STAR Flow, Chirality and Vorticity PWG

[subhash <subhash AT rcf.rhic.bnl.gov>]

Dear Li-Ke,

Nice slides. I have few suggestions for your consideration.

slide#4: "v2 can provide effective degree of freedom" --> Do you mean 
partonic/hadronic degrees of freedom?
are less affected by  ...
Can you also add some references for small cross-section, earlier 
freeze-outs etc.

slide#5: Can you be specific what do you mean by "Better track quality"?

slide#6: Can you increase font size inside figures, they are small.

slide#7: Do you want to point out any improvement in PID performance in 
BES-II compared to BES-I?

slide#8: In general legends are small to read the details, can you 
enlarge them?
Can you add either 2019 data or BES-II inside these figures?
Can you point out any improvement in signal/background improvement in 
BES-II relative to BES-I?

slide#9&10: Add either 2019 data or BES-II inside these figures
"Event-by-event fluctuation dominant" --> Do you mean originated 
dominant from event-by-event fluctuations?

slide#11; Can you add any statement on improvement in precision of NCQ 
scaling in BES-II relative to BES-I?

slide#12: "NCQ scaling of v2 observed" --> Seems not true for 0-80%. 
Suggest to rephrase the sentence.

Thanks and regards,
Subhash




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