Simulations for DY Measurements at STAR

Speaker : A. Ogawa


Talk time : 09:50, Duration : 00:40

Possible DY Physics at RHIC

Speaker : C. Gagliardi


Talk time : 09:30, Duration : 00:20

Spin Physics at Forward Rapidity

Speaker : Spin PWG , E.Sichtermann


Talk time : 09:10, Duration : 00:20

Introduction

Speaker : Nu Xu


Talk time : 09:00, Duration : 00:10

STAR forward Physics

2010-04-29 09:00
America/New York
Thursday, 29 April 2010
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

TimeTalkPresenter
09:00Introduction ( 00:10 ) 1 fileNu Xu
09:10Spin Physics at Forward Rapidity ( 00:20 ) 1 fileSpin PWG , E.Sichtermann
09:30Possible DY Physics at RHIC ( 00:20 ) 1 fileC. Gagliardi
09:50Simulations for DY Measurements at STAR ( 00:40 ) 1 fileA. Ogawa
10:30Coffee break ( 00:30 ) 0 files
11:00Forward Physics at STAR at RHIC ( 00:30 ) 0 filesH.Crawford
11:30Forward Lambda Spin Physics at STAR ( 00:30 ) 1 fileQ.Xu
13:30Spin at Forward Rapidity ( 00:30 ) 1 fileS. Heppelmann
14:00Physics, Plans and Estimates for a DY Measurement ( 00:30 ) 0 filesL.Bland
14:30Discussions and Action Items ( 01:30 ) 0 files

S&C Team April 2010

Under:
S&C Team April 2010

Crossing Angle Simulations


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

Implementation of an age2xml parser using the Parse::RecDecent module (perl)

A few preliminary notes on transforming our existing geometry files to a new format.
 
In an ideal world we would be able to have 100% backwards compatability between

Update

Speaker : Kin Yip


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

pp2pp weekly

2010-04-28 14:00
2010-04-28 15:30
America/New York
Wednesday, 28 April 2010
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

TimeTalkPresenter
14:00Update ( 00:20 ) 1 fileKin Yip
14:20Crossing Angle Simulations ( 00:20 ) 1 file

Possible DY Physics at RHIC

Speaker : C. Gagliardi


Talk time : 09:30, Duration : 00:20

Introdution

Speaker : N. Xu


Talk time : 09:00, Duration : 00:10

Introduction

TimeTalkPresenter
09:00Introdution ( 00:10 ) 0 filesN. Xu
09:10Spin Physics at Forward Rapidity ( 00:20 ) 1 fileSpin PWG
09:30Possible DY Physics at RHIC ( 00:20 ) 0 filesC. Gagliardi

STAR Discussion on Physics at Forward Rapidity

2010-04-29 09:01
2010-04-29 17:00
America/New York
-
from Thursday, 29 April 2010 to Thursday, 29 April 2010
ITD Seminar Room (B515)
Conference duration: 1 day

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

Meeting : 04/29

  1.  Jonathan
    1. Changes in MuKpi code : NTuple, files to include,new entries in the NTuple, correction to gRefMult, etc ...

ESMD pedestal status check with run 9059045 and run 9061019

     I checked the pedestal values for U pannel sector 2 strip 1, 11, 21 and 31 ( strip is marked from 0 to 287) in run08 pp run number 905