STAR Flow, Chirality and Vorticity PWG

[webmaster AT star.bnl.gov]

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

Zhenyu Chen ( zhenyuchen AT sdu.edu.cn ) has commented on a material originally  
submitted by Prabhupada Dixit ( prabhupadad AT iiserbpr.ac.in ) at
https://drupal.star.bnl.gov/STAR/presentations/Dynamics-QCD-2023/Azimuthal-anisotropic-flow-identified-hadrons-Au-Au-collisions-BES-I

Comment:
Dear Prabhupada,

Nice slides. I sign off with a few suggestions:
- Slide3: it's better to add a reference for quark coalescence model
- Slide4: lower left, move "iTPC upgrades" to "BESII with iTPC upgrades" in  
red
- Slide5-6: title, Analysis details -> Analysis techniques
- Slide6: would be good to show a invariant mass fit for Kshort, otherwise S  
and B become un-defined
- Slide7: statistical errors -> statistical uncertainties
- Slide12: I would not say partonice collectivity is absolutely not there, it 
 
could be a small contribution. I suggest to change the sentence to something  
like "hadronic collectivity dominates"

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