STAR Protected
FHC cosmic ray test status 2
With the same setup, I just use the cross CTB trigger cut to see whether there's some construction damage to the group from column 4 to column 6
FHC cosmic ray test status 2
With the same setup, I just use the cross CTB trigger cut to see whether there's some construction damage to the group from column 4 to column 6
Creating a Jet Filter for 2009
The purpose of creating a jet filter is to increase the sampled luminosity for the jet simulation sample.
Opening remarks / Welcome
Updated on Mon, 2009-12-28 17:59. Originally created by rexwg on 2009-11-16 16:53.Reference
Speaker : Local Organizer
Talk time : 09:00, Duration : 00:15
Opening / PID Plenary Session
Updated on Fri, 2009-12-04 14:32. Originally created by rexwg on 2009-11-16 16:51.| Time | Talk | Presenter |
|---|---|---|
| 09:00 | Opening remarks / Welcome ( 00:15 ) 0 files | Local Organizer |
| 09:15 | PID using TOF (30+5 Min) ( 00:35 ) 1 file | Xiaoping Zhang |
| 09:50 | Electromagnetic shower shape analysis for direct gamma/pi0 id and in-medium fragmentation function measurements (30+5 Min) ( 00:35 ) 1 file | Ahmed Hamed |
| 10:25 | Coffee break ( 00:20 ) 0 files | |
| 10:45 | W measurement and the identification of electrons (30+5 Min) ( 00:35 ) 1 file | Jan Balewski |
| 11:20 | Update on embedding (30+5 Min) ( 00:35 ) 2 files | Andrew Rose |
STAR Analysis Meeting (Jan 2010)
Updated on Mon, 2009-11-16 17:30. Originally created by rexwg on 2009-11-16 16:38.UT Austin
The chair of the organizing committee for the meeting is Prof. Jerry Hoffmann (UT Austin).
The scientific program committee is chaired by Prof. Christina Markert and the members are: Elena Bruna (Yale), Evan Finch (Yale), Mike Lisa (OSU), Christina Markert (UT Austin), Bedanga Mohanty (VECC), Lanny Ray (UT Austin), Shusu Shi (LBNL/IOPP), Ernst Sichtermann (LBNL), Jim Sowinski (IUCF), Gang Wang (UCLA).
STAR Analysis Meeting (Jan 12-16, 2010) at University of Texas, Austin
STAR Management Meeting
BNL, 50-Orange Room, at 16:00 (GMT), duration : 01:00
EVO: Title: STAR Management Meeting // Community: STAR // Password: star
Phone Bridge: +1 626 395 2112 (CA) / +1 631 344 6100 (NY) // ID: 39499 // Password: 0952
Time: 11 AM - 12 PM EDT
* --===================================================================--*
Agenda:
1) Run10 preparation - Bill
2) Physics program for 62.4 GeV Au+Au collisions (4 weeks) - Nu
3) New convener for Spectra PWG - Nu
4) Anti-nucleus trigger for run10 - All
5) TBD
* --====================================================================--*
Brief Summary: 0) Attendency:
Notes:
1) STAR TPC Review (key= star2009), June 4,5, BNL. Ron Settler (chair). Review report.
2) NPE Committee, H. Huang (chair)
3) STAR TOF Close Out Review, Aug. 10-11. Review report and The Plan.
4) STAR FMS Review agenda, Sept. 1-2, BNL, P. Jacobs (chair). Review report
Future Meetings and Reviews:
1) STAR Analysis Meeting, Jan. 11-15, 2010, UT Austin
2) APS April meeting, Feb. 13-17, 2010, Washongton DC.
In Progress
Quick-Reference Guide
Papers by Event Structure group and selected papers by group members. Suggestions and updates are welcome.
Ecalgeo V6.1
Plot of reconstructed energy/input energy as a function of input energy - comparing cvs version with version 6, version 6.1 and version 6.1 with pure lead. The replacement for pure lead means
Electron asymmetry
The goal is to obtain non-photonic electron asymmetry. To get there, various asymmetries need to be calculated, namely:
dE/dx cut, efficiency and electron purity
One of the electron id cut is the dE/dx cut. Unlike the other cuts, the efficiency of this cut is calculated from data instead of simulation.
Pre-embedding QA for W analysis II
Pre-embedding QA for W analysis II
Motivation: Verify compatibility of MC signal W events with real background events (zerobias) before embedding begins.
notes on w error
I've attached a latex document with some notes on sources of error for the W cross section. Please note that the latest version is entitled WxSectV2.