STAR Flow, Chirality and Vorticity PWG

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

Dear Xiaoyu,

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

s#2: "Problems to solve" --> Do you mean these potential issues in v1 
analysis using EPD?
Then, I suggest a rephrase "Potential issues in v1 measurement"

s#3: Correct the typo in title.
Resolution figure: Could you add Psi_1 resolution, add beam energy and 
data set.

s#5: Could you indicate where Mip enters into v1 calculation, as a 
weight?

s#6,7,8: Could you add beam energy, dataset on the figure. Add  Y-axis 
label for the bottom panels.

s#8-9: After the iteration steps, is there tolerance level to choose 
v1_output = v1_meas, I mean do you require them to be identical or 
within a tolerance limit e.g. ~ 5% level.

s#9: These figures and legends hard to read. Could you enlarge them?

s#11: Comparison with PHOBOS

s#12: "Problems solved" --> I suggest "Issues addressed"
It would be good to add v1(eta) measured within 10 units in rapidity (~ 
+/-5)

Outlook: Instead of 19.6 GeV, I would suggest other BES-II energies.

Thanks and regards,
Subhash


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