STAR Correlations and Fluctuations PWG

[Xiaofeng Luo <xfluo.star AT hotmail.com>]

Dear Dylan,

    Nice presentation.

    Since your slides only show results from AMPT and no STAR data yet, 
please find my minor suggestions/comment:

    1. It would be nice if you can prepare a slide to show the physics 
motivation of this analysis.
        For example, search for baryon clustering induced by CP ?

    2. It would be nice if you can have a slide to describe the AMPT 
model (default or string melting ?) and event statistics you used for each
        energy.

    3. In slide 8 and other slides, I see caps on the error bars, what 
is that ? systematic uncertainties ? But those are from model 
calculations and should have no systematic errors. I would be nice you 
have formula definition of kurtosis here. And how did you calculate the 
statistic errors, reference  ?

    4. I suggest to put "AMPT model" in figures, otherwise people may 
think it is STAR BES data.

    5. Did you try more bins rather than 3 bins ? It would be good you 
can compare results from different bin size.

    With those implemented, I sign off.
    Looking forward your nice results from STAR BES data in future PWG 
meeting.


Thank you,
Best Regards,
Xiaofeng

On 2020/10/15 2:32 PM, webmaster--- via Star-cf-l wrote:
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> https://drupal.star.bnl.gov/STAR/node/52378
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