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Strange Luminosity Dependence in 19.6 GeV 2019

 I presented at the Tuesday Centrality meeting (10/5/21) that <refMult> vs. ZdcCoincidenceRate had a positive slope. We expect luminosity dependence to have a negative slope.

Preliminary Figures for APS DNP 2021

 

Determing the Light Quark Diffusivity of the QGP

 

Preliminary results (2021 DNP meeting)

Fig.1 Give the v2-pT correlations for different beam energies.

Fig.2 Give the G2 (\Delta\phi) correlation function for different centrality

Update on elliptic and triangular flow of multi-strange hadrons at 54.4 GeV at STAR

 

Why Event plane distribution is not flat after phi weighting? Why do we need Psi-shifting?

  • phi-weighting: weight the track so that the phi distribution is flat.  
  1. Fill a TH1D of phi distribution: PhiDis->Fill(phi)

Weekly Meeting (Oct 5th, 2021)

 - Xiaoxuan: comments from Institute Review
 - Xilin: update on simulation results

3D STAR Detector

These plots are generated using the 3D open source software: Blender.

The parameters used are based on the plots made by Tai Sakuma: 

Azimuthal Partition Preliminary Request

 

TPC SC&GL Calibration: Run19 AuAu 200 GeV

This document summarize the space charge and grid leak calibration for Run 19 AuAu 200 GeV dataset.