STAR Correlations and Fluctuations PWG

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

Xin Dong ( xdong AT lbl.gov ) has commented on a material originally submitted  
by Jin Wu ( wj2016113394 AT mails.ccnu.edu.cn ) at
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2022/Measurement-Intermittency-Charged-Particles-Au-Au-Collisions-sqrts-0

Comment:
Hi Jin,
Thank you for addressing my comments and answering my questions. I only have  
a couple of more suggestions to the newly added beta_q vs. q figure.
1) It will be better to make the plot in a linear scale and not apply many  
folds of scaling factors. You want to reveal the power law dependence, but  
currently it is hard to see any dependence. You may just add a shift to  
different energies or make the plot in multiple panels. 
2) If you prefer to leave the figure on Slide 5, the last statement on Slide  
4 should be attached here.
3) Slide 5, It will be better to enlarge these figures a bit more so they are 
 
more readable, while you may move down the texts a bit and make them more  
concise, for example     " Scaling exponent vs. collision energy:   
 non-monotonic behavior in central collisions / flat distribution for 30-40% 
 
centrality collisions.       Scaling exponent vs. centrality:     
decrease from mid-central to central collisions.       Model studies /  
theory input to understand the baseline and the observed energy/centrality  
dependence."
Thank you and Best Regards
/xin

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