ZDC local polarimetry for run 22 rotator scan


GPC Code QA GPC#308 && GPC#292

 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

 

ECal pi0 with first gain correction

Speaker : Xilin Liang


Talk time : 12:20, Duration : 00:20

 

FCS_MIP_Day007

Speaker : Navagyan Ghimire


Talk time : 12:00, Duration : 00:20

 

Test of PR#281

 

Correlation between Lambda and CME, updated paper proposal

 

STAR computing needs

 

TpcRS update due to 19GeV 2019 (RDO mask, padGainT0, and Gating Grid)

 

FCS_MIP_Day007

 

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

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
TimeTalkPresenter
10:00Update on K3pi from embedding ( 00:20 ) 1 filePetr Chaloupka

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

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
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.

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

Polarized Light Gluon Collisions : STAR Preliminary Request for

Speaker : Daniel Brandenburg


Talk time : 11:20, Duration : 00:20

Update on pp elastic scattering at sqrt(s) = 510 GeV

Speaker : Wlodek Guryn ( BNL )


Talk time : 10:40, Duration : 00:40

 

He4L lifetime and yield measurements at AuAu 3GeV

Speaker : Xiujun Li


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

 

Installation and Commissioning

Speaker : Xu Sun, Yu Hu ( UIC, Fudan )


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

DAQ

Speaker : Tonko Ljubicic ( BNL )


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