STAR Flow, Chirality and Vorticity PWG

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Dear star-fcv-l AT lists.bnl.gov members,

Subhash Singha ( connectsubhash AT gmail.com ) has commented on a material  
originally submitted by ChunJian Zhang ( chunjianzhang AT fudan.edu.cn ) at
https://drupal.star.bnl.gov/STAR/presentations/INPC-2025/Imaging-shapes-atomic-nuclei-high-energy-nuclear-collisions-STAR-experiment

Comment:
Dear Chunjian,

Very nice abstract. I sign off with two minor suggestions:
It might be good to mention the exact method used e.g. flow-momentum  
correlation or Pearson correlations etc around line#4
l#12: it is not clear what are you going to show in O+O,  is it the same  
flow-momentum correlations or v2/e2 comparison with different IC models, may  
be you can rephrase accordingly.


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