STAR Flow, Chirality and Vorticity PWG

[Takafumi Niida <niida AT bnl.gov>]

Dear Chunjian,

I’m asked by STAR management to have a look at a few posters including yours. 
Please find my comments to your nice poster for your consideration.

“for the STAR Collaboration”: Only “Collaboration” looks italic.

Observables
- Only “Kurtosis” starts with capital letter while “mean” and others don’t. 
Nice to be consistent in style.
- Please consider to make these formula a bit larger as you have some space 
in the right.

Results in U+U and Au+Au
- Enhancement of v_{2,U}/v_{2,Au} is due to combined effects of the larger…
How about mid-central? If you mean only very central, consider to add “in 
most central collisions” before “is due to” above.

Results in Ru+Ru and Zr+Zr
- “<v2>^{1/2} — ratio”, “<v3>^{1/2} — ratio”: Is this true? Do you mean 
{v2^2}^{1/2}? At least the legend says “v2,Ru / v2,Zr”.

Conclusions
- assistant -> assists
- many-nucleon -> many-body nucleon?
- It seems that suddenly the words "gluon saturation and nPDF” appear and it 
wasn’t clear how these measurements are useful to understand them. It would 
be helpful if you can add a brief explanation or reference(s).

Bottom-left: change to “Supported in part by"

Best regards,
Takafumi

> On Aug 25, 2023, at 5:38, webmaster--- via Star-fcv-l 
> <star-fcv-l AT lists.bnl.gov> wrote:
> 
> Dear star-fcv-l AT lists.bnl.gov members,
> 
> ChunJian Zhang (czhang.phys AT gmail.com) has submitted a material for a 
> review,  
> please have a look:
> https://drupal.star.bnl.gov/STAR/node/64861
> 
> Deadline: 2023-09-03
> ---
> If you have any problems with the review process, please contact  
> webmaster AT www.star.bnl.gov
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