LFSUPC PWG QA 01/21/2022
Updated on Thu, 2022-01-20 16:51. Originally created by cj17 on 2022-01-20 16:51.STAR Collaboration Meeting - February 2022
Updated on Wed, 2022-02-23 09:32. Originally created by marr on 2022-01-20 11:24. 2022-02-14 09:00
2022-02-25 13:00
America/New York
from Monday, 14 February 2022 to Friday, 25 February 2022
Online
Online
Conference organizing committee information : Conference organizing committee information :
Aihong Tang (BNL, Chair)
Oleg Eyser (BNL)
Raghav Kunnawalkam Elayavalli (Yale)
Shuai Yang (SCNU)
J. H. Lee (BNL)
Conference duration: 12 days
Meeting agenda outline
Feb. 14: Junior's Day
Feb. 15-18: Parallel sessions
Feb. 21-25: Plenary sessions
ZDC local polarimetry for run 22 rotator scan
Updated on Thu, 2022-02-10 05:42. Originally created by jlzhang on 2022-01-20 08:08.
GPC Code QA GPC#308 && GPC#292
Updated on Thu, 2022-01-20 03:57. Originally created by linyf on 2022-01-20 03:57.This Blog only service for the GPC code QA in STAR
Yufu Lin(林裕富)
Status on net-proton high moments from 14.6GeV AuAu collisions
Updated on Wed, 2022-01-19 22:26. Originally created by yghuang on 2022-01-19 22:26.
ECal pi0 with first gain correction
Updated on Wed, 2022-01-19 12:31. Originally created by liangxl on 2022-01-19 12:02.Reference
Speaker : Xilin Liang
Talk time : 12:20, Duration : 00:20
FCS_MIP_Day007
Updated on Wed, 2022-01-19 11:58. Originally created by nghimire on 2022-01-19 11:56.Reference
Speaker : Navagyan Ghimire
Talk time : 12:00, Duration : 00:20
Correlation between Lambda and CME, updated paper proposal
Updated on Wed, 2022-01-26 22:57. Originally created by fengyich on 2022-01-18 18:50.
STAR computing needs
Updated on Fri, 2022-01-21 09:42. Originally created by ruanlj on 2022-01-18 15:21.
FCS_MIP_Day007
Updated on Tue, 2022-01-18 23:23. Originally created by nghimire on 2022-01-18 09:28.
Tracking Efficiency Uncertainty meeting
2022-02-01 10:00
2022-02-01 11:00
America/New York
Tuesday, 1 February 2022
https://bnl.zoomgov.com/j/1607035037?pwd=WDVqaEdwa0RtTEM5a1VvZ24yU2gwdz09, at 15:00 (GMT), duration : 01:00
https://bnl.zoomgov.com/j/1607035037?pwd=WDVqaEdwa0RtTEM5a1VvZ24yU2gwdz09, at 15:00 (GMT), duration : 01:00
Tracking Efficiency Uncertainty meeting
2022-02-08 10:00
2022-02-08 11:00
America/New York
Tuesday, 8 February 2022
https://bnl.zoomgov.com/j/1607035037?pwd=WDVqaEdwa0RtTEM5a1VvZ24yU2gwdz09, at 15:00 (GMT), duration : 01:00
https://bnl.zoomgov.com/j/1607035037?pwd=WDVqaEdwa0RtTEM5a1VvZ24yU2gwdz09, at 15:00 (GMT), duration : 01:00
| Time | Talk | Presenter |
|---|---|---|
| 10:00 | Update on K3pi from embedding ( 00:20 ) 1 file | Petr Chaloupka |
Tracking Efficiency Uncertainty meeting
2022-02-15 10:00
2022-02-15 11:00
America/New York
Tuesday, 15 February 2022
https://bnl.zoomgov.com/j/1607035037?pwd=WDVqaEdwa0RtTEM5a1VvZ24yU2gwdz09, at 15:00 (GMT), duration : 01:00
https://bnl.zoomgov.com/j/1607035037?pwd=WDVqaEdwa0RtTEM5a1VvZ24yU2gwdz09, at 15:00 (GMT), duration : 01:00
Tracking Efficiency Uncertainty meeting
2022-01-25 10:00
2022-01-25 11:00
America/New York
Tuesday, 25 January 2022
https://bnl.zoomgov.com/j/1607035037?pwd=WDVqaEdwa0RtTEM5a1VvZ24yU2gwdz09, at 15:00 (GMT), duration : 01:00
https://bnl.zoomgov.com/j/1607035037?pwd=WDVqaEdwa0RtTEM5a1VvZ24yU2gwdz09, at 15:00 (GMT), duration : 01:00
Minutes:
Starting analysis of cosmics data:
Gene pointed out that TOF corrections are turned off for cosmics since it is not know the real direction of the track.
Based on discussion the promissing data sets to look into are run16 and run19.
There was previously an analysis in which it was tried to matched together the two tracks from the same particle. Yuri will try to find the codes.
K-3pi:
Yuri tested the code for propagation of the fit parameters from primary vertex to the first point. It seem that he geometry parameters are fine however the covariance matrix not. This will affect the efficiency of finding the decay vertexes. Needs to be tested.
Starting analysis of cosmics data:
Gene pointed out that TOF corrections are turned off for cosmics since it is not know the real direction of the track.
Based on discussion the promissing data sets to look into are run16 and run19.
There was previously an analysis in which it was tried to matched together the two tracks from the same particle. Yuri will try to find the codes.
K-3pi:
Yuri tested the code for propagation of the fit parameters from primary vertex to the first point. It seem that he geometry parameters are fine however the covariance matrix not. This will affect the efficiency of finding the decay vertexes. Needs to be tested.
Tracking Efficiency Uncertainty meeting
2022-01-18 10:00
2022-01-18 11:00
America/New York
Tuesday, 18 January 2022
https://bnl.zoomgov.com/j/1607035037?pwd=WDVqaEdwa0RtTEM5a1VvZ24yU2gwdz09, at 15:00 (GMT), duration : 01:00
https://bnl.zoomgov.com/j/1607035037?pwd=WDVqaEdwa0RtTEM5a1VvZ24yU2gwdz09, at 15:00 (GMT), duration : 01:00
Polarized Light Gluon Collisions : STAR Preliminary Request for
Updated on Mon, 2022-01-17 10:50. Originally created by jdb on 2022-01-17 10:50.Reference
Speaker : Daniel Brandenburg
Talk time : 11:20, Duration : 00:20
Update on pp elastic scattering at sqrt(s) = 510 GeV
Updated on Mon, 2022-01-17 09:03. Originally created by wlodek on 2022-01-17 09:03.Reference
Speaker : Wlodek Guryn ( BNL )
Talk time : 10:40, Duration : 00:40