STAR Protected
ESMD pedestal status in run08 pp data
With 119 runs in pp run08 data, I checked the status of the ESMD strip pedestals.
STAR and Beam User Request - run 11/12
Updated on Tue, 2010-06-15 14:49 by nxu. Originally created by bedanga on 2010-05-01 22:18.Reference
Speaker : Nu Xu ( LBNL )
Talk time : 09:25, Duration : 00:35
STAR Analysis Meeting, June: 15 - 18, 2010
Updated on Sat, 2010-05-01 22:57. Originally created by bedanga on 2010-05-01 22:12.University of California Los Angeles
STAR Analysis Meeting is being held to discuss the recent progress in various physics programs in the STAR experiment.
track/dca/helix
meaning of different track utilities used in MuKpi/KFParticle:
- $STAR/StRoot/StDcaGeometry.cxx
ESMD pedestal cross check update
Qinghua and I found a debug in the StADCMaker.cxx. I should use the class "strip" not "hitstrip" to get the raw ADC distribution.
Some AuAu7 event images
Using st_physics_adc_11119033_raw_2500001, I created event display images from the first few events in the file (after deactivating some voltage=0 entries in the tpcAnodeHVavg table and
ESMD raw ADC cross check
With 5 runs in run08 pp data, the following are the run numbers,
STAR forward Physics
ITD conference room, BNL, at 13:00 (GMT), duration : 00:00
EVO: Title: STAR Management Meeting // Community: STAR // Password: star
Phone Bridge: +1 626 395 2112 (CA) / +1 631 344 6100 (NY) // ID: 1828254 // Password: 0952
Time: 9 AM - 5 PM EDT
| Time | Talk | Presenter |
|---|---|---|
| 09:00 | Introduction ( 00:10 ) 1 file | Nu Xu |
| 09:10 | Spin Physics at Forward Rapidity ( 00:20 ) 1 file | Spin PWG , E.Sichtermann |
| 09:30 | Possible DY Physics at RHIC ( 00:20 ) 1 file | C. Gagliardi |
| 09:50 | Simulations for DY Measurements at STAR ( 00:40 ) 1 file | A. Ogawa |
| 10:30 | Coffee break ( 00:30 ) 0 files | |
| 11:00 | Forward Physics at STAR at RHIC ( 00:30 ) 0 files | H.Crawford |
| 11:30 | Forward Lambda Spin Physics at STAR ( 00:30 ) 1 file | Q.Xu |
| 13:30 | Spin at Forward Rapidity ( 00:30 ) 1 file | S. Heppelmann |
| 14:00 | Physics, Plans and Estimates for a DY Measurement ( 00:30 ) 0 files | L.Bland |
| 14:30 | Discussions and Action Items ( 01:30 ) 0 files |
Implementation of an age2xml parser using the Parse::RecDecent module (perl)
pp2pp weekly
1-189 Physics, at 18:00 (GMT), duration : 01:30
Agenda
1. Update - Kin
2. How to converge with A_N paper - Wlodek + all
Call in 631 344 4048
Wlodek
| Time | Talk | Presenter |
|---|---|---|
| 14:00 | Update ( 00:20 ) 1 file | Kin Yip |
| 14:20 | Crossing Angle Simulations ( 00:20 ) 1 file |
Introdution
Updated on Wed, 2010-04-28 07:43. Originally created by nxu on 2010-04-28 07:42.Reference
Speaker : N. Xu
Talk time : 09:00, Duration : 00:10
Introduction
Updated on Wed, 2010-04-28 07:42. Originally created by nxu on 2010-04-28 07:40.| Time | Talk | Presenter |
|---|---|---|
| 09:00 | Introdution ( 00:10 ) 0 files | N. Xu |
| 09:10 | Spin Physics at Forward Rapidity ( 00:20 ) 1 file | Spin PWG |
| 09:30 | Possible DY Physics at RHIC ( 00:20 ) 0 files | C. Gagliardi |
STAR Discussion on Physics at Forward Rapidity
Updated on Wed, 2010-04-28 07:38. Originally created by nxu on 2010-04-28 07:38.ITD Seminar Room (B515)
EVO: Title: STAR Management Meeting // Community: STAR // Password: star
I/O Comparison between SSD, SAS and RAM-based filesystems
Primary test node:
Scientific Linux 5.3, kernel 2.6.18-164.15.1.el5 #1 SMP (x86_64)
Dell PowerEdge R610
12 GB of RAM (RAM type/speed?)
BHT3coin vs BHT3 resolved
Going back through the code I'm using has resolved the mismatch I saw last week in the ratio of BHT3coin to BHT3.
Understanding Track <z> Distribution
Understanding Track <z> Distribution
Data: L2W stream Data and ZeroBias Data from Fill 10531 (Run numbers 10101059-10101094)
ESMD number of transition strips run dependence studies
Using the 283 runs in run08 pp data, I studied when one