STAR Correlations and Fluctuations PWG

[Hanna Paulina Zbroszczyk <hanna.zbroszczyk AT pw.edu.pl>]

Dear Risa,

Please find below comments to your nice proceedings:

Abstract:

heavy ion -> heavy-ion

at 200 GeV -> at \sqrt{s_{NN}} = 200 GeV

If you use p+p in the math mode, you should do the same for Au+Au (general comment to the whole draft)

Introduction:

at 200 GeV -> at \sqrt{s_{NN}} = 200 GeV

Cumulants:

Please control numbering of your references, the reference [16] should change the number as it is cited after [6-8]

Data set:

30 (cm) -> 30 cm

2 (cm) -> 2 cm

1 (cm) -> 1 cm

Results:

at 200 GeV -> at \sqrt{s_{NN}} = 200 GeV

Summary:

at 200 GeV -> at \sqrt{s_{NN}} = 200 GeV (when you refer to Au+Au)

at 200 GeV -> at \sqrt{s} = 200 GeV (when you refer to p+p)

at 200 GeV -> at \sqrt{s_{NN}} = 200 GeV (when you refer to Au+Au)

With those implemented I sign off.

Thanks,

Hanna

Hanna Paulina Zbroszczyk

PhD DSc Eng, Professor WUT

E-mail: hanna.zbroszczyk AT pw.edu.pl

Tel: +48 22 234 5851 (office)

Address:

Warsaw University of Technology

Faculty of Physics

Nuclear Physics Division

Koszykowa 75

Office: 117b (via 115)

00-662 Warsaw, Poland

Wiadomość napisana przez webmaster--- via Star-cf-l <star-cf-l AT lists.bnl.gov> w dniu 03.09.2021, o godz. 04:01:

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

Risa Nishitani (s2312412 AT gmail.com) has submitted a material for a review,  
please have a look:
https://drupal.star.bnl.gov/STAR/node/56188

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