STAR Protected

Event Generator Framework for starsim and starvmc

Abstract: The accurate simulation of pp and heavy ion collisions at STAR requires the use of validated, well tuned event generators.

FMS meeting 20100412 calibration update

Kurtosis analysis of p+p, Cu+Cu and Au+Au collisions

Speaker : Xiaofeng Luo ( LBNL/USTC )


Talk time : 14:00, Duration : 00:30

9:2010/APR/8 Updated HF priority list

8.APRIL. 2010

NPE p+p  requests moved to higher  priority.

This is done because existing  paper proposal and urgency to resolve the issue

Physics goals for a draft 2011, 2012 beam-use request

Abstract for Meson 2010

MinuitVF performance in Au+Au 2010

Evaluation code run in stardev

day 40 trigger id 260021

BHT3coin vs dijets

 I've made some progress toward validating the BHT3coincidence requirement's stability vs the dijet rate.

Pre-embedding TpcRS QA for W analysis III

Pre-embedding TpcRS QA for W analysis III

Alignment update

Speaker : ODU


Talk time : 14:50, Duration : 00:20

Draft of the DIS10 talk

STAR Management Meeting

2010-04-08 11:00
2010-04-08 12:00
America/New York
Thursday, 8 April 2010
BNL, 50-I-189, at 15:00 (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: 56533 // Password: 0952

   Time:  11 AM - 12 PM EDT

 *--===================================================================--*

I. Agenda:

1) Run10 status / Next Tuesday presentation - Bill

2) FMS & forward physics issues - Nu

3) BUR11 committee

4) HEPNAMES - All

5) PP enforcement - Nu

6) TBD

 

*--===================================================================--*

II. Brief Summary and/or Action Items:

            0) Attendency:

 

III. Note:

► RHIC Planning Meeting Website

► STAR BUR11 Committee: J. Dunlop, O. Evdokimov, C. Gagliardi, B. Mohanty, B. Surrow, E. Schitermann, P. Sorensen, S. Trentalange, N. Xu (chair), Z.B. Xu and the Charge. STAR BUR09 and BUR10.

Charge for New Decadal Plan, Steve Vigdor, Dec. 17, 2009

► STAR NPE Committee, H. Huang (chair), April 2008

► STAR FMS Review: Sept. 1-2, BNL. P. Jacobs (chair). Review Report

*--===================================================================--*

IV. Future Meetings and Reviews:

RHIC and AGS User's Annual Meeting: June 7-11, 2010, BNL

STAR Analysis Meeting: June 15-18, 2010, UCLA. Chair: H. Huang

► RHIC PAC Meeting: June 21-23, 2010, BNL

► RHIC Science and Technology Review: June 28-30, 2010, BNL

Spin2010: Sept. 27 - Oct. 2, 2010, Juelich, Germany

► STAR Collaboration Meeting: Oct. 27 - Nov. 1, 2010, BNL. Chair: J. Dunlop

DNP2010: Nov. 3-6, 2010, Santa Fe, NM

pp2pp weekly

2010-04-07 14:00
2010-04-07 15:30
America/New York
Wednesday, 7 April 2010
1-189 Physics, at 18:00 (GMT), duration : 01:30

1. Central Production JH

2. Analysis Update Kin

3. Alignment, transport update ODU

4. Other all

EVO bridge has been reserved:


Description: pp2pp weekly
Community: Universe
Password: WeeklyElastic

Meeting Access Information:
- Meeting URL
http://evo.caltech.edu/evoGate/koala.jnlp?meeting=ete8eavsvaauaDaIIt

- Password: WeeklyElastic
- Phone Bridge
ID: 42134
Password: 9771


EVO Phone Bridge Telephone Numbers:
---------------
- USA (Caltech, Pasadena, CA)
+1 626 395 2112

- USA (BNL, Upton, NY)
+1 631 344 6100

TimeTalkPresenter
14:00Central production ( 00:20 ) 1 fileJH Lee (BNL)
14:20Analysis update (all runs) ( 00:30 ) 1 fileKin (BNL)
14:50Alignment update ( 00:20 ) 3 filesODU

Generic queue between Atlas/STAR

General

This blog follows a request to restore the general queue usage and sharing between Atlas and STAR.

Chi-Square Cut for 2009 pp 500 and 200 GeV

DIS2010 Talk - Gluon Polarization

Posting of DIS2010 (April 19-23, 2010) on:

 

Exploring the Gluon Polarization with Inclusive and Correlation Measurement

Detector ADC distribution studies 3

  I checked the raw ADC distribution strip by strip for the ESMD.

W paper comments

Comments on v 1.3.1.  Other comments pending new release.

Detector gain studies 1

      To get a general idea about the gain values used before for the ESMD, I checked the gain values related with the

Zero Field and TPC Hit Errors

Prompted by a suggestion from Alex Schmah, I decided to have another look at zero field data, using run 6065039 (during Run 5) as another factor in understanding TPC alignment.