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 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 comments:

Style of referring can be unified, eg s#3 is different than others;
s#2: reference to flow paper can be included; If Psi_n is event plane, then  
there will be a resolution factor;
s#4: # of accepted events or good events; Please also mention your vertex  
selections; There are other analysis using wider vertex selection reports a  
different # of events at these energies;
s#5: resolution formula should be different, right? strictly you are not  
calculating it simply by sqrt<cos (a-b)>;
s#6: If the v_2 is not corrected for resolution, it should be v_2^observed;
s#12,13: We have a clear breaking of NCQ at 3.2 GeV; It may be mentioned or  
the recent QM2023 preliminary plot may be added for completeness;
s#13: You start with a motivation about phi meson NCQ scaling breaking below  
19.6 GeV in BES-I; I think you can emphasize that \phi participated in  
scaling up to 14.6 GeV as a sub-bullet;


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