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 Junyi Han ( jyhan AT mails.ccnu.edu.cn ) at
https://drupal.star.bnl.gov/STAR/presentations/SQM-2024/Directed-Flow-Hyper-Nuclei-High-Baryon-Density-STAR

Comment:
Hi Junyi,
Nice slides. I have a few comments for your consideration:
s#1: we usually have a DOE support logo in all STAR talks.
s#3: "difficulty to reconcile" -->Â difficult to reconcile
s#4: "helps to explore" -->Â help explore
s#5:Â considered as a sensitive
s#8: Events --> Analyzed events (?)I think it is the number of good/accepted  
events, right? You can consider adding a reference of flow method paper
s#12: You may write the right bottom blue equation math form like you have in 
 
the left
s#13: Is the v1 fitting range same for all particles, it might be good to  
indicate.
You do not have "p0" in the linear equations inside the table, pls correct it
s#16: I suggest "high baryon density in STAR" --> for sNN = X.X - X.X GeV in 
 
STAR (at high baryon density)
You can remove "in 3.0 – 4.5 GeV collisions" in the 2nd bullet

I sign-off with these being addressed.

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