STAR Flow, Chirality and Vorticity PWG

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

Dear Rishabh,

Nice slides. I have a few suggestions for your consideration:

s#4: This is for my understanding, how light nuclei v3 of has better 
sensitivity to initial fluctuation, if they are formed at later stage?

s#9: Could you indicate the fraction of reduction in error in BES-II 
relative to BES-I?

s#14: At the lowest pT, I see v3 of p and d are consistent. It might be 
better if you specify the pt-range for which mass dependence is 
observed.

s#15: You can indicate fit to proton data beside the function in the 
legend.
The Y-axis scale of the bottom panels is very large, can you try 
reducing them, so the level of scaling would be clearly visible.


Thanks and regsrds,
Subhash


On 2023-08-24 10:01 PM, webmaster--- via Star-fcv-l wrote:
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