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star-cf-l - Re: [Star-cf-l] STAR presentation by Pawel Szymanski for HYP 2022 submitted for review

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Subject: STAR Correlations and Fluctuations PWG

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  • From: Xiaofeng Luo <xfluo.star AT hotmail.com>
  • To: webmaster--- via Star-cf-l <star-cf-l AT lists.bnl.gov>
  • Subject: Re: [Star-cf-l] STAR presentation by Pawel Szymanski for HYP 2022 submitted for review
  • Date: Sat, 18 Jun 2022 23:41:33 +0800

Hi Pawel,

    Nice poster.
    Please find my comments/suggestions:

    1. I suggest to plot dE/dx of all particle together without applying Nsigma cut and also plottng theoretical dE/dx curve on the bands.
    2. You may mention somewhere that only statistical errors are presented for correlation functions.
    3. You mention "𝐶+(𝑘 ∗ ) – first (lighter) particle is faster,  𝐶−(𝑘 ∗ ) – second (heavier) particle is faster "
         Could you explain more about these conclusion ?

   4. Please define the radius R in the poster. It is the Y-axis title of the left figure in the results part.
       Please write some captions for the figures. and label the order of the figure, such as Fig. 1, 2.

    5. For the band on the data points in R and mu. Are those systematic errors ?
        If it is so, please mention somewhere in the poster. and how it is evaluated ?

Thank you,
Best Regards,
Xiaofeng

On 2022/6/10 15:30, webmaster--- via Star-cf-l wrote:
Dear star-cf-l AT lists.bnl.gov members,

Pawel Szymanski (pawszy91 AT gmail.com) has submitted a material for a review,
please have a look:
https://drupal.star.bnl.gov/STAR/node/59924

---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
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Xiaofeng Luo
Professor of Physics
College of Physical Science and Technology
Central China Normal University
Luoyu Road 152, Wuhan China
Office Phone #: +86-27-67867500





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