RDO Board
Updated on Tue, 2010-02-09 21:09. Originally created by matis on 2010-02-09 21:09.Speaker : Micheal
Talk time : 09:40, Duration : 00:20
Ladder Board
Updated on Tue, 2010-02-09 21:08. Originally created by matis on 2010-02-09 21:08.Speaker : Christophe
Talk time : 09:20, Duration : 00:20
News
Updated on Tue, 2010-02-09 21:07. Originally created by matis on 2010-02-09 21:07.Speaker : Howard
Talk time : 09:00, Duration : 00:20
lfspectra Run 10 QA
Updated on Wed, 2010-02-10 12:09 by tone421. Originally created by jeromel on 2010-02-09 20:53.Speaker : Anthony Timmins ( WSU )
Talk time : 12:40, Duration : 00:20
Embedding status - current, pending, incoming tasks
Updated on Tue, 2010-02-09 23:30 by hmasui. Originally created by jeromel on 2010-02-09 20:51.Speaker : Hiroshi Masui ( LBNL )
Talk time : 12:20, Duration : 00:20
StPythiaEvent and unified event structure
Speaker : All ( All )
Talk time : 12:00, Duration : 00:20
Victor P., Jason W., Jerome L., Mike B.
Software and Computing phone meeting
1-189, EVO, at 17:00 (GMT), duration : 01:00
| Time | Talk | Presenter |
|---|---|---|
| 12:00 | StPythiaEvent and unified event structure ( 00:20 ) 3 files | All (All) |
| 12:20 | Embedding status - current, pending, incoming tasks ( 00:20 ) 1 file | Hiroshi Masui (LBNL) |
| 12:40 | lfspectra Run 10 QA ( 00:20 ) 2 files | Anthony Timmins (WSU) |
Progress
The following changes are madeto fix the histogram problem
1> geantBranch -> geant
vpdSimMaker
Energy deposition distributions, after the cut 20%*PeakEnergy employed.
BSMD Calibration Update 2/9
Our stats have been expanded to include the whole pp500 dataset (thanks Matt), so the next step is to try to fit the ADC distribution in each momentum slice. At Joe's suggestion I gave up try
Amassed PDFs and E866 Data
I have amassed a large amount of pdf information and put it together in the following plot.
Run 10 scaler plots
Updated on Fri, 2010-02-26 13:16. Originally created by genevb on 2010-02-09 10:32.Here are plots of BBC backgrounds divided by ZDC coincidence rates vs. day using the RICH scaler ntuple for Run 10:
No Significant Correlation between Luminosity and MIPs
After confirming an apparent MIP-position dependency on time, we have now begun to investigate potential causes. Since we know that luminosity has also varied over time, we attempted to disco
W papers by C. Bourrely and J. Soffer
Nuclear Physics paper: Nucl. Phys. B509 (1998) 297.
Physics Letter paper: Physics Letters B314 (1993) 132.
Committee on dispute over submission of ISMD09 Proceedings - Kettler
Committee members: Declan Keane, Jerome Lauret, Saskia Mioduszewski
CSW4DB Phase II follow-up
ITD Conference Room / Conf. Room B515, at 14:00 (GMT), duration : 08:00
We will review our timetable and project milestones, deliverables and work ahead from both side.
The current contract and payment to BNL needs to be settled.
APS W Cross Section Talk February 16 2010
See attachments. Please choose the most recent version.
FMS simulation
I ran some Pythia simulation together with GSTAR for FMS and here are some of the results. The basic settings for the study are:
1. Pythia 6.222 + GSTAR.