Pixel Mechanical
Updated on Wed, 2009-04-15 22:23. Originally created by matis on 2009-04-15 22:23.Speaker : Eric
Talk time : 11:20, Duration : 00:20
News
Updated on Wed, 2009-04-15 22:22. Originally created by matis on 2009-04-15 22:22.Talk time : 11:00, Duration : 00:20
STAR Analysis Meeting 09
Updated on Wed, 2009-07-08 15:18. Originally created by gdwebb on 2009-04-15 20:17.Updates on the UE Studies
Data & Simulation comparison: Phi
Updated on Thu, 2009-04-16 14:10. Originally created by kurnadi on 2009-04-15 17:56.Comparing track phi between data (2005) and simulation (y2005).
Would you be in favor of a group common calendar sharing your days off?
Updated on Fri, 2009-04-17 18:56 by testadmin. Originally created by jeromel on 2009-04-15 16:17.Constraining Eta Dependence in the BEMC Calibration Systematic
Updated on Tue, 2009-04-14 17:46. Originally created by betan on 2009-04-14 16:46.In the Monday EMC meeting, a concern was raised regarding a possible eta dependence to the new BEMC calibration systematic calculation.
2009.04.17 WSU nuclear seminar
The STAR spin program with longitudinally polarized proton beams
04 Apr
April 2009 posts
L2Jet algo: True 2D Search
Updated on Fri, 2009-04-17 10:44. Originally created by pagebs on 2009-04-14 02:17.There are concerns that the current L2jet code, described »
Luminosity - Run 9 / 500GeV
Updated on Mon, 2009-04-13 16:54. Originally created by surrow on 2009-04-13 15:35.Luminosity - Run 9 / 500GeV
Vers1: Individual triggers (Total, 230530 and 230531)
Vers2: Total only (For RHIC Presentations)
minutes
Updated on Mon, 2009-04-13 13:20. Originally created by bouchet on 2009-04-13 13:17.W analysis status page - PWG updates - Run 9 / 500GeV
Updated on Sun, 2009-04-12 22:30. Originally created by surrow on 2009-04-12 22:30.W analysis sta
DIS 2009 talk - Exploring the Gluon Polarization with Inclusive and Correlation Measurements
Updated on Tue, 2009-04-21 13:22. Originally created by surrow on 2009-04-12 11:54.DIS 2009 talk - Tuesday, April 28, 2009
STAR Management Meeting
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
* --===================================--*
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
News (Production etc)
Updated on Fri, 2009-04-10 10:20. Originally created by margetis on 2009-04-10 10:20.Thicker IST puzzle
Updated on Mon, 2009-04-13 13:16 by bouchet. Originally created by margetis on 2009-04-10 10:18.Reference
Speaker : Jonathan/All
Talk time : 13:50, Duration : 00:20
ratio THICK IST / THIN IST : the ratio, per species, is a bit lower than 1 for the first pt bin (except the kaons).
It is more visible (mass dependence ?)
What is left for CD0 response?
Updated on Fri, 2009-04-10 10:21. Originally created by margetis on 2009-04-10 10:18.HFT Software
Updated on Fri, 2009-04-10 10:17. Originally created by margetis on 2009-04-10 10:17.510-4867333, at 17:30 (GMT), duration : 01:00
Here
| Time | Talk | Presenter |
|---|---|---|
| 13:30 | News (Production etc) ( 00:05 ) 0 files | All |
| 13:35 | What is left for CD0 response? ( 00:20 ) 0 files | All |
| 13:50 | Thicker IST puzzle ( 00:20 ) 2 files | Jonathan/All |
| 14:10 | minutes ( 00:20 ) 0 files |