #* KK: we should double check why the difference in the error bar to the average between the dithering and regression. Ryan: will work on plots (maybe vs minirun). KK: the dithering mostly likely will need work (together with the dithering experts). Ryan: will work with Devi | ||
# PREX1 AT systematics summary: Ciprian | # PREX1 AT systematics summary: Ciprian | ||
| − | #* | + | #* next time |
== Present == | == Present == | ||
| − | + | KK, Dustin M, Devi A, Ryan R, Robert R, Weibin Z, Sakib R, Ciprian G, David A | |
[[Category:Meetings]] | [[Category:Meetings]] | ||
[[Category:AT Meetings]] | [[Category:AT Meetings]] | ||
Latest revision as of 15:56, 2 June 2020
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Agenda
- CREX AT runs update: Weibin & Robert haplog4120
- WZ: for the dpp i have the mean and RMS
- KK: it's important to see the tails (5-10 sigma away) and log plots
- KK: for the narrow peak we should look into detail (vs event number)
- Ryan: started looking at the form factors. At 2GeV the C fraction is much larger than at 1GeV. 4.2MHz for C and 13.6MHz for Pb. Still cross checking the form factors. DA: Using a different technique, I get 2.23 ration of C/Pb (will upload calculation). These are different things and Devi and Ryan will work through it.
- CG: we should get some dithering results for these runs as well.
- PREX2 AT runs update: Ryan haplog4119
- Ryan: still need to recover what the raster size is.
- CG: we should confirm 4120, 4121 was hitting the frame. Ryan: will do
- Ryan: will work on getting more detailed plots (similar to what Weibin has)
- KK: we should double check why the difference in the error bar to the average between the dithering and regression. Ryan: will work on plots (maybe vs minirun). KK: the dithering mostly likely will need work (together with the dithering experts). Ryan: will work with Devi
- PREX1 AT systematics summary: Ciprian
- next time
Present
KK, Dustin M, Devi A, Ryan R, Robert R, Weibin Z, Sakib R, Ciprian G, David A
