IRMIS progress

Speaker : Jiro Fujita ( Creighton )


Talk time : 14:10, Duration : 00:20

Follow-ups

Speaker : All ( All )


Talk time : 14:00, Duration : 00:10
  • Comments on the SSH-key management plans - access model (last slide) from You do not have access to view this node
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  • AIDE

Run VII preparation, meeting #8

Under:
-00-00
Thursday, 1 January 1970
, at 00:00 (GMT), duration : 00:00
TimeTalkPresenter
14:00Follow-ups ( 00:10 ) 1 fileAll (All)
14:10IRMIS progress ( 00:20 ) 0 filesJiro Fujita (Creighton)
14:30Offline QA and online ( 00:10 ) 0 filesJerome Lauret / Gene Van Buren (BNL)
14:40Electronic Elog ( 00:10 ) 0 filesLevente Hajdu (BNL)
14:50AOB ( 00:10 ) 0 filesAll (All)

P bar

P06ib: Plots_Nfit-Pbar-nfit_0.20pT0.30_0nch1000
P06ib: Pbar 0.20pT0.30_0nch1000

      

Proton

P06ib: Plots_Nfit-Proton-nfit_0.20pT0.30_0nch1000
P06ib: Proton 0.20pT0.30_0nch1000

      

K Plus

P06ib: Plots_Nfit-KPlusMinus-nfit_0.20pT0.30_0nch1000
P06ib: K plus 0.20pT0.30_0nch1000

      

K Minus

P06ib: Plots_Nfit-KMinus-nfit_0.20pT0.30_0nch1000
P06ib: K minus 0.20pT0.30_0nch1000

      

Pi Plus

P06ib: Plots_Nfit-PiPlusMinus-nfit_0.20pT0.30_0nch1000
P06ib: Pi plus 0.20pT0.30_0nch1000

      

Pi Minus

P06ib: Plots_Nfit-PiMinus-nfit_0.20pT0.30_0nch1000
P06ib: Pi minus 0.20pT0.30_0nch1000

      

Plots - Number of Fitted Points

The Following are the results for dca distributions for different pT bins in Pi Minus. The results of dca agrees reasonable for the cut-off of 2 cm and above. These plots were done using the macro plot_dca.C

UrQMD study of two-particle correlations

Speaker : Hania Gos ( WUT, SUBATECH )


Talk time : 11:00, Duration : 00:10

Plot_Hits.C

void plotHits() { gROOT->LoadMacro("~/mymacros/Utility.C"); // f = new TFile("PiPlus200_SimDb_p2.root","read"); //f = new TFile("PiMinus200_SimDb_lowTest_03pt04.root","read");

Scan-Hits.C

#ifndef __CINT__ #include "TROOT.h" #include "TSystem.h" #include #include "TH1.h" #include "TH2.h" #include "TH3.h" #include "TFile.h" #include "TTree.h" #include "TChain.h"

Jobs Done

P06ib:
6050022_1050001.28606: /eliza5/starprod/embedding/P06ib
6050022_1050001.7247: /eliza5/starprod/embedding/P06ib
6050022_1060001.3717: /eliza5/starprod/embedding/P06ib
 6050022_1070001.10533: /eliza5/starprod/embedding/P06ib

P05ic



Missing /Dead Areas

Hits-P05ic_200gev_auau-PiMinus_hitsXYeast_p2.gif

Performance

Under:

Below is a listing of adjustable mysql performance parameters, their descriptions and their current settings.

Space-momentum correlations, the smoothness approximation, and strong final-state ineractions

Speaker : Mike Lisa ( The Ohio State University )


Talk time : 10:30, Duration : 00:30
talk can be also found at http://www.star.bnl.gov/protected/hbt/chajecki/mike/

Setting Up A Star Offline Database Mirror

Under:

Set up an environment consistent with the STAR db environments.

  1. Create a user named 'mysql' and a group 'mysql' on the system.
  2. Create a directory for the mysql installation a

P07ib

Test done on P07ib - Doing claibration on dE/dx

K star

Files: pdsf>/eliza1/starprod/embedding/KstarM* ( July 31 2007)