STAR Protected
STAR endcap TOF/CBM TOF meeting
The meeting is scheduled on Bluejeans: https://bluejeans.com/303776107, at 15:15 (GMT), duration : 02:00
Time | Talk | Presenter |
---|---|---|
10:15 | Efficiency in FXT ( 00:20 ) 1 file | Philipp Weidenkaff |
STAR endcap TOF/CBM TOF meeting
The meeting is scheduled on Bluejeans: https://bluejeans.com/303776107, at 15:15 (GMT), duration : 02:00
STAR endcap TOF/CBM TOF meeting
The meeting is scheduled on Bluejeans: https://bluejeans.com/303776107, at 15:15 (GMT), duration : 02:00
STAR endcap TOF/CBM TOF meeting
The meeting is scheduled on Bluejeans: https://bluejeans.com/303776107, at 15:15 (GMT), duration : 02:00
Time | Talk | Presenter |
---|---|---|
10:15 | Fixed Target matching ratio ( 00:20 ) 1 file | Philipp Weidenkaff |
STAR endcap TOF/CBM TOF meeting
The meeting is scheduled on Bluejeans: https://bluejeans.com/303776107, at 15:15 (GMT), duration : 02:00
Run12 p+p jet mass measurement paper page
Title:
First measurements of the invariant jet mass in p+p collisions at \sqrt{s} = 200 GeV at STAR
Abstract:
Update [01.02.2020] -- Track Pt in Run 9 pp Data and Embedding
Following up on the previous post:
Update [12.29.2019] -- Event Pt in Run 9 pp Data and Embedding
We've been trying to assess how big of an effect feed-down from secondary vertices have on our analysis. Some of our previous efforts can be found here:
Update [12.19.2019] -- Tracking Efficiencies for Decays On vs. Off in Run 9 Dijet Embedding Sample
Previously, I summarized our investigation of how to assess the systematic due to secondary vertices in our analysis:
Update [12.19.2019] -- Understanding Turning Decays On vs. Off in Run 9 Dijet Embedding Sample
One systematic uncertainties we need to assess in the neutral-triggered run 9 pp jet reconstruction analysis is the impact of secondary vertices on our measurement. The plot below shows the syst
Search for the Chiral Magnetic Effect in Au+Au collisions at 27 GeV with the STAR forward Event Plane Detectors
Title: Search for the Chiral Magnetic Effect in Au+Au collisions at $\sqrt{s_{_{\rm{NN}}}}=27$ GeV with the STAR forward Event Plane Detectors
pulser time difference in Gbtx
time difference of pulser digis within the same Gbtx (e.g. due to cables) compared to counter 1
variables:
STAR endcap TOF/CBM TOF meeting
The meeting is scheduled on Bluejeans: https://bluejeans.com/303776107, at 15:15 (GMT), duration : 02:00
STAR endcap TOF/CBM TOF meeting
The meeting is scheduled on Bluejeans: https://bluejeans.com/303776107, at 16:00 (GMT), duration : 02:00
STAR endcap TOF/CBM TOF meeting
The meeting is scheduled on Bluejeans: https://bluejeans.com/303776107, at 16:00 (GMT), duration : 02:00