STAR Protected

EVO

This section contains information about using EVO for STAR meetings.

EVO Conference Computer

If you would like to be able to use EVO in the 1006 trailer, there is a conference PC setup for use.  There is a generic account on the computer for everyone to share.

Investigating Shower Shapes & Chi2

Introduction

 

Idea here is to try to revive the chi2 method and to see if adding a chi2 cut to the conversion method selection - CDF did this - makes sense.

Progress Report on work on non-linear response of FMS

Summary of progress:
  1.  

Transverse Spin Talk for DIS 2009

 Please find the latest draft of my Transverse Spin talk for DIS 2009 below and please send comments.

 

RICH Scaler diagram

This is the RICH scaler diagram for the BBC portion.  It is adjusted as of Apr. 15, 2009, and again Feb. 17, 2016

 

Disk space for FY09

Institution disk space

The below is what was gathered as the call sent to starsoft "Inquiry - instit

04 Apr

April 2009 posts

STAR Management Meeting

2009-04-23 11:00
2009-04-23 12:00
Etc/GMT-7
Thursday, 23 April 2009
BNL, 50-Orange Room, 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: 923329 // Password: 0952

   Time:  11am - 12noon EDT

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

  Agenda:

    1)    Run9 Status: Bill / Bernd
    2)   
e-h correlation paper and NPE issue - Bedanga

    3)    AoB

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

    Brief Summary:

   0) Attending:

   1)

 

  Notes:
    1) China-STAR ToF meeting: April 26-29, Hangzhou, China

    2) STAR Regional meeting: May 6-9, 2009, Pusan, Korea

    3) CPOD2009: June 8-12, 2009, BNL

    4) BNL PAC: June 15-16, 2009, BNL

    4) STAR Regional meeting: June 29-30, 2009, Dubna, Russia

    5) STAR Analysis meeting, July 7-11, 2009, MIT, Boston

    6) STAR Regional meeting: Sept. 25-26, Rio, Brazil

    7) SQM2009: Sept. 27-Oct. 2, Buzios, Brazil

 

CNI summary analysis from fill 10373 to fill 10507

       In attachment shows the compare between polarimeter 1 and polarimeter 2 for blue (yellow) beam.  And also

STAR Management Meeting

2009-04-16 11:00
2009-04-16 12:00
Etc/GMT-7
Thursday, 16 April 2009
BNL, 50-Orange Room, 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: 923318 // Password: 0952

   Time:  11am - 12noon EDT

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

  Agenda:

    1)    Run9 Status: Switching to 200GeV - Bill / Bernd
    2)    Plans for data analysis on 500 GeV spin data - Ernst/Jim

    3)    Publication speed up - Jerome

    4)    AOB

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

    Brief Summary:

   1) Attending: Bill, Bernd, Jerome, Jamie, Olga, Bedanga, Helen, Jim, Ernst, Flemming, Nu

   2) Spin discussions: PWG goals are (i) Top priority is the 200 GeV data taking; (ii) the next is the analysis of the 500 GeV data to demonstrate the W-peak.

   3) Paper process: the discussions to be continued.

 

  Notes:

   1) TPC Committee, Ron Settler (chair), review due June 4,5.

   2) NPE Committee, H. Huang (chair)

 

  Meetings:


    1) China-STAR ToF meeting: April 26-29, Hangzhou, China

    2) STAR Regional meeting: May 6-9, 2009, Pusan, Korea

    3) CPOD2009: June 8-12, 2009, BNL

    4) BNL PAC: June 15-16, 2009, BNL

    4) STAR Regional meeting: June 29-30, 2009, Dubna, Russia

    5) STAR Analysis meeting, July 7-11, 2009, MIT, Boston

    6) STAR Regional meeting: Sept. 25-26, Rio, Brazil

    7) SQM2009: Sept. 27-Oct. 2, Buzios, Brazil

 

Scanning Isolation & Hadronic Veto

Introduction

DSM check

The purpose of the analysis is to compare various DSM inputs to the corresponding values constructed from Qtdata according to my best understanding of Eleanor's trigger document.

PSU FMS photon reconstruction

 Penn State FMS (Run 8) Software for StRoot

version build12 (Aug 31 2009)

STAR Management Meeting

2009-04-09 11:00
2009-04-09 12:00
Etc/GMT-7
Thursday, 9 April 2009
BNL, 50-Orange Room, 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: 923307 // Password: 0952

   Time:  11am - 12noon EDT

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

  Agenda:

    1)    Run9 Status: Switching to 200GeV - Bill / Bernd
    2)    Tom Trainor - Nu

    3)    BulkCorr PWG co-convener (M. Lisa) - Nu
    4)    QM09 (three plenary talks; 21 parallel talks; four selected poster talks; two awards) - Bedanga

    5)    HLT review report - Nu

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

    Brief Summary:

   0) Attending: Jerome, Olga, Helen, Bill, Flemming, Nu, Bedanga

   1) HLT: inform PAs to proceed test in Run9 and complete the arguements for he phsyics case

   2) Trainor: lots of discussions and more are needed.

  Notes:
    1) China-STAR ToF meeting: April 26-29, Hangzhou, China

    2) STAR Regional meeting: May 6-9, 2009, Pusan, Korea

    3) STAR Analysis meeting, July 7-11, 2009, MIT, Boston

    4) STAR Regional meeting: Sept. 25-26, Rio, Brazil

    5) Nu's comment on BES Summary document - 4/11/09, pdf file

Trigger Bias Rescaling

As a reminder, these were the bias distributions we got out of raw Pythia in Trigger Bias Redux:

Beam energy scan table - statistical needs

This is the table of statistical requirements for various analyses.  Later I will document here where we came up with the particular numbers.

Transverse components in longitudinal beam fills

A simple spreadsheet to plot the transverse components of the longitudinal fills from ZDC polarimeter runs is attached.  The data are taken from Olkesandr's online fill plots (last page - not

Simulations of Central Production

Len's Software Trigger Algorithm

Just ths weekend, Len completed code that emulates the function of Eleanor's trigger algorithm.