STAR Flow, Chirality and Vorticity PWG

[webmaster AT star.bnl.gov]

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

Subhash Singha ( connectsubhash AT gmail.com ) has commented on a material  
originally submitted by Muhammad Farhan Taseer ( mfarhan_taseer AT yahoo.com )  
at
https://drupal.star.bnl.gov/STAR/presentations/SQM-2024/Measurement-charge-dependent-directed-flow-STAR-Beam-Energy-Scan-BES-II-AuA-2

Comment:
Dear Farhan,

Nice proceedings. For record, I sign off with following additional  
suggestions.

l#43: in Au+Au collisions --> in peripheral Au+Au collisions

The X-axis in Fig-4 should be smaller case p_{T}

l#77: "is observed at lower BES-II energies (7.7 – 19.6 GeV) in Au+Au  
collisions"
--> is observed in BES-II Au+Au collisions at s_NN = 7.7 – 19.6 GeV.

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