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 Gaoguo Yan ( gaoguo.yan AT Outlook.com ) at
https://drupal.star.bnl.gov/STAR/presentations/ATHIC-2023/Longitudinal-De-correlation-Anisotropic-Flow-RHIC-STAR-0

Comment:
Dear Gaoguo, Nice slides. It seems I Drupal missed your email. Sorry about  
that. I am signing off and sending your contribution to star-talks with a few 
 
minor comments:

s#6: Can you please check the formatting of the figures, In my screen I see  
some additional boarder lines around the figures.

Beam Energy Scans --> Beam Energy Scan

s#7: Better event plane resolution

s#12: Clear energy dependence --> Indication of energy dependence
I think hard to conclude on energy dependence considering error bars.

s#13:
Do you mean  "...between forward and backward directions"?

Longitudinal de-correlation in smaller collisions system is expected to be  
larger

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