STAR Protected
Electron identification efficiency
The electron identificatione fficiency is calculated to determine how effective the electron identification process done in this analysis is, and hence how much electrons there actually are, given
Photonic electron reconstruction efficiency
Photonic electron reconstruction efficiency is the background rejection efficiency.
Simulation analysis: track association and identifcation
To calculate electron identification and photonic electron reconstruction efficiencies, simulation dataset for both 2005 and 2006 are used.
Status of the work related to the problem of big memory usage in central hijing events
Description of the problem: big memory usage in reconstruction of AuAu 200 GeV hijing central events.
Time Dependency in BEMC Gains, Refit with Gain Corrections
To address some concerns and improve the quality of our analysis, we have converted ADC tower response to energy using 2006 gains. We then repeated our analysis in the new scale. T
Consistency Between Run 6 FPD and Run 8 FMS Eta Transverse Single Spin Asymmetry
We discussed that the status of the Run 8 FMS analysis for Eta asymmetry should be reconsidered and a comparison should be made to the FPD Run 6 analysis (if possible) before we proceed to writing
FPD Eta Event Display
The large single spin asymmetries associated with the ETA meson implies that relatively few events contribute to large values of AN.
Non-photonic electron analysis, update 11/12/2009
Outline of analysis:
Final objective is both non-photonic electron cross-section and ALL.
For both:
Summary of Lead Problems
Original hint something strange was going on in the new vs.
Run 10 preparation meetings #3
1-189, EVO, at 19:00 (GMT), duration : 02:00
| Time | Talk | Presenter |
|---|---|---|
| 15:00 | General introduction ( 00:20 ) 1 file | Jerome Lauret (BNL) |
| 15:20 | Storage and network project ( 00:20 ) 3 files | Wayne Betts (BNL) |
Run X
Below are the related meetings:
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x0/y0 into the Geometry/pp2pp database
Hi,
I've written our x0,y0 offset (13 sets) --- each set contains a row of 32 numbers --- into the database of Geometry/pp2pp of StarDb in the table of "pp2ppOffset".