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.
response to questions
Updated on Fri, 2009-11-13 15:32. Originally created by wieman on 2009-11-13 15:32.Reference
Speaker : response to questions
Talk time : 16:10, Duration : 00:20
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.
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.